2MASS Second Incremental Data Release Explanatory Supplement: Release Contents

Column Descriptions for the 2MASS Second Incremental Release Extended Source Catalog (XSC)

Column #	Column Name	Description	Units	Bytes	Format^a	Nulls Allowed
1	hemis	hemisphere (N/S) of observation	---	5	5s	n
2	date	observation date	---	8-13	6s	n
3	scan	scan number (unique within date)	---	15-18	4hd	n
4	coadd	3-digit coadded atlas image number (unique within scan)	---	20-23	4hd	n
5	id	source ID number (unique within scan, image)	---	25-28	4d	n
6	ra	right ascension (J2000 decimal deg) based on peak pixel	deg	30-39	10.6f	n
7	dec	declination (J2000 decimal deg) based on peak pixel	deg	41-50	10.6f	n
8	glon	galactic longitude (decimal deg) based on peak pixel	deg	52-61	10.6f	n
9	glat	galactic latitude (decimal deg) based on peak pixel	deg	63-72	10.6f	n
10	designation	source designation formed from sexigesimal coordinates	---	74-87	14s	n
	Notes for designation: This is the object sequence designation, or object "name" as specified by the IAU recommendations on source nomenclature. It is derived from the J2000 sexigesimal coordinates of the source and has the form HHMMSSS+/-DDMMSS, where HH are the hours of right ascension, MM the RA minutes and SSS are the deci-seconds of RA. DD are the degrees in declination, MM are DEC minutes and SS the declination seconds. Note that both the RA deci-seconds of time and DEC seconds of arc are truncated rather than rounded, per the IAU recommendation.
11	x_coadd	x (cross-scan) position (image coord.)	arcsec	89-93	5.1f	n
12	y_coadd	y (in-scan) position (image coord.)	arcsec	95-100	6.1f	n
13	r_3sig	3-sigma K isophotal semi-major axis	arcsec	102-106	5.1f	y
14	j_ba	J minor/major axis ratio fit to the 3-sigma isophote	---	108-112	5.3f	y
15	h_ba	H minor/major axis ratio fit to the 3-sigma isophote	---	114-118	5.3f	y
16	k_ba	K minor/major axis ratio fit to the 3-sigma isophote	---	120-124	5.3f	y
17	j_phi	J angle to 3-sigma major axis (E of N)	deg	126-129	4hd	y
18	h_phi	H angle to 3-sigma major axis (E of N)	deg	131-134	4hd	y
19	k_phi	K angle to 3-sigma major axis (E of N)	deg	136-139	4hd	y
20	j_m	J selected "default" magnitude	mag	141-146	6.3f	y
	Notes for j_m: This is the selected "default" magnitude for each band. The first choice for the [jhk]_m values are the mags in each band at 20 mag/sq.arcsec w/K fiducial circular aperture ([jhk]_m_k20fc), indicated by [jhk]_mtype values of 0. If, however, the K band mag in this group is > 14.0 (including negative flux or no mag found), all 3 [jhk]_m values will be the mags at 21 mag/sq.arcsec w/J fiducial circular aperture ([jhk]_m_j21fc) and the flags [jhk]_mtype are set to 1. If any one of chosen set of "default" mags is > 99, indicating no mag found, the DB entry for that "default" mag will be set to NULL. Thus, the [jhk]_mtype flags will indicate the source of the "default" mags and sigmas as follows: 0: [jhk]_m_k20fe values 1: [jhk]_m_j21fe values
21	h_m	H selected "default" magnitude	mag	148-153	6.3f	y
	Notes for h_m: This is the selected "default" magnitude for each band. The first choice for the [jhk]_m values are the mags in each band at 20 mag/sq.arcsec w/K fiducial circular aperture ([jhk]_m_k20fc), indicated by [jhk]_mtype values of 0. If, however, the K band mag in this group is > 14.0 (including negative flux or no mag found), all 3 [jhk]_m values will be the mags at 21 mag/sq.arcsec w/J fiducial circular aperture ([jhk]_m_j21fc) and the flags [jhk]_mtype are set to 1. If any one of chosen set of "default" mags is > 99, indicating no mag found, the DB entry for that "default" mag will be set to NULL. Thus, the [jhk]_mtype flags will indicate the source of the "default" mags and sigmas as follows: 0: [jhk]_m_k20fe values 1: [jhk]_m_j21fe values
22	k_m	K selected "default" magnitude	mag	155-160	6.3f	y
	Notes for k_m: This is the selected "default" magnitude for each band. The first choice for the [jhk]_m values are the mags in each band at 20 mag/sq.arcsec w/K fiducial circular aperture ([jhk]_m_k20fc), indicated by [jhk]_mtype values of 0. If, however, the K band mag in this group is > 14.0 (including negative flux or no mag found), all 3 [jhk]_m values will be the mags at 21 mag/sq.arcsec w/J fiducial circular aperture ([jhk]_m_j21fc) and the flags [jhk]_mtype are set to 1. If any one of chosen set of "default" mags is > 99, indicating no mag found, the DB entry for that "default" mag will be set to NULL. Thus, the [jhk]_mtype flags will indicate the source of the "default" mags and sigmas as follows: 0: [jhk]_m_k20fe values 1: [jhk]_m_j21fe values
23	j_msig	J "default" mag uncertainty	mag	162-166	5.3f	y
	Notes for j_msig: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
24	h_msig	H "default" mag uncertainty	mag	168-172	5.3f	y
	Notes for h_msig: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
25	k_msig	K "default" mag uncertainty	mag	174-178	5.3f	y
	Notes for k_msig: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
26	j_flg	J confusion flag for "default" magnitude	---	180-183	4hd	y
	Notes for j_flg: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
27	h_flg	H confusion flag for "default" magnitude	---	185-188	4hd	y
	Notes for h_flg: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
28	k_flg	K confusion flag for "default" magnitude	---	190-193	4hd	y
	Notes for k_flg: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
29	j_mtype	source of J "default" mag (0=j_m_k20fc, 1=j_m_j21fc)	---	195-198	4hd	n
30	h_mtype	source of H "default" mag (0=h_m_k20fc, 1=h_m_j21fc)	---	200-203	4hd	n
31	k_mtype	source of K "default" mag (0=k_m_k20fc, 1=k_m_j21fc)	---	205-208	4hd	n
32	j_r_e	J Kron elliptical aperture semi-major axis	arcsec	210-214	5.1f	y
33	h_r_e	H Kron elliptical aperture semi-major axis	arcsec	216-220	5.1f	y
34	k_r_e	K Kron elliptical aperture semi-major axis	arcsec	222-226	5.1f	y
35	j_m_e	J Kron elliptical aperture magnitude	mag	228-233	6.3f	y
36	h_m_e	H Kron elliptical aperture magnitude	mag	235-240	6.3f	y
37	k_m_e	K Kron elliptical aperture magnitude	mag	242-247	6.3f	y
38	j_msig_e	J 1-sigma uncertainty in Kron elliptical mag	mag	249-253	5.3f	y
	Notes for j_msig_e: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
39	h_msig_e	H 1-sigma uncertainty in Kron elliptical mag	mag	255-259	5.3f	y
	Notes for h_msig_e: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
40	k_msig_e	K 1-sigma uncertainty in Kron elliptical mag	mag	261-265	5.3f	y
	Notes for k_msig_e: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
41	j_flg_e	J confusion flag for Kron elliptical mag	---	267-270	4hd	y
	Notes for j_flg_e: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
42	h_flg_e	H confusion flag for Kron elliptical mag	---	272-275	4hd	y
	Notes for h_flg_e: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
43	k_flg_e	K confusion flag for Kron elliptical mag	---	277-280	4hd	y
	Notes for k_flg_e: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
44	r_fe	K fiducial Kron elliptical aperture semi-major axis	arcsec	282-286	5.1f	y
	Notes for r_fe: "Fiducial" apertures are determined for each type of total and isophotal photometry measurements as described in the GALWORKS SDS. Essentially, they are used to make mag measurements for each type of photometry with the same aperture size in all three bands. The fiducial band for the total Kron photometry and 20mag/sq." isophotal photometry is the K band, and for the 21mag/sq." isophotal photometry it is the J band.
