Appendix 2. Calibration Scan Working Databases and Images

3. Calibration Extended Source Working Database and Metadata Table Formats

b. Calibration Extended Source Working Databases Column Descriptions

The 2MASS Calibration Scan Extended Source Working Databases (Cal-XSWDB, LMC/SMC Cal-XSWDB) contain 388 columns of information per source entry (most of which is photometry). Because extended sources are much more complicated than point sources, it takes many more parameters to characterize them. Some parameters are required to describe the spatial extent of a source, and many more are required to characterize the photometry. In addition to a number of standard measures of photometry, the Cal-XSWDBs also report the magnitude as measured in a number of different fixed-size apertures. The columns are described in the tables below. We have separated the columns accordingto their basic function and utility.

Photometry algorithms and performance, "Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags," are discussed in Section IV.5e. The information contained in the All-Sky Release Extended Source Catalog (XSC) FAQ and Primer, "How to Use the 2MASS XSC -- FAQ Sheet" (Section II.3b) is directly applicable to the Cal-XSWDBs since the calibration scan data were reduced using the same algorithms as the All-Sky Survey.

Name/Position Info

Standard Photometry & Orientation

Large Aperture Photometry

Miscellaneous Photometry and Characterization

A. Name and Position Information

column	Parameter Name	View	Format	Units	Description
1	jdate	L	13.4f	day	Julian date of the source measurement accurate to ±3 minutes. This value is the mean Julian date of the scan observation in which this source falls. For a more precise value of Julian date for this source, see the jdate entry in the PSWDB using the pts_key index as a cross-reference.
---	Position Information
3	ra	S	10.6f	deg	Right ascension (J2000 decimal deg) based on peak pixel.
4	dec	S	10.6f	deg	Declination (J2000 decimal deg) based on peak pixel.
5	sup_ra	L	10.6f	deg	Super-coadd centroid RA (J2000 decimal deg).
6	sup_dec	L	10.6f	deg	Super-coadd centroid Dec (J2000 decimal deg).
7	glon	L	7.3f	deg	Galactic longitude (decimal deg) based on peak pixel. Galactic coordinate for 2MASS source derived by precessing reconstructed ra and dec to B1950, and performing rotational transformation into l_II, b_II coordinate system. This coordinate should not be used as an astrometric reference because it has been rounded to 0.001 deg.
8	glat	L	7.3f	deg	Galactic latitude (decimal deg) based on peak pixel. Galactic coordinate for 2MASS source derived by precessing reconstructed ra and dec to B1950, and performing rotational transformation into l_II, b_II coordinate system. This coordinate should not be used as an astrometric reference because it has been rounded to 0.001 deg.
9	density	L	5.2f	-	Coadd log(density) of stars with k<14 mag. See Stellar Number Density Metric: "density".

B. Standard (recommended) Photometry: Isophotal Apertures Based on the Ks 20 mag/arcsec^2 Elliptical Isophote, and 2-D Orientation

column	Parameter Name	View	Format	Units	Description
---	Isophotal photom at 20 using K fiducial ellip ap
10	r_k20fe	S	6.1f	arcsec	20mag/sq." isophotal K fiducial ell. ap. semi-major axis. "Fiducial" apertures are determined for each type of total and isophotal photometry measurements. 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. See Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags.
11	j_m_k20fe	S	6.3f	mag	J 20mag/sq." isophotal fiducial ell. ap. magnitude. See Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags.
12	j_msig_k20fe	S	5.3f	mag	J 1-sigma uncertainty in 20mag/sq." iso.fid.ell.mag.
13	j_flg_k20fe	S	1hd	-	J confusion flag for 20mag/sq." iso. fid. ell. mag. 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 coadd 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 coadd 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.
14	h_m_k20fe	S	6.3f	mag	H 20mag/sq." isophotal fiducial ell. ap. magnitude. See Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags.
15	h_msig_k20fe	S	5.3f	mag	H 1-sigma uncertainty in 20mag/sq." iso.fid.ell.mag.
16	h_flg_k20fe	S	1hd	-	H confusion flag for 20mag/sq." iso. fid. ell. mag. 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 coadd 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 coadd 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.
17	k_m_k20fe	S	6.3f	mag	K 20mag/sq." isophotal fiducial ell. ap. magnitude. See Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags.
18	k_msig_k20fe	S	5.3f	mag	K 1-sigma uncertainty in 20mag/sq." iso.fid.ell.mag.
19	k_flg_k20fe	S	1hd	-	K confusion flag for 20mag/sq." iso. fid. ell. mag. 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 coadd 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 coadd 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.
---	Elliptical Isophotal Orientation
20	r_3sig	L	5.1f	arcsec	3-sigma K isophotal semi-major axis.
21	j_ba	L	5.3f	-	J minor/major axis ratio fit to the 3-sigma isophote.
22	j_phi	L	3hd	deg	J angle to 3-sigma major axis (E of N), quantized to 5°. For large galaxies measured as part of the 2MASS Large Galaxy Atlas (cc_flg="Z"), the position angles are quantized to 2°.
23	h_ba	L	5.3f	-	H minor/major axis ratio fit to the 3-sigma isophote.
24	h_phi	L	3hd	deg	H angle to 3-sigma major axis (E of N), quantized to 5°. For large galaxies measured as part of the 2MASS Large Galaxy Atlas (cc_flg="Z"), the position angles are quantized to 2°.
25	k_ba	S	5.3f	-	K minor/major axis ratio fit to the 3-sigma isophote.
26	k_phi	S	3hd	deg	K angle to 3-sigma major axis (E of N), quantized to 5°. For large galaxies measured as part of the 2MASS Large Galaxy Atlas (cc_flg="Z"), the position angles are quantized to 2°.
27	sup_r_3sig	L	5.1f	arcsec	Super-coadd 3-sigma isophotal semi-major axis radius.
28	sup_ba	S	5.3f	-	Minor/major axis ratio fit to 3-sig. super-coadd isophote.
29	sup_phi	S	3hd	deg	Super-coadd angle to major axis (E of N), quantized to 5°. For large galaxies measured as part of the 2MASS Large Galaxy Atlas (cc_flg="Z"), the position angles are quantized to 2°.