45	j_m_fe	J fiducial Kron elliptical aperture magnitude	mag	288-293	6.3f	y
46	h_m_fe	H fiducial Kron elliptical aperture magnitude	mag	295-300	6.3f	y
47	k_m_fe	K fiducial Kron elliptical aperture magnitude	mag	302-307	6.3f	y
48	j_msig_fe	J 1-sigma uncertainty in fiducial Kron ell. mag	mag	309-313	5.3f	y
	Notes for j_msig_fe: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
49	h_msig_fe	H 1-sigma uncertainty in fiducial Kron ell. mag	mag	315-319	5.3f	y
	Notes for h_msig_fe: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
50	k_msig_fe	K 1-sigma uncertainty in fiducial Kron ell. mag	mag	321-325	5.3f	y
	Notes for k_msig_fe: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
51	j_flg_fe	J confusion flag for fiducial Kron ell. mag	---	327-330	4hd	y
	Notes for j_flg_fe: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
52	h_flg_fe	H confusion flag for fiducial Kron ell. mag	---	332-335	4hd	y
	Notes for h_flg_fe: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
53	k_flg_fe	K confusion flag for fiducial Kron ell. mag	---	337-340	4hd	y
	Notes for k_flg_fe: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
54	j_r_c	J Kron circular aperture radius	arcsec	342-346	5.1f	y
55	h_r_c	H Kron circular aperture radius	arcsec	348-352	5.1f	y
56	k_r_c	K Kron circular aperture radius	arcsec	354-358	5.1f	y
57	j_m_c	J Kron circular aperture magnitude	mag	360-365	6.3f	y
58	h_m_c	H Kron circular aperture magnitude	mag	367-372	6.3f	y
59	k_m_c	K Kron circular aperture magnitude	mag	374-379	6.3f	y
60	j_msig_c	J 1-sigma uncertainty in Kron circular mag	mag	381-385	5.3f	y
	Notes for j_msig_c: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
61	h_msig_c	H 1-sigma uncertainty in Kron circular mag	mag	387-391	5.3f	y
	Notes for h_msig_c: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
62	k_msig_c	K 1-sigma uncertainty in Kron circular mag	mag	393-397	5.3f	y
	Notes for k_msig_c: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
63	j_flg_c	J confusion flag for Kron circular mag	---	399-402	4hd	y
	Notes for j_flg_c: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
64	h_flg_c	H confusion flag for Kron circular mag	---	404-407	4hd	y
	Notes for h_flg_c: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
65	k_flg_c	K confusion flag for Kron circular mag	---	409-412	4hd	y
	Notes for k_flg_c: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
66	r_fc	K fiducial Kron circular aperture radius	arcsec	414-418	5.1f	y
	Notes for r_fc: "Fiducial" apertures are determined for each type of total and isophotal photometry measurements as described in the GALWORKS SDS. Essentially, they are used to make mag measurements for each type of photometry with the same aperture size in all three bands. The fiducial band for the total Kron photometry and 20mag/sq." isophotal photometry is the K band, and for the 21mag/sq." isophotal photometry it is the J band.
67	j_m_fc	J fiducial Kron circular magnitude	mag	420-425	6.3f	y
68	h_m_fc	H fiducial Kron circular magnitude	mag	427-432	6.3f	y
69	k_m_fc	K fiducial Kron circular magnitude	mag	434-439	6.3f	y
70	j_msig_fc	J 1-sigma uncertainty in fiducial Kron circ. mag	mag	441-445	5.3f	y
	Notes for j_msig_fc: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
71	h_msig_fc	H 1-sigma uncertainty in fiducial Kron circ. mag	mag	447-451	5.3f	y
	Notes for h_msig_fc: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
72	k_msig_fc	K 1-sigma uncertainty in fiducial Kron circ. mag	mag	453-457	5.3f	y
	Notes for k_msig_fc: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
73	j_flg_fc	J confusion flag for fiducial Kron circ. mag	---	459-462	4hd	y
	Notes for j_flg_fc: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
74	h_flg_fc	H confusion flag for fiducial Kron circ. mag	---	464-467	4hd	y
	Notes for h_flg_fc: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
75	k_flg_fc	K confusion flag for fiducial Kron circ. mag	---	469-472	4hd	y
	Notes for k_flg_fc: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
76	j_r_i20e	J 20mag/sq." isophotal elliptical ap. semi-major axis	arcsec	474-478	5.1f	y
77	h_r_i20e	H 20mag/sq." isophotal elliptical ap. semi-major axis	arcsec	480-484	5.1f	y
78	k_r_i20e	K 20mag/sq." isophotal elliptical ap. semi-major axis	arcsec	486-490	5.1f	y
79	j_m_i20e	J 20mag/sq." isophotal elliptical ap. magnitude	mag	492-497	6.3f	y
80	h_m_i20e	H 20mag/sq." isophotal elliptical ap. magnitude	mag	499-504	6.3f	y
81	k_m_i20e	K 20mag/sq." isophotal elliptical ap. magnitude	mag	506-511	6.3f	y
82	j_msig_i20e	J 1-sigma uncertainty in 20mag/sq." iso. ell. mag	mag	513-517	5.3f	y
	Notes for j_msig_i20e: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
83	h_msig_i20e	H 1-sigma uncertainty in 20mag/sq." iso. ell. mag	mag	519-523	5.3f	y
	Notes for h_msig_i20e: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
84	k_msig_i20e	K 1-sigma uncertainty in 20mag/sq." iso. ell. mag	mag	525-529	5.3f	y
	Notes for k_msig_i20e: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
85	j_flg_i20e	J confusion flag for 20mag/sq." iso. ell. mag	---	531-534	4hd	y
	Notes for j_flg_i20e: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
86	h_flg_i20e	H confusion flag for 20mag/sq." iso. ell. mag	---	536-539	4hd	y
	Notes for h_flg_i20e: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
87	k_flg_i20e	K confusion flag for 20mag/sq." iso. ell. mag	---	541-544	4hd	y
	Notes for k_flg_i20e: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
88	r_k20fe	20mag/sq." isophotal K fiducial ell. ap. semi-major axis	arcsec	546-550	5.1f	y
	Notes for r_k20fe: "Fiducial" apertures are determined for each type of total and isophotal photometry measurements as described in the GALWORKS SDS. Essentially, they are used to make mag measurements for each type of photometry with the same aperture size in all three bands. The fiducial band for the total Kron photometry and 20mag/sq." isophotal photometry is the K band, and for the 21mag/sq." isophotal photometry it is the J band.
89	j_m_k20fe	J 20mag/sq." isophotal fiducial ell. ap. magnitude	mag	552-557	6.3f	y
90	h_m_k20fe	H 20mag/sq." isophotal fiducial ell. ap. magnitude	mag	559-564	6.3f	y
91	k_m_k20fe	K 20mag/sq." isophotal fiducial ell. ap. magnitude	mag	566-571	6.3f	y
92	j_msig_k20fe	J 1-sigma uncertainty in 20mag/sq." iso.fid.ell.mag	mag	573-577	5.3f	y
	Notes for j_msig_k20fe: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
93	h_msig_k20fe	H 1-sigma uncertainty in 20mag/sq." iso.fid.ell.mag	mag	579-583	5.3f	y
	Notes for h_msig_k20fe: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
94	k_msig_k20fe	K 1-sigma uncertainty in 20mag/sq." iso.fid.ell.mag	mag	585-589	5.3f	y
	Notes for k_msig_k20fe: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
95	j_flg_k20fe	J confusion flag for 20mag/sq." iso. fid. ell. mag	---	591-594	4hd	y
	Notes for j_flg_k20fe: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
96	h_flg_k20fe	H confusion flag for 20mag/sq." iso. fid. ell. mag	---	596-599	4hd	y
	Notes for h_flg_k20fe: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
97	k_flg_k20fe	K confusion flag for 20mag/sq." iso. fid. ell. mag	---	601-604	4hd	y
	Notes for k_flg_k20fe: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
98	j_r_i20c	J 20mag/sq." isophotal circular aperture radius	arcsec	606-610	5.1f	y
99	h_r_i20c	H 20mag/sq." isophotal circular aperture radius	arcsec	612-616	5.1f	y
100	k_r_i20c	K 20mag/sq." isophotal circular aperture radius	arcsec	618-622	5.1f	y
101	j_m_i20c	J 20mag/sq." isophotal circular ap. magnitude	mag	624-629	6.3f	y
102	h_m_i20c	H 20mag/sq." isophotal circular ap. magnitude	mag	631-636	6.3f	y
103	k_m_i20c	K 20mag/sq." isophotal circular ap. magnitude	mag	638-643	6.3f	y
104	j_msig_i20c	J 1-sigma uncertainty in 20mag/sq." iso. circ. mag	mag	645-649	5.3f	y
	Notes for j_msig_i20c: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
105	h_msig_i20c	H 1-sigma uncertainty in 20mag/sq." iso. circ. mag	mag	651-655	5.3f	y
	Notes for h_msig_i20c: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
106	k_msig_i20c	K 1-sigma uncertainty in 20mag/sq." iso. circ. mag	mag	657-661	5.3f	y
	Notes for k_msig_i20c: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
107	j_flg_i20c	J confusion flag for 20mag/sq." iso. circ. mag	---	663-666	4hd	y
	Notes for j_flg_i20c: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
108	h_flg_i20c	H confusion flag for 20mag/sq." iso. circ. mag	---	668-671	4hd	y
	Notes for h_flg_i20c: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
109	k_flg_i20c	K confusion flag for 20mag/sq." iso. circ. mag	---	673-676	4hd	y
	Notes for k_flg_i20c: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
110	r_k20fc	20mag/sq." isophotal K fiducial circular ap. radius	arcsec	678-682	5.1f	y
	Notes for r_k20fc: "Fiducial" apertures are determined for each type of total and isophotal photometry measurements as described in the GALWORKS SDS. Essentially, they are used to make mag measurements for each type of photometry with the same aperture size in all three bands. The fiducial band for the total Kron photometry and 20mag/sq." isophotal photometry is the K band, and for the 21mag/sq." isophotal photometry it is the J band.
111	j_m_k20fc	J 20mag/sq." isophotal fiducial circ. ap. mag	mag	684-689	6.3f	y
112	h_m_k20fc	H 20mag/sq." isophotal fiducial circ. ap. mag	mag	691-696	6.3f	y
113	k_m_k20fc	K 20mag/sq." isophotal fiducial circ. ap. mag	mag	698-703	6.3f	y
114	j_msig_k20fc	J 1-sigma uncertainty in 20mag/sq." iso.fid.circ. mag	mag	705-709	5.3f	y
	Notes for j_msig_k20fc: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
115	h_msig_k20fc	H 1-sigma uncertainty in 20mag/sq." iso.fid.circ. mag	mag	711-715	5.3f	y
	Notes for h_msig_k20fc: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
116	k_msig_k20fc	K 1-sigma uncertainty in 20mag/sq." iso.fid.circ. mag	mag	717-721	5.3f	y
	Notes for k_msig_k20fc: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
117	j_flg_k20fc	J confusion flag for 20mag/sq." iso. fid. circ. mag	---	723-726	4hd	y
	Notes for j_flg_k20fc: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
118	h_flg_k20fc	H confusion flag for 20mag/sq." iso. fid. circ. mag	---	728-731	4hd	y
	Notes for h_flg_k20fc: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
119	k_flg_k20fc	K confusion flag for 20mag/sq." iso. fid. circ. mag	---	733-736	4hd	y
	Notes for k_flg_k20fc: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
120	j_r_i21e	J 21mag/sq." isophotal elliptical ap. semi-major axis	arcsec	738-742	5.1f	y
121	h_r_i21e	H 21mag/sq." isophotal elliptical ap. semi-major axis	arcsec	744-748	5.1f	y
122	k_r_i21e	K 21mag/sq." isophotal elliptical ap. semi-major axis	arcsec	750-754	5.1f	y
123	j_m_i21e	J 21mag/sq." isophotal elliptical ap. magnitude	mag	756-761	6.3f	y
124	h_m_i21e	H 21mag/sq." isophotal elliptical ap. magnitude	mag	763-768	6.3f	y
125	k_m_i21e	K 21mag/sq." isophotal elliptical ap. magnitude	mag	770-775	6.3f	y
126	j_msig_i21e	J 1-sigma uncertainty in 21mag/sq." iso. ell. mag	mag	777-781	5.3f	y
	Notes for j_msig_i21e: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
127	h_msig_i21e	H 1-sigma uncertainty in 21mag/sq." iso. ell. mag	mag	783-787	5.3f	y
	Notes for h_msig_i21e: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
128	k_msig_i21e	K 1-sigma uncertainty in 21mag/sq." iso. ell. mag	mag	789-793	5.3f	y
	Notes for k_msig_i21e: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
129	j_flg_i21e	J confusion flag for 21mag/sq." iso. ell. mag	---	795-798	4hd	y
	Notes for j_flg_i21e: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
130	h_flg_i21e	H confusion flag for 21mag/sq." iso. ell. mag	---	800-803	4hd	y
	Notes for h_flg_i21e: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
131	k_flg_i21e	K confusion flag for 21mag/sq." iso. ell. mag	---	805-808	4hd	y
	Notes for k_flg_i21e: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
132	r_j21fe	21mag/sq." isophotal J fiducial ell. ap. semi-major axis	arcsec	810-814	5.1f	y
	Notes for r_j21fe: "Fiducial" apertures are determined for each type of total and isophotal photometry measurements as described in the GALWORKS SDS. Essentially, they are used to make mag measurements for each type of photometry with the same aperture size in all three bands. The fiducial band for the total Kron photometry and 20mag/sq." isophotal photometry is the K band, and for the 21mag/sq." isophotal photometry it is the J band.