C. Large Apertures, including Kron and Total Versions, and Surface Brightness

column	Parameter Name	View	Format	Units	Description
---	Photometry using Kron elliptical aperture
30	r_fe	L	6.1f	arcsec	K fiducial Kron elliptical aperture semi-major axis. "Fiducial" apertures are determined for each type of total and isophotal photometry measurements. 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. See Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags.
31	j_m_fe	L	6.3f	mag	J fiducial Kron elliptical aperture magnitude. See Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags.
32	j_msig_fe	L	5.3f	mag	J 1-sigma uncertainty in fiducial Kron ell. mag.
33	j_flg_fe	L	1hd	-	J confusion flag for fiducial Kron ell. mag. 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 coadd 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 coadd 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.
34	h_m_fe	L	6.3f	mag	H fiducial Kron elliptical aperture magnitude. See Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags.
35	h_msig_fe	L	5.3f	mag	H 1-sigma uncertainty in fiducial Kron ell. mag.
36	h_flg_fe	L	1hd	-	H confusion flag for fiducial Kron ell. mag. 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 coadd 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 coadd 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.
37	k_m_fe	L	6.3f	mag	K fiducial Kron ell. mag aperture magnitude. See Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags.
38	k_msig_fe	L	5.3f	mag	K 1-sigma uncertainty in fiducial Kron ell. mag.
39	k_flg_fe	L	1hd	-	K confusion flag for fiducial Kron ell. mag. 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 coadd 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 coadd 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.
---	Total Photometry from extrapolation of fit to radial profile
40	r_ext	S	7.2f	arcsec	extrapolation/total radius. See Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags.
41	j_m_ext	S	6.3f	mag	J mag from fit extrapolation. See Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags.
42	j_msig_ext	L	5.3f	mag	J 1-sigma uncertainty in mag from fit extrapolation.
43	j_pchi	S	6.3f	-	J chi^2 of fit to rad. profile (LCSB: alpha scale len). If the source is not an LCSB, these fields contain the reduced chi-squared values for each band of the modified exponential fits to the elliptical radial profiles, used for extrapolation and half-light estimates. For LCSBs, they contain the alpha scale lengths.
44	h_m_ext	S	6.3f	mag	H mag from fit extrapolation. See Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags.
45	h_msig_ext	S	5.3f	mag	H 1-sigma uncertainty in mag from fit extrapolation.
46	h_pchi	L	6.3f	-	H chi^2 of fit to rad. profile (LCSB: alpha scale len). If the source is not an LCSB, these fields contain the reduced chi-squared values for each band of the modified exponential fits to the elliptical radial profiles, used for extrapolation and half-light estimates. For LCSBs, they contain the alpha scale lengths.
47	k_m_ext	S	6.3f	mag	K mag from fit extrapolation. See Large Aperture Photometry: Profile Fitting, Isophotal & Total Mags.
48	k_msig_ext	S	5.3f	mag	K 1-sigma uncertainty in mag from fit extrapolation.
49	k_pchi	L	6.3f	-	K chi^2 of fit to rad. profile (LCSB: alpha scale len). If the source is not an LCSB, these fields contain the reduced chi-squared values for each band of the modified exponential fits to the elliptical radial profiles, used for extrapolation and half-light estimates. For LCSBs, they contain the alpha scale lengths.
---	Effective radii and mean surface brightness
50	j_r_eff	L	6.2f	arcsec	J half-light (integrated half-flux point) radius. See Half-Light "Effective" Aperture & Concentration Index Beware the circularizing effect of the PSF on small galaxies. See The 2MASS Beam.
51	j_mnsurfb_eff	L	5.2f	mag	J mean surface brightness at the half-light radius. See Half-Light "Effective" Aperture & Concentration Index Beware the circularizing effect of the PSF on small galaxies. See The 2MASS Beam.
52	h_r_eff	L	6.2f	arcsec	H half-light (integrated half-flux point) radius. See Half-Light "Effective" Aperture & Concentration Index Beware the circularizing effect of the PSF on small galaxies. See The 2MASS Beam.
53	h_mnsurfb_eff	L	5.2f	mag	H mean surface brightness at the half-light radius. See Half-Light "Effective" Aperture & Concentration Index Beware the circularizing effect of the PSF on small galaxies. See The 2MASS Beam.
54	k_r_eff	L	6.2f	arcsec	K half-light (integrated half-flux point) radius. See Half-Light "Effective" Aperture & Concentration Index Beware the circularizing effect of the PSF on small galaxies. See The 2MASS Beam.
55	k_mnsurfb_eff	L	5.2f	mag	K mean surface brightness at the half-light radius. See Half-Light "Effective" Aperture & Concentration Index Beware the circularizing effect of the PSF on small galaxies. See The 2MASS Beam.
56	j_con_indx	L	5.2f	-	J concentration index r_75%/r_25%. The concentration index for the galaxy in each band is the ratio of the radii which contain 75% and 25% of the total light, r_75%/r_25%. See Half-Light "Effective" Aperture & Concentration Index Beware the circularizing effect of the PSF on small galaxies. See The 2MASS Beam.
57	h_con_indx	L	5.2f	-	H concentration index r_75%/r_25%. The concentration index for the galaxy in each band is the ratio of the radii which contain 75% and 25% of the total light, r_75%/r_25%. See Half-Light "Effective" Aperture & Concentration Index Beware the circularizing effect of the PSF on small galaxies. See The 2MASS Beam.
58	k_con_indx	L	5.2f	-	K concentration index r_75%/r_25%. The concentration index for the galaxy in each band is the ratio of the radii which contain 75% and 25% of the total light, r_75%/r_25%. See Half-Light "Effective" Aperture & Concentration Index Beware the circularizing effect of the PSF on small galaxies. See The 2MASS Beam.
59	j_peak	L	6.2f	mag	J peak pixel brightness.
60	h_peak	L	6.2f	mag	H peak pixel brightness.
61	k_peak	L	6.2f	mag	K peak pixel brightness.
62	j_5surf	L	6.2f	mag	J central surface brightness (r<=5).
63	h_5surf	L	6.2f	mag	H central surface brightness (r<=5).
64	k_5surf	L	6.2f	mag	K central surface brightness (r<=5).