133	j_m_j21fe	J 21mag/sq." isophotal fiducial ell. ap. magnitude	mag	816-821	6.3f	y
134	h_m_j21fe	H 21mag/sq." isophotal fiducial ell. ap. magnitude	mag	823-828	6.3f	y
135	k_m_j21fe	K 21mag/sq." isophotal fiducial ell. ap. magnitude	mag	830-835	6.3f	y
136	j_msig_j21fe	J 1-sigma uncertainty in 21mag/sq." iso.fid.ell.mag	mag	837-841	5.3f	y
	Notes for j_msig_j21fe: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
137	h_msig_j21fe	H 1-sigma uncertainty in 21mag/sq." iso.fid.ell.mag	mag	843-847	5.3f	y
	Notes for h_msig_j21fe: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
138	k_msig_j21fe	K 1-sigma uncertainty in 21mag/sq." iso.fid.ell.mag	mag	849-853	5.3f	y
	Notes for k_msig_j21fe: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
139	j_flg_j21fe	J confusion flag for 21mag/sq." iso. fid. ell. mag	---	855-858	4hd	y
	Notes for j_flg_j21fe: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
140	h_flg_j21fe	H confusion flag for 21mag/sq." iso. fid. ell. mag	---	860-863	4hd	y
	Notes for h_flg_j21fe: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
141	k_flg_j21fe	K confusion flag for 21mag/sq." iso. fid. ell. mag	---	865-868	4hd	y
	Notes for k_flg_j21fe: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
142	j_r_i21c	J 21mag/sq." isophotal circular aperture radius	arcsec	870-874	5.1f	y
143	h_r_i21c	H 21mag/sq." isophotal circular aperture radius	arcsec	876-880	5.1f	y
144	k_r_i21c	K 21mag/sq." isophotal circular aperture radius	arcsec	882-886	5.1f	y
145	j_m_i21c	J 21mag/sq." isophotal circular ap. magnitude	mag	888-893	6.3f	y
146	h_m_i21c	H 21mag/sq." isophotal circular ap. magnitude	mag	895-900	6.3f	y
147	k_m_i21c	K 21mag/sq." isophotal circular ap. magnitude	mag	902-907	6.3f	y
148	j_msig_i21c	J 1-sigma uncertainty in 21mag/sq." iso. circ. mag	mag	909-913	5.3f	y
	Notes for j_msig_i21c: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
149	h_msig_i21c	H 1-sigma uncertainty in 21mag/sq." iso. circ. mag	mag	915-919	5.3f	y
	Notes for h_msig_i21c: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
150	k_msig_i21c	K 1-sigma uncertainty in 21mag/sq." iso. circ. mag	mag	921-925	5.3f	y
	Notes for k_msig_i21c: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
151	j_flg_i21c	J confusion flag for 21mag/sq." iso. circ. mag	---	927-930	4hd	y
	Notes for j_flg_i21c: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
152	h_flg_i21c	H confusion flag for 21mag/sq." iso. circ. mag	---	932-935	4hd	y
	Notes for h_flg_i21c: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
153	k_flg_i21c	K confusion flag for 21mag/sq." iso. circ. mag	---	937-940	4hd	y
	Notes for k_flg_i21c: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
154	r_j21fc	21mag/sq." isophotal J fiducial circular ap. radius	arcsec	942-946	5.1f	y
	Notes for r_j21fc: "Fiducial" apertures are determined for each type of total and isophotal photometry measurements as described in the GALWORKS SDS. Essentially, they are used to make mag measurements for each type of photometry with the same aperture size in all three bands. The fiducial band for the total Kron photometry and 20mag/sq." isophotal photometry is the K band, and for the 21mag/sq." isophotal photometry it is the J band.
155	j_m_j21fc	J 21mag/sq." isophotal fiducial circ. ap. mag	mag	948-953	6.3f	y
156	h_m_j21fc	H 21mag/sq." isophotal fiducial circ. ap. mag	mag	955-960	6.3f	y
157	k_m_j21fc	K 21mag/sq." isophotal fiducial circ. ap. mag	mag	962-967	6.3f	y
158	j_msig_j21fc	J 1-sigma uncertainty in 21mag/sq." iso.fid.circ.mag	mag	969-973	5.3f	y
	Notes for j_msig_j21fc: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
159	h_msig_j21fc	H 1-sigma uncertainty in 21mag/sq." iso.fid.circ.mag	mag	975-979	5.3f	y
	Notes for h_msig_j21fc: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
160	k_msig_j21fc	K 1-sigma uncertainty in 21mag/sq." iso.fid.circ.mag	mag	981-985	5.3f	y
	Notes for k_msig_j21fc: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
161	j_flg_j21fc	J confusion flag for 21mag/sq." iso. fid. circ. mag	---	987-990	4hd	y
	Notes for j_flg_j21fc: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
162	h_flg_j21fc	H confusion flag for 21mag/sq." iso. fid. circ. mag	---	992-995	4hd	y
	Notes for h_flg_j21fc: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
163	k_flg_j21fc	K confusion flag for 21mag/sq." iso. fid. circ. mag	---	997-1000	4hd	y
	Notes for k_flg_j21fc: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
164	j_r_ext	J extrapolation radius	arcsec	1002-1005	4.1f	y
165	h_r_ext	H extrapolation radius	arcsec	1007-1010	4.1f	y
166	k_r_ext	K extrapolation radius	arcsec	1012-1015	4.1f	y
167	j_m_ext	J mag from fit extrapolation	mag	1017-1022	6.3f	y
168	h_m_ext	H mag from fit extrapolation	mag	1024-1029	6.3f	y
169	k_m_ext	K mag from fit extrapolation	mag	1031-1036	6.3f	y
170	j_m_5	J 5 arcsec radius circular aperture magnitude	mag	1038-1043	6.3f	y
171	h_m_5	H 5 arcsec radius circular aperture magnitude	mag	1045-1050	6.3f	y
172	k_m_5	K 5 arcsec radius circular aperture magnitude	mag	1052-1057	6.3f	y
173	j_msig_5	J 1-sigma uncertainty in 5 arcsec circular ap. mag	mag	1059-1063	5.3f	y
	Notes for j_msig_5: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
174	h_msig_5	H 1-sigma uncertainty in 5 arcsec circular ap. mag	mag	1065-1069	5.3f	y
	Notes for h_msig_5: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
175	k_msig_5	K 1-sigma uncertainty in 5 arcsec circular ap. mag	mag	1071-1075	5.3f	y
	Notes for k_msig_5: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
176	j_flg_5	J confusion flag for 5 arcsec circular ap. mag	---	1077-1080	4hd	y
	Notes for j_flg_5: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
177	h_flg_5	H confusion flag for 5 arcsec circular ap. mag	---	1082-1085	4hd	y
	Notes for h_flg_5: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
178	k_flg_5	K confusion flag for 5 arcsec circular ap. mag	---	1087-1090	4hd	y
	Notes for k_flg_5: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
179	j_m_7	J 7 arcsec radius circular aperture magnitude	mag	1092-1097	6.3f	y
180	h_m_7	H 7 arcsec radius circular aperture magnitude	mag	1099-1104	6.3f	y
181	k_m_7	K 7 arcsec radius circular aperture magnitude	mag	1106-1111	6.3f	y
182	j_msig_7	J 1-sigma uncertainty in 7 arcsec circular ap. mag	mag	1113-1117	5.3f	y
	Notes for j_msig_7: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
183	h_msig_7	H 1-sigma uncertainty in 7 arcsec circular ap. mag	mag	1119-1123	5.3f	y
	Notes for h_msig_7: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
184	k_msig_7	K 1-sigma uncertainty in 7 arcsec circular ap. mag	mag	1125-1129	5.3f	y
	Notes for k_msig_7: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
185	j_flg_7	J confusion flag for 7 arcsec circular ap. mag	---	1131-1134	4hd	y
	Notes for j_flg_7: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
186	h_flg_7	H confusion flag for 7 arcsec circular ap. mag	---	1136-1139	4hd	y
	Notes for h_flg_7: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
187	k_flg_7	K confusion flag for 7 arcsec circular ap. mag	---	1141-1144	4hd	y