D. Miscellaneous Photometry and Characterization Measures

column	Parameter Name	View	Format	Units	Description
---	Quality and Star-Galaxy Discrimination Scores
65	rel	S	1s	-	Reliability flag. Single character flag that is related to the probability that the extraction is a valid detection of a near infrared source on the sky at the time of the observation, and that the source is resolved relative to the 2MASS point spread function. "A" - P>90% "B" - 80%<P<90% "C" - 70%<P<80% "D" - 50%<P<70% "E" - 20%<P<50% "F" - P<20% This flag does not provide information about the quality of the position or flux measurement. For that, users should refer to e_score, g_score, vc, cc_flg and positional and photometric uncertainties.
66	e_score	L	5.2f	-	extended score: 1(extended) < e_score < 2(point-like). See the FAQ: Star-Galaxy Separation: How do the E and G-scores work?
67	g_score	L	5.2f	-	galaxy score: 1(extended) < g_score < 2(point-like). See the FAQ: Star-Galaxy Separation: How do the E and G-scores work?
68	vc	L	2hd	-	visual verification score for source. The visual classification 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) See Visual Inspection of Extended Sources
69	cc_flg	S	1s	-	indicates artifact contamination and/or confusion. 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: A - Known artifacts 0 - Default value -- not contaminated See Extended Source Confusion Flag
70	spos	S	5d	-	Number of scans covering the position of this extraction. This is computed during the WDB merging process, using boundaries of each scan that are great-circle interpolations connecting the 3-band coverage corners. Since actual scans "wiggle" slightly in RA due to telescope motions, the actual number of coverages for extractions near scan edges can differ from spos. A null value in this column indicates that the source was not included in the source merging process because of low reliability, or proximity to a scan edge.
71	sdet	S	5d	-	Total number of detections of this extraction in any band in this WDB table, in all scans covering its position, determined during the WDB merging processing. It is possible to have sdet > spos for extractions because extended sources may have in-scan duplicate extractions in the Atlas Image overlap regions, and near scan edges because of the approximations used to determine spos. A null value in this column indicates that the source was not included in the source merging process because of low reliability, or proximity to a scan edge.
72	gcntr	S	5d	-	Unique identification number of the record in the Merged Extended Source Information table corresponding to the merged "group" containing this extraction. The merged "group" contains the combined position and brightness information for all extractions falling within ~5" of each other in the WDB. In confused cases where this extraction appears in more than one group (gcnf>1), the indicated group is the one to which this extraction lies closest. A null value in this column indicates that the source either that the position of this extraction was observed only once, or it was not included in the source merging process because of low reliability, or proximity to a scan edge.
73	gcnf	S	1d	-	Merging confusion flag. Single digit flag that indicates whether this extraction was associated with more than one group during the WDB merging process. "0,1" - Extraction associated with only one group. "2,3" - Extraction associated with more than one group. Group indicated in the gcntr column is one whose center lies closest to the position of this extraction. "null" - Extraction was observed only once, or was not included in the source merging process because of low reliability, or proximity to a scan edge.
---	Postage-stamp image parameter
74	im_nx	L	4hd	-	Size of postage stamp image in pixels. Calibration scan extended source postage stamp images are not currently available. To access the All-Sky XSC postage stamp images (both jpeg and FITS versions), click 2MASS All-Sky XSC Full-Resolution Image Server
---	Isophotal photom at 20 using K fiducial circ ap
75	r_k20fc	L	5.1f	arcsec	20mag/sq." isophotal K fiducial circular ap. radius. "Fiducial" apertures are determined for each type of total and isophotal photometry measurements. 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. Cautionary note: A negative value in this column indicates that the source measurement was corrupted, usually due to confusion from a nearby source, and the derived radius is not meaningful.
76	j_m_k20fc	L	6.3f	mag	J 20mag/sq." isophotal fiducial circ. ap. mag.
77	j_msig_k20fc	L	5.3f	mag	J 1-sigma uncertainty in 20mag/sq." iso.fid.circ. mag.
78	j_flg_k20fc	L	1hd	-	J confusion flag for 20mag/sq." iso. fid. circ. mag. 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 coadd 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 coadd 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.
79	h_m_k20fc	L	6.3f	mag	H 20mag/sq." isophotal fiducial circ. ap. mag.
80	h_msig_k20fc	L	5.3f	mag	H 1-sigma uncertainty in 20mag/sq." iso.fid.circ. mag.
81	h_flg_k20fc	L	1hd	-	H confusion flag for 20mag/sq." iso. fid. circ. mag. 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 coadd 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 coadd 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.
82	k_m_k20fc	L	6.3f	mag	K 20mag/sq." isophotal fiducial circ. ap. mag.
83	k_msig_k20fc	L	5.3f	mag	K 1-sigma uncertainty in 20mag/sq." iso.fid.circ. mag.
84	k_flg_k20fc	L	1hd	-	K confusion flag for 20mag/sq." iso. fid. circ. mag. 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 coadd 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 coadd 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.
---	Kron elliptical photometry
85	j_r_e	L	5.1f	arcsec	J Kron elliptical aperture semi-major axis.
86	j_m_e	L	6.3f	mag	J Kron elliptical aperture magnitude.
87	j_msig_e	L	5.3f	mag	J 1-sigma uncertainty in Kron elliptical mag.
88	j_flg_e	L	1hd	-	J confusion flag for Kron elliptical mag. 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 coadd 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 coadd 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.
89	h_r_e	L	5.1f	arcsec	H Kron elliptical aperture semi-major axis.
90	h_m_e	L	6.3f	mag	H Kron elliptical aperture magnitude.
91	h_msig_e	L	5.3f	mag	H 1-sigma uncertainty in Kron elliptical mag.
92	h_flg_e	L	1hd	-	H confusion flag for Kron elliptical mag. 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 coadd 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 coadd 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.
93	k_r_e	L	5.1f	arcsec	K Kron elliptical aperture semi-major axis.
94	k_m_e	L	6.3f	mag	K Kron elliptical aperture magnitude.
95	k_msig_e	L	5.3f	mag	K 1-sigma uncertainty in Kron elliptical mag.
96	k_flg_e	L	1hd	-	K confusion flag for Kron elliptical mag. 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 coadd 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 coadd 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.
---	Kron circular photometry
97	j_r_c	L	5.1f	arcsec	J Kron circular aperture radius.
98	j_m_c	L	6.3f	mag	J Kron circular aperture magnitude.
99	j_msig_c	L	5.3f	mag	J 1-sigma uncertainty in Kron circular mag.
100	j_flg_c	L	1hd	-	J confusion flag for Kron circular mag. 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 coadd 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 coadd 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.
101	h_r_c	L	5.1f	arcsec	H Kron circular aperture radius.
102	h_m_c	L	6.3f	mag	H Kron circular aperture magnitude.
103	h_msig_c	L	5.3f	mag	H 1-sigma uncertainty in Kron circular mag.
104	h_flg_c	L	1hd	-	H confusion flag for Kron circular mag. 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 coadd 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 coadd 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.
105	k_r_c	L	5.1f	arcsec	K Kron circular aperture radius.
106	k_m_c	L	6.3f	mag	K Kron circular aperture magnitude.
107	k_msig_c	L	5.3f	mag	K 1-sigma uncertainty in Kron circular mag.
108	k_flg_c	L	1hd	-	K confusion flag for Kron circular mag. 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 coadd 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 coadd 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.
---	Kron photometry using K fiducial circular aperture
109	r_fc	L	5.1f	arcsec	K fiducial Kron circular aperture radius. "Fiducial" apertures are determined for each type of total and isophotal photometry measurements. 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.
110	j_m_fc	L	6.3f	mag	J fiducial Kron circular magnitude.
111	j_msig_fc	L	5.3f	mag	J 1-sigma uncertainty in fiducial Kron circ. mag.
112	j_flg_fc	L	1hd	-	J confusion flag for fiducial Kron circ. mag. 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 coadd 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 coadd 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.
113	h_m_fc	L	6.3f	mag	H fiducial Kron circular magnitude.
114	h_msig_fc	L	5.3f	mag	H 1-sigma uncertainty in fiducial Kron circ. mag.
115	h_flg_fc	L	1hd	-	H confusion flag for fiducial Kron circ. mag. 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 coadd 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 coadd 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.
116	k_m_fc	L	6.3f	mag	K fiducial Kron circular magnitude.
117	k_msig_fc	L	5.3f	mag	K 1-sigma uncertainty in fiducial Kron circ. mag.
118	k_flg_fc	L	1hd	-	K confusion flag for fiducial Kron circ. mag. 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 coadd 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 coadd 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.
---	Isophotal photom at 20 mag/sq.arcsec using ell ap
119	j_r_i20e	L	5.1f	arcsec	J 20mag/sq." isophotal elliptical ap. semi-major axis.
120	j_m_i20e	L	6.3f	mag	J 20mag/sq." isophotal elliptical ap. magnitude.
121	j_msig_i20e	L	5.3f	mag	J 1-sigma uncertainty in 20mag/sq." iso. ell. mag.
122	j_flg_i20e	L	1hd	-	J confusion flag for 20mag/sq." iso. ell. mag. 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 coadd 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 coadd 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.
123	h_r_i20e	L	5.1f	arcsec	H 20mag/sq." isophotal elliptical ap. semi-major axis.
124	h_m_i20e	L	6.3f	mag	H 20mag/sq." isophotal elliptical ap. magnitude.
125	h_msig_i20e	L	5.3f	mag	H 1-sigma uncertainty in 20mag/sq." iso. ell. mag.
126	h_flg_i20e	L	1hd	-	H confusion flag for 20mag/sq." iso. ell. mag. 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 coadd 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 coadd 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.
127	k_r_i20e	L	5.1f	arcsec	K 20mag/sq." isophotal elliptical ap. semi-major axis.
128	k_m_i20e	L	6.3f	mag	K 20mag/sq." isophotal elliptical ap. magnitude.
129	k_msig_i20e	L	5.3f	mag	K 1-sigma uncertainty in 20mag/sq." iso. ell. mag.
130	k_flg_i20e	L	1hd	-	K confusion flag for 20mag/sq." iso. ell. mag. 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 coadd 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 coadd 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.
---	Isophotal photom at 20 mag/sq.arcsec using circ ap
131	j_r_i20c	L	5.1f	arcsec	J 20mag/sq." isophotal circular aperture radius.
132	j_m_i20c	L	6.3f	mag	J 20mag/sq." isophotal circular ap. magnitude.
133	j_msig_i20c	L	5.3f	mag	J 1-sigma uncertainty in 20mag/sq." iso. circ. mag.
134	j_flg_i20c	L	1hd	-	J confusion flag for 20mag/sq." iso. circ. mag. 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 coadd 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 coadd 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.
135	h_r_i20c	L	5.1f	arcsec	H 20mag/sq." isophotal circular aperture radius.
136	h_m_i20c	L	6.3f	mag	H 20mag/sq." isophotal circular ap. magnitude.
137	h_msig_i20c	L	5.3f	mag	H 1-sigma uncertainty in 20mag/sq." iso. circ. mag.
138	h_flg_i20c	L	1hd	-	H confusion flag for 20mag/sq." iso. circ. mag. 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 coadd 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 coadd 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.