	Notes for k_flg_7: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
188	j_m_10	J 10 arcsec radius circular aperture magnitude	mag	1146-1151	6.3f	y
189	h_m_10	H 10 arcsec radius circular aperture magnitude	mag	1153-1158	6.3f	y
190	k_m_10	K 10 arcsec radius circular aperture magnitude	mag	1160-1165	6.3f	y
191	j_msig_10	J 1-sigma uncertainty in 10 arcsec circular ap. mag	mag	1167-1171	5.3f	y
	Notes for j_msig_10: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
192	h_msig_10	H 1-sigma uncertainty in 10 arcsec circular ap. mag	mag	1173-1177	5.3f	y
	Notes for h_msig_10: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
193	k_msig_10	K 1-sigma uncertainty in 10 arcsec circular ap. mag	mag	1179-1183	5.3f	y
	Notes for k_msig_10: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
194	j_flg_10	J confusion flag for 10 arcsec circular ap. mag	---	1185-1188	4hd	y
	Notes for j_flg_10: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
195	h_flg_10	H confusion flag for 10 arcsec circular ap. mag	---	1190-1193	4hd	y
	Notes for h_flg_10: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
196	k_flg_10	K confusion flag for 10 arcsec circular ap. mag	---	1195-1198	4hd	y
	Notes for k_flg_10: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
197	j_m_15	J 15 arcsec radius circular aperture magnitude	mag	1200-1205	6.3f	y
198	h_m_15	H 15 arcsec radius circular aperture magnitude	mag	1207-1212	6.3f	y
199	k_m_15	K 15 arcsec radius circular aperture magnitude	mag	1214-1219	6.3f	y
200	j_msig_15	J 1-sigma uncertainty in 15 arcsec circular ap. mag	mag	1221-1225	5.3f	y
	Notes for j_msig_15: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
201	h_msig_15	H 1-sigma uncertainty in 15 arcsec circular ap. mag	mag	1227-1231	5.3f	y
	Notes for h_msig_15: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
202	k_msig_15	K 1-sigma uncertainty in 15 arcsec circular ap. mag	mag	1233-1237	5.3f	y
	Notes for k_msig_15: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
203	j_flg_15	J confusion flag for 15 arcsec circular ap. mag	---	1239-1242	4hd	y
	Notes for j_flg_15: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
204	h_flg_15	H confusion flag for 15 arcsec circular ap. mag	---	1244-1247	4hd	y
	Notes for h_flg_15: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
205	k_flg_15	K confusion flag for 15 arcsec circular ap. mag	---	1249-1252	4hd	y
	Notes for k_flg_15: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
206	j_m_20	J 20 arcsec radius circular aperture magnitude	mag	1254-1259	6.3f	y
207	h_m_20	H 20 arcsec radius circular aperture magnitude	mag	1261-1266	6.3f	y
208	k_m_20	K 20 arcsec radius circular aperture magnitude	mag	1268-1273	6.3f	y
209	j_msig_20	J 1-sigma uncertainty in 20 arcsec circular ap. mag	mag	1275-1279	5.3f	y
	Notes for j_msig_20: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
210	h_msig_20	H 1-sigma uncertainty in 20 arcsec circular ap. mag	mag	1281-1285	5.3f	y
	Notes for h_msig_20: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
211	k_msig_20	K 1-sigma uncertainty in 20 arcsec circular ap. mag	mag	1287-1291	5.3f	y
	Notes for k_msig_20: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
212	j_flg_20	J confusion flag for 20 arcsec circular ap. mag	---	1293-1296	4hd	y
	Notes for j_flg_20: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
213	h_flg_20	H confusion flag for 20 arcsec circular ap. mag	---	1298-1301	4hd	y
	Notes for h_flg_20: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
214	k_flg_20	K confusion flag for 20 arcsec circular ap. mag	---	1303-1306	4hd	y
	Notes for k_flg_20: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
215	j_m_25	J 25 arcsec radius circular aperture magnitude	mag	1308-1313	6.3f	y
216	h_m_25	H 25 arcsec radius circular aperture magnitude	mag	1315-1320	6.3f	y
217	k_m_25	K 25 arcsec radius circular aperture magnitude	mag	1322-1327	6.3f	y
218	j_msig_25	J 1-sigma uncertainty in 25 arcsec circular ap. mag	mag	1329-1333	5.3f	y
	Notes for j_msig_25: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
219	h_msig_25	H 1-sigma uncertainty in 25 arcsec circular ap. mag	mag	1335-1339	5.3f	y
	Notes for h_msig_25: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
220	k_msig_25	K 1-sigma uncertainty in 25 arcsec circular ap. mag	mag	1341-1345	5.3f	y
	Notes for k_msig_25: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
221	j_flg_25	J confusion flag for 25 arcsec circular ap. mag	---	1347-1350	4hd	y
	Notes for j_flg_25: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
222	h_flg_25	H confusion flag for 25 arcsec circular ap. mag	---	1352-1355	4hd	y
	Notes for h_flg_25: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
223	k_flg_25	K confusion flag for 25 arcsec circular ap. mag	---	1357-1360	4hd	y
	Notes for k_flg_25: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
224	j_m_30	J 30 arcsec radius circular aperture magnitude	mag	1362-1367	6.3f	y
225	h_m_30	H 30 arcsec radius circular aperture magnitude	mag	1369-1374	6.3f	y
226	k_m_30	K 30 arcsec radius circular aperture magnitude	mag	1376-1381	6.3f	y
227	j_msig_30	J 1-sigma uncertainty in 30 arcsec circular ap. mag	mag	1383-1387	5.3f	y
	Notes for j_msig_30: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
228	h_msig_30	H 1-sigma uncertainty in 30 arcsec circular ap. mag	mag	1389-1393	5.3f	y
	Notes for h_msig_30: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
229	k_msig_30	K 1-sigma uncertainty in 30 arcsec circular ap. mag	mag	1395-1399	5.3f	y
	Notes for k_msig_30: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
230	j_flg_30	J confusion flag for 30 arcsec circular ap. mag	---	1401-1404	4hd	y
	Notes for j_flg_30: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
231	h_flg_30	H confusion flag for 30 arcsec circular ap. mag	---	1406-1409	4hd	y
	Notes for h_flg_30: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
232	k_flg_30	K confusion flag for 30 arcsec circular ap. mag	---	1411-1414	4hd	y
	Notes for k_flg_30: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
233	j_m_40	J 40 arcsec radius circular aperture magnitude	mag	1416-1421	6.3f	y
234	h_m_40	H 40 arcsec radius circular aperture magnitude	mag	1423-1428	6.3f	y
235	k_m_40	K 40 arcsec radius circular aperture magnitude	mag	1430-1435	6.3f	y
236	j_msig_40	J 1-sigma uncertainty in 40 arcsec circular ap. mag	mag	1437-1441	5.3f	y
	Notes for j_msig_40: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
237	h_msig_40	H 1-sigma uncertainty in 40 arcsec circular ap. mag	mag	1443-1447	5.3f	y
	Notes for h_msig_40: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
238	k_msig_40	K 1-sigma uncertainty in 40 arcsec circular ap. mag	mag	1449-1453	5.3f	y
	Notes for k_msig_40: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
239	j_flg_40	J confusion flag for 40 arcsec circular ap. mag	---	1455-1458	4hd	y
	Notes for j_flg_40: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
240	h_flg_40	H confusion flag for 40 arcsec circular ap. mag	---	1460-1463	4hd	y
	Notes for h_flg_40: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
241	k_flg_40	K confusion flag for 40 arcsec circular ap. mag	---	1465-1468	4hd	y
	Notes for k_flg_40: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
242	j_m_50	J 50 arcsec radius circular aperture magnitude	mag	1470-1475	6.3f	y
243	h_m_50	H 50 arcsec radius circular aperture magnitude	mag	1477-1482	6.3f	y
244	k_m_50	K 50 arcsec radius circular aperture magnitude	mag	1484-1489	6.3f	y
245	j_msig_50	J 1-sigma uncertainty in 50 arcsec circular ap. mag	mag	1491-1495	5.3f	y
	Notes for j_msig_50: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
246	h_msig_50	H 1-sigma uncertainty in 50 arcsec circular ap. mag	mag	1497-1501	5.3f	y
	Notes for h_msig_50: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
247	k_msig_50	K 1-sigma uncertainty in 50 arcsec circular ap. mag	mag	1503-1507	5.3f	y
	Notes for k_msig_50: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
248	j_flg_50	J confusion flag for 50 arcsec circular ap. mag	---	1509-1512	4hd	y
	Notes for j_flg_50: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
249	h_flg_50	H confusion flag for 50 arcsec circular ap. mag	---	1514-1517	4hd	y
	Notes for h_flg_50: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
250	k_flg_50	K confusion flag for 50 arcsec circular ap. mag	---	1519-1522	4hd	y
	Notes for k_flg_50: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
251	j_m_60	J 60 arcsec radius circular aperture magnitude	mag	1524-1529	6.3f	y
252	h_m_60	H 60 arcsec radius circular aperture magnitude	mag	1531-1536	6.3f	y
253	k_m_60	K 60 arcsec radius circular aperture magnitude	mag	1538-1543	6.3f	y
254	j_msig_60	J 1-sigma uncertainty in 60 arcsec circular ap. mag	mag	1545-1549	5.3f	y
	Notes for j_msig_60: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
255	h_msig_60	H 1-sigma uncertainty in 60 arcsec circular ap. mag	mag	1551-1555	5.3f	y
	Notes for h_msig_60: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
256	k_msig_60	K 1-sigma uncertainty in 60 arcsec circular ap. mag	mag	1557-1561	5.3f	y
	Notes for k_msig_60: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
257	j_flg_60	J confusion flag for 60 arcsec circular ap. mag	---	1563-1566	4hd	y
	Notes for j_flg_60: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
258	h_flg_60	H confusion flag for 60 arcsec circular ap. mag	---	1568-1571	4hd	y
	Notes for h_flg_60: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
259	k_flg_60	K confusion flag for 60 arcsec circular ap. mag	---	1573-1576	4hd	y
	Notes for k_flg_60: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
260	j_m_70	J 70 arcsec radius circular aperture magnitude	mag	1578-1583	6.3f	y
261	h_m_70	H 70 arcsec radius circular aperture magnitude	mag	1585-1590	6.3f	y
262	k_m_70	K 70 arcsec radius circular aperture magnitude	mag	1592-1597	6.3f	y
263	j_msig_70	J 1-sigma uncertainty in 70 arcsec circular ap. mag	mag	1599-1603	5.3f	y
	Notes for j_msig_70: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
264	h_msig_70	H 1-sigma uncertainty in 70 arcsec circular ap. mag	mag	1605-1609	5.3f	y
	Notes for h_msig_70: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
265	k_msig_70	K 1-sigma uncertainty in 70 arcsec circular ap. mag	mag	1611-1615	5.3f	y
	Notes for k_msig_70: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
266	j_flg_70	J confusion flag for 70 arcsec circular ap. mag	---	1617-1620	4hd	y
	Notes for j_flg_70: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
267	h_flg_70	H confusion flag for 70 arcsec circular ap. mag	---	1622-1625	4hd	y
	Notes for h_flg_70: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
268	k_flg_70	K confusion flag for 70 arcsec circular ap. mag	---	1627-1630	4hd	y
	Notes for k_flg_70: The confusion flags [jhk]_flg* for each mag are defined as follows: 0 if no other sources within aperture used 1 if ap contained pixels masked off in atlas image 2 if ap contained pixels masked off due to neighboring sources 3 if ap contained pixels that had a point source flux subtracted off 4 if ap contained pixels within bright star mask 5 if ap contained pixels masked off due to persistence 6 if aperture ran into atlas image boundary 7 if ap contained pixels within bright galaxy mask 9 if integrated flux is negative If the integrated flux is negative, a mag value is calculated using BFMag = 99.0 - [ZERO_CAL - 2.5 log10(\|flux\|)]; the resulting mag range is between ~ 75 and 99.
269	j_m_sys	J system photometry magnitude	mag	1632-1637	6.3f	y
	Notes for j_m_sys: The system flux includes the flux from this extended source and anything else in the immediate area, including stars and neighboring galaxies that "touch" this source.
270	h_m_sys	H system photometry magnitude	mag	1639-1644	6.3f	y
	Notes for h_m_sys: The system flux includes the flux from this extended source and anything else in the immediate area, including stars and neighboring galaxies that "touch" this source.
271	k_m_sys	K system photometry magnitude	mag	1646-1651	6.3f	y
	Notes for k_m_sys: The system flux includes the flux from this extended source and anything else in the immediate area, including stars and neighboring galaxies that "touch" this source.
272	j_msig_sys	J 1-sigma uncertainty in system photometry mag	mag	1653-1657	5.3f	y
	Notes for j_msig_sys: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
273	h_msig_sys	H 1-sigma uncertainty in system photometry mag	mag	1659-1663	5.3f	y
	Notes for h_msig_sys: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
274	k_msig_sys	K 1-sigma uncertainty in system photometry mag	mag	1665-1669	5.3f	y
	Notes for k_msig_sys: All quoted magnitude uncertainties are the "combined" uncertainties for each band that provide an estimate of all random errors that contribute to the photometry. These uncertainties are the quadratic combination of the source extraction uncertainites, the photometric zero point offset uncertainties from the night during which the source was observed ([jhk]_zperr from the "Scan Data" table), and the residual flat-fielding errors (estimated to be 0.005 mags for all bands). The simple measurement uncertainty can be recovered by backing out the contributions of the photometric zero point uncertainty and the flat-fielding uncertainty from the values listed.
275	sys_flg	system flag: 0=no system, 1=nearby galaxy flux incl. in mag	---	1671-1674	4hd	y
276	contam_flg	stellar and artifact contamination flag	---	1676-1679	4hd	y
	Notes for contam_flg: The stellar and artifact contamination flag provides information about whether the extended source brightness estimate may be contaminated by superimposed point sources, or possible confusion with image artifacts generated by nearby bright stars (e.g. latent images, diffraction spikes, confusion halos and ghosts, and stripes). The value of the flag is given by: (stellar_contam_flg*10) + artflag. "Stellar_contam_flg"=0 if there is no contamination by superimposed point sources and =1 if there is. "Artflag" is the key to possible bright star artifact contamination and has the value: 0=no contamination, 1=dichroic glint, 2=latent or persistence image, 3=diffraction spike, 4=confusion in wings of a bright star.