139	k_r_i20c	L	5.1f	arcsec	K 20mag/sq." isophotal circular aperture radius.
140	k_m_i20c	L	6.3f	mag	K 20mag/sq." isophotal circular ap. magnitude.
141	k_msig_i20c	L	5.3f	mag	K 1-sigma uncertainty in 20mag/sq." iso. circ. mag.
142	k_flg_i20c	L	1hd	-	K confusion flag for 20mag/sq." iso. circ. mag. 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 coadd 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 coadd 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.
---	Isophotal photom at 21 mag/sq.arcsec using ell ap
143	j_r_i21e	L	5.1f	arcsec	J 21mag/sq." isophotal elliptical ap. semi-major axis.
144	j_m_i21e	L	6.3f	mag	J 21mag/sq." isophotal elliptical ap. magnitude.
145	j_msig_i21e	L	5.3f	mag	J 1-sigma uncertainty in 21mag/sq." iso. ell. mag.
146	j_flg_i21e	L	1hd	-	J confusion flag for 21mag/sq." iso. ell. mag. 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 coadd 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 coadd 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.
147	h_r_i21e	L	5.1f	arcsec	H 21mag/sq." isophotal elliptical ap. semi-major axis.
148	h_m_i21e	L	6.3f	mag	H 21mag/sq." isophotal elliptical ap. magnitude.
149	h_msig_i21e	L	5.3f	mag	H 1-sigma uncertainty in 21mag/sq." iso. ell. mag.
150	h_flg_i21e	L	1hd	-	H confusion flag for 21mag/sq." iso. ell. mag. 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 coadd 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 coadd 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.
151	k_r_i21e	L	5.1f	arcsec	K 21mag/sq." isophotal elliptical ap. semi-major axis.
152	k_m_i21e	L	6.3f	mag	K 21mag/sq." isophotal elliptical ap. magnitude.
153	k_msig_i21e	L	5.3f	mag	K 1-sigma uncertainty in 21mag/sq." iso. ell. mag.
154	k_flg_i21e	L	1hd	-	K confusion flag for 21mag/sq." iso. ell. mag. 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 coadd 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 coadd 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.
---	Isophotal photom at 21 using J fiducial ellip ap
155	r_j21fe	L	5.1f	arcsec	21mag/sq." isophotal J fiducial ell. ap. semi-major axis. "Fiducial" apertures are determined for each type of total and isophotal photometry measurements. 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.
156	j_m_j21fe	L	6.3f	mag	J 21mag/sq." isophotal fiducial ell. ap. magnitude.
157	j_msig_j21fe	L	5.3f	mag	J 1-sigma uncertainty in 21mag/sq." iso.fid.ell.mag.
158	j_flg_j21fe	L	1hd	-	J confusion flag for 21mag/sq." iso. fid. ell. mag. 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 coadd 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 coadd 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.
159	h_m_j21fe	L	6.3f	mag	H 21mag/sq." isophotal fiducial ell. ap. magnitude.
160	h_msig_j21fe	L	5.3f	mag	H 1-sigma uncertainty in 21mag/sq." iso.fid.ell.mag.
161	h_flg_j21fe	L	1hd	-	H confusion flag for 21mag/sq." iso. fid. ell. mag. 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 coadd 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 coadd 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	k_m_j21fe	L	6.3f	mag	K 21mag/sq." isophotal fiducial ell. ap. magnitude.
163	k_msig_j21fe	L	5.3f	mag	K 1-sigma uncertainty in 21mag/sq." iso.fid.ell.mag.
164	k_flg_j21fe	L	1hd	-	K confusion flag for 21mag/sq." iso. fid. ell. mag. 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 coadd 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 coadd 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.
---	Isophotal photom at 21 using circ ap
165	j_r_i21c	L	5.1f	arcsec	J 21mag/sq." isophotal circular aperture radius.
166	j_m_i21c	L	6.3f	mag	J 21mag/sq." isophotal circular ap. magnitude.
167	j_msig_i21c	L	5.3f	mag	J 1-sigma uncertainty in 21mag/sq." iso. circ. mag.
168	j_flg_i21c	L	1hd	-	J confusion flag for 21mag/sq." iso. circ. mag. 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 coadd 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 coadd 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.
169	h_r_i21c	L	5.1f	arcsec	H 21mag/sq." isophotal circular aperture radius.
170	h_m_i21c	L	6.3f	mag	H 21mag/sq." isophotal circular ap. magnitude.
171	h_msig_i21c	L	5.3f	mag	H 1-sigma uncertainty in 21mag/sq." iso. circ. mag.
172	h_flg_i21c	L	1hd	-	H confusion flag for 21mag/sq." iso. circ. mag. 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 coadd 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 coadd 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.
173	k_r_i21c	L	5.1f	arcsec	K 21mag/sq." isophotal circular aperture radius.
174	k_m_i21c	L	6.3f	mag	K 21mag/sq." isophotal circular ap. magnitude.
175	k_msig_i21c	L	5.3f	mag	K 1-sigma uncertainty in 21mag/sq." iso. circ. mag.
176	k_flg_i21c	L	1hd	-	K confusion flag for 21mag/sq." iso. circ. mag. 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 coadd 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 coadd 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.
---	Isophotal photom at 21 mag/sq.arcsec using J fiducial circ ap
177	r_j21fc	L	5.1f	arcsec	21mag/sq." isophotal J fiducial circular ap. radius. "Fiducial" apertures are determined for each type of total and isophotal photometry measurements. 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.
178	j_m_j21fc	L	6.3f	mag	J 21mag/sq." isophotal fiducial circ. ap. mag.
179	j_msig_j21fc	L	5.3f	mag	J 1-sigma uncertainty in 21mag/sq." iso.fid.circ.mag.
180	j_flg_j21fc	L	1hd	-	J confusion flag for 21mag/sq." iso. fid. circ. mag. 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 coadd 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 coadd 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.
181	h_m_j21fc	L	6.3f	mag	H 21mag/sq." isophotal fiducial circ. ap. mag.
182	h_msig_j21fc	L	5.3f	mag	H 1-sigma uncertainty in 21mag/sq." iso.fid.circ.mag.
183	h_flg_j21fc	L	1hd	-	H confusion flag for 21mag/sq." iso. fid. circ. mag. 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 coadd 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 coadd 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.
184	k_m_j21fc	L	6.3f	mag	K 21mag/sq." isophotal fiducial circ. ap. mag.