277	j_r_3signorm	J 3-sigma radius normalized by shape radius	arcsec	1681-1685	5.1f	y
278	h_r_3signorm	H 3-sigma radius normalized by shape radius	arcsec	1687-1691	5.1f	y
279	k_r_3signorm	K 3-sigma radius normalized by shape radius	arcsec	1693-1697	5.1f	y
280	j_mnsurfb	J mean surface brightness at the 3-sig norm. radius	mag	1699-1703	5.2f	y
281	h_mnsurfb	H mean surface brightness at the 3-sig norm. radius	mag	1705-1709	5.2f	y
282	k_mnsurfb	K mean surface brightness at the 3-sig norm. radius	mag	1711-1715	5.2f	y
283	j_5sig_ba	J minor/major axis ratio fit to the 5-sigma isophote	---	1717-1721	5.3f	y
284	h_5sig_ba	H minor/major axis ratio fit to the 5-sigma isophote	---	1723-1727	5.3f	y
285	k_5sig_ba	K minor/major axis ratio fit to the 5-sigma isophote	---	1729-1733	5.3f	y
286	j_5sig_phi	J angle to 5-sigma major axis (E of N)	deg	1735-1738	4hd	y
287	h_5sig_phi	H angle to 5-sigma major axis (E of N)	deg	1740-1743	4hd	y
288	k_5sig_phi	K angle to 5-sigma major axis (E of N)	deg	1745-1748	4hd	y
289	j_d_area	J 5-sigma to 3-sigma differential area	---	1750-1753	4hd	y
290	h_d_area	H 5-sigma to 3-sigma differential area	---	1755-1758	4hd	y
291	k_d_area	K 5-sigma to 3-sigma differential area	---	1760-1763	4hd	y
292	j_perc_darea	J 5-sigma to 3-sigma percent area change	---	1765-1768	4hd	y
293	h_perc_darea	H 5-sigma to 3-sigma percent area change	---	1770-1773	4hd	y
294	k_perc_darea	K 5-sigma to 3-sigma percent area change	---	1775-1778	4hd	y
295	j_bisym_rat	J bi-symmetric flux ratio	---	1780-1784	5.3f	y
296	h_bisym_rat	H bi-symmetric flux ratio	---	1786-1790	5.3f	y
297	k_bisym_rat	K bi-symmetric flux ratio	---	1792-1796	5.3f	y
298	j_bisym_chi	J bi-symmetric cross-correlation chi	---	1798-1802	5.3f	y
299	h_bisym_chi	H bi-symmetric cross-correlation chi	---	1804-1808	5.3f	y
300	k_bisym_chi	K bi-symmetric cross-correlation chi	---	1810-1814	5.3f	y
301	j_sh0	J ridge shape (LCSB: BSNR limit)	---	1816-1819	4.2f	y
302	h_sh0	H ridge shape (LCSB: BSNR limit)	---	1821-1824	4.2f	y
303	k_sh0	K ridge shape (LCSB: BSNR limit)	---	1826-1829	4.2f	y
304	j_sig_sh0	J ridge shape sigma (LCSB: B2SNR limit)	---	1831-1834	4.2f	y
305	h_sig_sh0	H ridge shape sigma (LCSB: B2SNR limit)	---	1836-1839	4.2f	y
306	k_sig_sh0	K ridge shape sigma (LCSB: B2SNR limit)	---	1841-1844	4.2f	y
307	j_sc_mxdn	J mxdn (score) (LCSB: BSNR - block/smoothed SNR)	---	1846-1850	5.1f	y
308	h_sc_mxdn	H mxdn (score) (LCSB: BSNR - block/smoothed SNR)	---	1852-1856	5.1f	y
309	k_sc_mxdn	K mxdn (score) (LCSB: BSNR - block/smoothed SNR)	---	1858-1862	5.1f	y
310	j_sc_sh	J shape (score)	---	1864-1868	5.1f	y
311	h_sc_sh	H shape (score)	---	1870-1874	5.1f	y
312	k_sc_sh	K shape (score)	---	1876-1880	5.1f	y
313	j_sc_wsh	J wsh (score) (LCSB: PSNR - peak raw SNR)	---	1882-1886	5.1f	y
314	h_sc_wsh	H wsh (score) (LCSB: PSNR - peak raw SNR)	---	1888-1892	5.1f	y
315	k_sc_wsh	K wsh (score) (LCSB: PSNR - peak raw SNR)	---	1894-1898	5.1f	y
316	j_sc_r23	J r23 (score) (LCSB: TSNR - integrated SNR for r=15)	---	1900-1904	5.1f	y
317	h_sc_r23	H r23 (score) (LCSB: TSNR - integrated SNR for r=15)	---	1906-1910	5.1f	y
318	k_sc_r23	K r23 (score) (LCSB: TSNR - integrated SNR for r=15)	---	1912-1916	5.1f	y
319	j_sc_1mm	J 1st moment (score) (LCSB: super blk 2,4,8 SNR)	---	1918-1922	5.1f	y
320	h_sc_1mm	H 1st moment (score) (LCSB: super blk 2,4,8 SNR)	---	1924-1928	5.1f	y
321	k_sc_1mm	K 1st moment (score) (LCSB: super blk 2,4,8 SNR)	---	1930-1934	5.1f	y
322	j_sc_2mm	J 2nd moment (score) (LCSB: SNRMAX - super SNR max)	---	1936-1940	5.1f	y
323	h_sc_2mm	H 2nd moment (score) (LCSB: SNRMAX - super SNR max)	---	1942-1946	5.1f	y
324	k_sc_2mm	K 2nd moment (score) (LCSB: SNRMAX - super SNR max)	---	1948-1952	5.1f	y
325	j_sc_vmn	J vmean (score)	---	1954-1958	5.1f	y
326	h_sc_vmn	H vmean (score)	---	1960-1964	5.1f	y
327	k_sc_vmn	K vmean (score)	---	1966-1970	5.1f	y
328	j_sc_vint	J vint (score)	---	1972-1976	5.1f	y
329	h_sc_vint	H vint (score)	---	1978-1982	5.1f	y
330	k_sc_vint	K vint (score)	---	1984-1988	5.1f	y
331	j_scalen	J alpha scale length	---	1990-1993	4.1f	y
332	h_scalen	H alpha scale length	---	1995-1998	4.1f	y
333	k_scalen	K alpha scale length	---	2000-2003	4.1f	y
334	j_sc_r1	J r1 (score)	---	2005-2009	5.1f	y
335	h_sc_r1	H r1 (score)	---	2011-2015	5.1f	y
336	k_sc_r1	K r1 (score)	---	2017-2021	5.1f	y
337	j_sc_msh	J median shape score	---	2023-2027	5.1f	y
338	h_sc_msh	H median shape score	---	2029-2033	5.1f	y
339	k_sc_msh	K median shape score	---	2035-2039	5.1f	y
340	j_subst2	J residual background #2 (score)	---	2041-2046	6.1f	y
341	h_subst2	H residual background #2 (score)	---	2048-2053	6.1f	y
342	k_subst2	K residual background #2 (score)	---	2055-2060	6.1f	y
343	j_chif_ellf	J % chi-fraction for elliptical fit to 3-sig isophote	---	2062-2065	4.1f	y
344	k_chif_ellf	K % chi-fraction for elliptical fit to 3-sig isophote	---	2067-2070	4.1f	y
345	sup_chif_ellf	super-image % chi-fraction for ellip. fit to 3-sig isophote	---	2072-2075	4.1f	y
346	j_back	J image median background	---	2077-2082	6.1f	y
347	h_back	H image median background	---	2084-2089	6.1f	y
348	k_back	K image median background	---	2091-2096	6.1f	y
349	j_resid_ann	J residual annulus background median	DN	2098-2103	6.3f	y
350	h_resid_ann	H residual annulus background median	DN	2105-2110	6.3f	y
351	k_resid_ann	K residual annulus background median	DN	2112-2117	6.3f	y
352	j_peak	J peak pixel brightness	mag	2119-2123	5.2f	y
353	h_peak	H peak pixel brightness	2125-2129	5.2f	mag	y
354	k_peak	K peak pixel brightness	mag	2131-2135	5.2f	y
355	j_5surf	J central surface brightness (r<=5)	mag	2137-2141	5.2f	y
356	h_5surf	H central surface brightness (r<=5)	mag	2143-2147	5.2f	y
357	k_5surf	K central surface brightness (r<=5)	mag	2149-2153	5.2f	y
358	j_bndg_per	J banding Fourier Transf. period on this side of image	arcsec	2155-2158	4d	y
359	j_bndg_amp	J banding maximum FT amplitude on this side of image	DN	2160-2164	5.3f	y
360	h_bndg_per	H banding Fourier Transf. period on this side of image	arcsec	2166-2169	4d	y
361	h_bndg_amp	H banding maximum FT amplitude on this side of image	DN	2171-2175	5.3f	y
362	k_bndg_per	K banding Fourier Transf. period on this side of image	arcsec	2177-2180	4d	y
363	k_bndg_amp	K banding maximum FT amplitude on this side of image	DN	2182-2186	5.3f	y
364	j_seetrack	J band seetracking score	---	2188-2191	4.1f	y
365	h_seetrack	H band seetracking score	---	2193-2196	4.1f	y
366	k_seetrack	K band seetracking score	---	2198-2201	4.1f	y
367	j_airglow	J band airglow score	---	2203-2206	4.2f	y
368	h_airglow	H band airglow score	---	2208-2211	4.2f	y
369	k_airglow	K band airglow score	---	2213-2216	4.2f	y
370	density	image log(density) of stars with k<14 mag	---	2218-2221	4.2f	y
371	sup_r_3sig	super-image 3-sigma isophotal semi-major axis radius	arcsec	2223-2227	5.1f	y
372	sup_ba	minor/major axis ratio fit to 3-sig. super-image isophote	---	2229-2233	5.3f	y
373	sup_phi	super-image angle to major axis (E of N)	deg	2235-2238	4hd	y
374	sup_r_3signorm	super-image 3-sigma radius normalized by shape radius	arcsec	2240-2244	5.1f	y
375	sup_mnsurfb	super-image mean surface brightness at 3-sig norm. radius	mag	2246-2250	5.2f	y
376	im_nx	size of postage stamp image in pixels	---	2252-2255	4hd	n
377	n_blank	number of blanked source records	---	2257-2260	4hd	n
	Notes for n_blank: These parameters refer to sources that were blanked and/or subtracted from the images before doing photometry. Data for each of these blanked/ subtracted sources are found in the blanked and subtracted source tables.
378	n_sub	number of subtracted source records	---	2262-2265	4hd	n
	Notes for n_sub: These parameters refer to sources that were blanked and/or subtracted from the images before doing photometry. Data for each of these blanked/ subtracted sources are found in the blanked and subtracted source tables.
379	bl_sub_flg	blanked/subtracted src description flag	---	2267-2270	4hd	n
380	id_flg	type/galaxy ID flag (0=non-catalog, 1=catalog, 2=LCSB)	---	2272-2272	1hd	n
	Notes for id_flg: This flag indicates the extended source catalog type as follows: 0 = extended source not found in another catalog 1 = extended source is found in galaxy catalog (ID found in id_cat field) 2 = LCSB (Low Central Surface Brightness) source
381	id_cat	matched galaxy's catalog name	---	2274-2283	10s	y
382	r_ngc	distance from nearest big galaxy	arcsec	2285-2289	5.2f	y
383	fg_flg	flux-growth convergence flag	---	2291-2296	6s	y
384	blk_fac	LCSB blocking factor (1, 2, 4, 8)	---	2298-2301	4hd	y
385	ellfit_flg	ellipse fitting contamination flag	---	2303-2306	4hd	y
386	j_h	default J-H mag color	mag	2308-2314	7.3f	y
	Notes for j_h: Magnitude colors are calculated using the [jhk]_m default mags and sigmas for the extended sources and the optical mags [br]_m_opt in the associated point source entry. If one of the mags used in a color calculation is NULL, the color value is an upper or lower limit. (Color limits are NOT calculated when both mags are NULL.)
387	j_h_sig	sigma for J-H mag color	mag	2316-2321	6.3f	y
	Notes for j_h_sig: For colors having detections in both bands, the color mag sigma values are the root-sum-square of the two mag sigmas. If one of the mags used in the calculation is NULL, the color sigma is the other band's mag sigma.
388	h_k	default H-K mag color	mag	2323-2329	7.3f	y
	Notes for h_k: Magnitude colors are calculated using the [jhk]_m default mags and sigmas for the extended sources and the optical mags [br]_m_opt in the associated point source entry. If one of the mags used in a color calculation is NULL, the color value is an upper or lower limit. (Color limits are NOT calculated when both mags are NULL.)
389	h_k_sig	sigma for H-K mag color	mag	2331-2336	6.3f	y
	Notes for h_k_sig: For colors having detections in both bands, the color mag sigma values are the root-sum-square of the two mag sigmas. If one of the mags used in the calculation is NULL, the color sigma is the other band's mag sigma.
390	j_k	default J-K mag color	mag	2338-2344	7.3f	y
	Notes for j_k: Magnitude colors are calculated using the [jhk]_m default mags and sigmas for the extended sources and the optical mags [br]_m_opt in the associated point source entry. If one of the mags used in a color calculation is NULL, the color value is an upper or lower limit. (Color limits are NOT calculated when both mags are NULL.)
391	j_k_sig	sigma for J-K mag color	mag	2346-2351	6.3f	y
	Notes for j_k_sig: For colors having detections in both bands, the color mag sigma values are the root-sum-square of the two mag sigmas. If one of the mags used in the calculation is NULL, the color sigma is the other band's mag sigma.
392	b_r	B-R mag color of associated optical source	mag	2353-2359	7.3f	y
393	r_k	default R-K mag color (using associated optical source)	mag	2361-2367	7.3f	y
	Notes for r_k: Magnitude colors are calculated using the [jhk]_m default mags and sigmas for the extended sources and the optical mags [br]_m_opt in the associated point source entry. If one of the mags used in a color calculation is NULL, the color value is an upper or lower limit. (Color limits are NOT calculated when both mags are NULL.)
394	b_k	default B-K mag color	mag	2369-2375	7.3f	y
	Notes for b_k: Magnitude colors are calculated using the [jhk]_m default mags and sigmas for the extended sources and the optical mags [br]_m_opt in the associated point source entry. If one of the mags used in a color calculation is NULL, the color value is an upper or lower limit. (Color limits are NOT calculated when both mags are NULL.)
395	r_j	default R-J mag color	mag	2377-2383	7.3f	y
	Notes for r_j: Magnitude colors are calculated using the [jhk]_m default mags and sigmas for the extended sources and the optical mags [br]_m_opt in the associated point source entry. If one of the mags used in a color calculation is NULL, the color value is an upper or lower limit. (Color limits are NOT calculated when both mags are NULL.)
396	b_j	default B-J mag color	mag	2385-2391	7.3f	y
	Notes for b_j: Magnitude colors are calculated using the [jhk]_m default mags and sigmas for the extended sources and the optical mags [br]_m_opt in the associated point source entry. If one of the mags used in a color calculation is NULL, the color value is an upper or lower limit. (Color limits are NOT calculated when both mags are NULL.)
397	e_score	extended score: 1 (extended) < e_score < 2 (point-like)	---	2393-2396	4.2f	y
398	g_score	galaxy score: 1 (extended) < g_score < 2 (point-like)	---	2398-2401	4.2f	y
399	feye	"eye" score for source	---	2403-2406	4hd	y
	Notes for feye: The "eye" score gives the source type for those sources examined "by eye": -2 = unknown -1 = no verification (i.e., not examined) 1 = galaxy 2 = non-extended (e.g., star, double, triple, artifact)
400	cc_flag	indicates artifact contamination and/or confusion	---	2408-2408	1s	y
	Notes for cc_flg: The contamination/confusion flag indicates whether the source's photometry and position may be affected by artifacts of, or confusion with, nearby bright stars. The flag consists of a single character string. Sources are tested for contamination and/or confusion in the order given below, and once a flag is applied to the source, testing is stopped in that band. The flag values indicate the source may be: U: unreliable source; probable image artifact detection C: affected by confusion with or artifact of a nearby bright star 0: default value -- not contaminated

^aThese are C format statements, which do not include blanks that separate fields and which are set to the maximum possible number of characters in each string. Fields that have values much less than the maximum possible number may have additional leading blanks. For example, 10° < ra < 100° will have a format 9.6f. A caveat is that fields that are allowed to contain "null," as indicated in the final column of this table, must be read in as strings, checked for null, and then converted to the appropriate type.