185	k_msig_j21fc	L	5.3f	mag	K 1-sigma uncertainty in 21mag/sq." iso.fid.circ.mag.
186	k_flg_j21fc	L	1hd	-	K confusion flag for 21mag/sq." iso. fid. circ. mag. 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 coadd 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 coadd 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.
---	Photometry from fixed circular aperture
187	j_m_5	L	6.3f	mag	J 5 arcsec radius circular aperture magnitude.
188	j_msig_5	L	5.3f	mag	J 1-sigma uncertainty in 5 arcsec circular ap. mag.
189	j_flg_5	L	1hd	-	J confusion flag for 5 arcsec circular ap. mag. 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 coadd 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 coadd 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.
190	h_m_5	L	6.3f	mag	H 5 arcsec radius circular aperture magnitude.
191	h_msig_5	L	5.3f	mag	H 1-sigma uncertainty in 5 arcsec circular ap. mag.
192	h_flg_5	L	1hd	-	H confusion flag for 5 arcsec circular ap. mag. 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 coadd 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 coadd 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.
193	k_m_5	L	6.3f	mag	K 5 arcsec radius circular aperture magnitude.
194	k_msig_5	L	5.3f	mag	K 1-sigma uncertainty in 5 arcsec circular ap. mag.
195	k_flg_5	L	1hd	-	K confusion flag for 5 arcsec circular ap. mag. 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 coadd 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 coadd 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	j_m_7	L	6.3f	mag	J 7 arcsec radius circular aperture magnitude.
197	j_msig_7	L	5.3f	mag	J 1-sigma uncertainty in 7 arcsec circular ap. mag.
198	j_flg_7	L	1hd	-	J confusion flag for 7 arcsec circular ap. mag. 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 coadd 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 coadd 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.
199	h_m_7	L	6.3f	mag	H 7 arcsec radius circular aperture magnitude.
200	h_msig_7	L	5.3f	mag	H 1-sigma uncertainty in 7 arcsec circular ap. mag.
201	h_flg_7	L	1hd	-	H confusion flag for 7 arcsec circular ap. mag. 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 coadd 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 coadd 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.
202	k_m_7	L	6.3f	mag	K 7 arcsec radius circular aperture magnitude.
203	k_msig_7	L	5.3f	mag	K 1-sigma uncertainty in 7 arcsec circular ap. mag.
204	k_flg_7	L	1hd	-	K confusion flag for 7 arcsec circular ap. mag. 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 coadd 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 coadd 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	j_m_10	L	6.3f	mag	J 10 arcsec radius circular aperture magnitude.
206	j_msig_10	L	5.3f	mag	J 1-sigma uncertainty in 10 arcsec circular ap. mag.
207	j_flg_10	L	1hd	-	J confusion flag for 10 arcsec circular ap. mag. 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 coadd 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 coadd 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.
208	h_m_10	L	6.3f	mag	H 10 arcsec radius circular aperture magnitude.
209	h_msig_10	L	5.3f	mag	H 1-sigma uncertainty in 10 arcsec circular ap. mag.
210	h_flg_10	L	1hd	-	H confusion flag for 10 arcsec circular ap. mag. 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 coadd 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 coadd 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.
211	k_m_10	L	6.3f	mag	K 10 arcsec radius circular aperture magnitude.
212	k_msig_10	L	5.3f	mag	K 1-sigma uncertainty in 10 arcsec circular ap. mag.
213	k_flg_10	L	1hd	-	K confusion flag for 10 arcsec circular ap. mag. 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 coadd 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 coadd 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	j_m_15	L	6.3f	mag	J 15 arcsec radius circular aperture magnitude.
215	j_msig_15	L	5.3f	mag	J 1-sigma uncertainty in 15 arcsec circular ap. mag.
216	j_flg_15	L	1hd	-	J confusion flag for 15 arcsec circular ap. mag. 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 coadd 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 coadd 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.
217	h_m_15	L	6.3f	mag	H 15 arcsec radius circular aperture magnitude.
218	h_msig_15	L	5.3f	mag	H 1-sigma uncertainty in 15 arcsec circular ap. mag.
219	h_flg_15	L	1hd	-	H confusion flag for 15 arcsec circular ap. mag. 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 coadd 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 coadd 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.
220	k_m_15	L	6.3f	mag	K 15 arcsec radius circular aperture magnitude.
221	k_msig_15	L	5.3f	mag	K 1-sigma uncertainty in 15 arcsec circular ap. mag.
222	k_flg_15	L	1hd	-	K confusion flag for 15 arcsec circular ap. mag. 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 coadd 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 coadd 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	j_m_20	L	6.3f	mag	J 20 arcsec radius circular aperture magnitude.
224	j_msig_20	L	5.3f	mag	J 1-sigma uncertainty in 20 arcsec circular ap. mag.
225	j_flg_20	L	1hd	-	J confusion flag for 20 arcsec circular ap. mag. 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 coadd 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 coadd 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.
226	h_m_20	L	6.3f	mag	H 20 arcsec radius circular aperture magnitude.
227	h_msig_20	L	5.3f	mag	H 1-sigma uncertainty in 20 arcsec circular ap. mag.
228	h_flg_20	L	1hd	-	H confusion flag for 20 arcsec circular ap. mag. 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 coadd 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 coadd 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.
229	k_m_20	L	6.3f	mag	K 20 arcsec radius circular aperture magnitude.
230	k_msig_20	L	5.3f	mag	K 1-sigma uncertainty in 20 arcsec circular ap. mag.
231	k_flg_20	L	1hd	-	K confusion flag for 20 arcsec circular ap. mag. 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 coadd 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 coadd 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	j_m_25	L	6.3f	mag	J 25 arcsec radius circular aperture magnitude.
233	j_msig_25	L	5.3f	mag	J 1-sigma uncertainty in 25 arcsec circular ap. mag.
234	j_flg_25	L	1hd	-	J confusion flag for 25 arcsec circular ap. mag. 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 coadd 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 coadd 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.
235	h_m_25	L	6.3f	mag	H 25 arcsec radius circular aperture magnitude.
236	h_msig_25	L	5.3f	mag	H 1-sigma uncertainty in 25 arcsec circular ap. mag.
237	h_flg_25	L	1hd	-	H confusion flag for 25 arcsec circular ap. mag. 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 coadd 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 coadd 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.
238	k_m_25	L	6.3f	mag	K 25 arcsec radius circular aperture magnitude.
239	k_msig_25	L	5.3f	mag	K 1-sigma uncertainty in 25 arcsec circular ap. mag.
240	k_flg_25	L	1hd	-	K confusion flag for 25 arcsec circular ap. mag. 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 coadd 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 coadd 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	j_m_30	L	6.3f	mag	J 30 arcsec radius circular aperture magnitude.
242	j_msig_30	L	5.3f	mag	J 1-sigma uncertainty in 30 arcsec circular ap. mag.
243	j_flg_30	L	1hd	-	J confusion flag for 30 arcsec circular ap. mag. 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 coadd 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 coadd 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.
244	h_m_30	L	6.3f	mag	H 30 arcsec radius circular aperture magnitude.
245	h_msig_30	L	5.3f	mag	H 1-sigma uncertainty in 30 arcsec circular ap. mag.
246	h_flg_30	L	1hd	-	H confusion flag for 30 arcsec circular ap. mag. 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 coadd 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 coadd 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.
247	k_m_30	L	6.3f	mag	K 30 arcsec radius circular aperture magnitude.
248	k_msig_30	L	5.3f	mag	K 1-sigma uncertainty in 30 arcsec circular ap. mag.
249	k_flg_30	L	1hd	-	K confusion flag for 30 arcsec circular ap. mag. 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 coadd 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 coadd 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	j_m_40	L	6.3f	mag	J 40 arcsec radius circular aperture magnitude.
251	j_msig_40	L	5.3f	mag	J 1-sigma uncertainty in 40 arcsec circular ap. mag.
252	j_flg_40	L	1hd	-	J confusion flag for 40 arcsec circular ap. mag. 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 coadd 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 coadd 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.
253	h_m_40	L	6.3f	mag	H 40 arcsec radius circular aperture magnitude.
254	h_msig_40	L	5.3f	mag	H 1-sigma uncertainty in 40 arcsec circular ap. mag.
255	h_flg_40	L	1hd	-	H confusion flag for 40 arcsec circular ap. mag. 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 coadd 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 coadd 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.
256	k_m_40	L	6.3f	mag	K 40 arcsec radius circular aperture magnitude.
257	k_msig_40	L	5.3f	mag	K 1-sigma uncertainty in 40 arcsec circular ap. mag.
258	k_flg_40	L	1hd	-	K confusion flag for 40 arcsec circular ap. mag. 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 coadd 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 coadd 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	j_m_50	L	6.3f	mag	J 50 arcsec radius circular aperture magnitude.
260	j_msig_50	L	5.3f	mag	J 1-sigma uncertainty in 50 arcsec circular ap. mag.
261	j_flg_50	L	1hd	-	J confusion flag for 50 arcsec circular ap. mag. 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 coadd 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 coadd 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.
262	h_m_50	L	6.3f	mag	H 50 arcsec radius circular aperture magnitude.
263	h_msig_50	L	5.3f	mag	H 1-sigma uncertainty in 50 arcsec circular ap. mag.
264	h_flg_50	L	1hd	-	H confusion flag for 50 arcsec circular ap. mag. 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 coadd 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 coadd 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.
265	k_m_50	L	6.3f	mag	K 50 arcsec radius circular aperture magnitude.
266	k_msig_50	L	5.3f	mag	K 1-sigma uncertainty in 50 arcsec circular ap. mag.
267	k_flg_50	L	1hd	-	K confusion flag for 50 arcsec circular ap. mag. 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 coadd 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 coadd 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	j_m_60	L	6.3f	mag	J 60 arcsec radius circular aperture magnitude.
269	j_msig_60	L	5.3f	mag	J 1-sigma uncertainty in 60 arcsec circular ap. mag.
270	j_flg_60	L	1hd	-	J confusion flag for 60 arcsec circular ap. mag. 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 coadd 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 coadd 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.
271	h_m_60	L	6.3f	mag	H 60 arcsec radius circular aperture magnitude.
272	h_msig_60	L	5.3f	mag	H 1-sigma uncertainty in 60 arcsec circular ap. mag.
273	h_flg_60	L	1hd	-	H confusion flag for 60 arcsec circular ap. mag. 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 coadd 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 coadd 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.
274	k_m_60	L	6.3f	mag	K 60 arcsec radius circular aperture magnitude.
275	k_msig_60	L	5.3f	mag	K 1-sigma uncertainty in 60 arcsec circular ap. mag.
276	k_flg_60	L	1hd	-	K confusion flag for 60 arcsec circular ap. mag. 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 coadd 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 coadd 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.
277	j_m_70	L	6.3f	mag	J 70 arcsec radius circular aperture magnitude.
278	j_msig_70	L	5.3f	mag	J 1-sigma uncertainty in 70 arcsec circular ap. mag.
279	j_flg_70	L	1hd	-	J confusion flag for 70 arcsec circular ap. mag. 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 coadd 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 coadd 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.
280	h_m_70	L	6.3f	mag	H 70 arcsec radius circular aperture magnitude.
281	h_msig_70	L	5.3f	mag	H 1-sigma uncertainty in 70 arcsec circular ap. mag.
282	h_flg_70	L	1hd	-	H confusion flag for 70 arcsec circular ap. mag. 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 coadd 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 coadd 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.
283	k_m_70	L	6.3f	mag	K 70 arcsec radius circular aperture magnitude.
284	k_msig_70	L	5.3f	mag	K 1-sigma uncertainty in 70 arcsec circular ap. mag.
285	k_flg_70	L	1hd	-	K confusion flag for 70 arcsec circular ap. mag. 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 coadd 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 coadd 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.
---	System photometry
286	j_m_sys	L	6.3f	mag	J system photometry magnitude. 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.
287	j_msig_sys	L	5.3f	mag	J 1-sigma uncertainty in system photometry mag.
288	h_m_sys	L	6.3f	mag	H system photometry magnitude. 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.
289	h_msig_sys	L	5.3f	mag	H 1-sigma uncertainty in system photometry mag.
290	k_m_sys	L	6.3f	mag	K system photometry magnitude. 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.
291	k_msig_sys	L	5.3f	mag	K 1-sigma uncertainty in system photometry mag.
292	sys_flg	L	1hd	-	system flag: 0=no system, 1=nearby galaxy flux incl. in mag.
293	contam_flg	L	1hd	-	contamination flag: 0=no stars, 1=stellar flux incl. in mag.
---	5-sigma area ratios
294	j_5sig_ba	L	5.3f	-	J minor/major axis ratio fit to the 5-sigma isophote.
295	j_5sig_phi	L	3hd	deg	J angle to 5-sigma major axis (E of N).
296	h_5sig_ba	L	5.3f	-	H minor/major axis ratio fit to the 5-sigma isophote.
297	h_5sig_phi	L	3hd	deg	H angle to 5-sigma major axis (E of N).
298	k_5sig_ba	L	5.3f	-	K minor/major axis ratio fit to the 5-sigma isophote.
299	k_5sig_phi	L	3hd	deg	K angle to 5-sigma major axis (E of N).
---	5-sigma to 3-sigma area
300	j_d_area	L	3hd	-	J 5-sigma to 3-sigma differential area.
301	j_perc_darea	L	3hd	-	J 5-sigma to 3-sigma percent area change.
302	h_d_area	L	3hd	-	H 5-sigma to 3-sigma differential area.
303	h_perc_darea	L	3hd	-	H 5-sigma to 3-sigma percent area change.
304	k_d_area	L	3hd	-	K 5-sigma to 3-sigma differential area.
305	k_perc_darea	L	3hd	-	K 5-sigma to 3-sigma percent area change.
---	Bi-symmetric quantities
306	j_bisym_rat	L	5.3f	-	J bi-symmetric flux ratio.
307	j_bisym_chi	L	6.3f	-	J bi-symmetric cross-correlation chi.
308	h_bisym_rat	L	5.3f	-	H bi-symmetric flux ratio.
309	h_bisym_chi	L	6.3f	-	H bi-symmetric cross-correlation chi.
310	k_bisym_rat	L	5.3f	-	K bi-symmetric flux ratio.
311	k_bisym_chi	L	6.3f	-	K bi-symmetric cross-correlation chi.
---	Parameters for extended src discrimination from point srcs
312	j_sh0	L	5.2f	-	J ridge shape (LCSB: BSNR limit).
313	j_sig_sh0	L	5.2f	-	J ridge shape sigma (LCSB: B2SNR limit).
314	h_sh0	L	5.2f	-	H ridge shape (LCSB: BSNR limit).
315	h_sig_sh0	L	5.2f	-	H ridge shape sigma (LCSB: B2SNR limit).
316	k_sh0	L	5.2f	-	K ridge shape (LCSB: BSNR limit).
317	k_sig_sh0	L	5.2f	-	K ridge shape sigma (LCSB: B2SNR limit).
318	j_sc_mxdn	L	6.1f	-	J mxdn (score) (LCSB: BSNR - block/smoothed SNR).
319	j_sc_sh	L	6.1f	-	J shape (score).
320	j_sc_wsh	L	6.1f	-	J wsh (score) (LCSB: PSNR - peak raw SNR).
321	j_sc_r23	L	6.1f	-	J r23 (score) (LCSB: TSNR - integrated SNR for r=15).
322	j_sc_1mm	L	6.1f	-	J 1st moment (score) (LCSB: super blk 2,4,8 SNR).
323	j_sc_2mm	L	6.1f	-	J 2nd moment (score) (LCSB: SNRMAX - super SNR max).
324	j_sc_vint	L	6.1f	-	J vint (score).
325	j_sc_r1	L	6.1f	-	J r1 (score).
326	j_sc_msh	L	6.1f	-	J median shape score.
327	h_sc_mxdn	L	6.1f	-	H mxdn (score) (LCSB: BSNR - block/smoothed SNR).
328	h_sc_sh	L	6.1f	-	H shape (score).
329	h_sc_wsh	L	6.1f	-	H wsh (score) (LCSB: PSNR - peak raw SNR).
330	h_sc_r23	L	6.1f	-	H r23 (score) (LCSB: TSNR - integrated SNR for r=15).
331	h_sc_1mm	L	6.1f	-	H 1st moment (score) (LCSB: super blk 2,4,8 SNR).
332	h_sc_2mm	L	6.1f	-	H 2nd moment (score) (LCSB: SNRMAX - super SNR max).
333	h_sc_vint	L	6.1f	-	H vint (score).
334	h_sc_r1	L	6.1f	-	H r1 (score).
335	h_sc_msh	L	6.1f	-	H median shape score.
336	k_sc_mxdn	L	6.1f	-	K mxdn (score) (LCSB: BSNR - block/smoothed SNR).
337	k_sc_sh	L	6.1f	-	K shape (score).
338	k_sc_wsh	L	6.1f	-	K wsh (score) (LCSB: PSNR - peak raw SNR).
339	k_sc_r23	L	6.1f	-	K r23 (score) (LCSB: TSNR - integrated SNR for r=15).
340	k_sc_1mm	L	6.1f	-	K 1st moment (score) (LCSB: super blk 2,4,8 SNR).
341	k_sc_2mm	L	6.1f	-	K 2nd moment (score) (LCSB: SNRMAX - super SNR max).
342	k_sc_vint	L	6.1f	-	K vint (score).
343	k_sc_r1	L	6.1f	-	K r1 (score).
344	k_sc_msh	L	6.1f	-	K median shape score.
345	j_chif_ellf	L	6.1f	-	J % chi-fraction for elliptical fit to 3-sig isophote.
346	k_chif_ellf	L	6.1f	-	K % chi-fraction for elliptical fit to 3-sig isophote.
347	ellfit_flg	L	1hd	-	ellipse fitting contamination flag.
348	sup_chif_ellf	L	6.1f	-	super-coadd % chi-fraction for ellip. fit to 3-sig isophote.
---	Coadd background, brightness
349	n_blank	L	4hd	-	number of blanked source records. These parameters refer to sources that were blanked and/or subtracted from the images before doing photometry. Data for each of these blanked or subtracted sources are found in the blanked and subtracted source tables.
350	n_sub	L	4hd	-	number of subtracted source records. These parameters refer to sources that were blanked and/or subtracted from the images before doing photometry. Data for each of these blanked or subtracted sources are found in the blanked and subtracted source tables.
351	bl_sub_flg	L	1hd	-	blanked/subtracted src description flag.
---	Other miscellaneous parameters
352	id_flg	L	1hd	-	type/galaxy ID flag (0=non-catalog, 1=catalog, 2=LCSB). 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
353	id_cat	L	20s	-	matched galaxy's catalog name.
354	fg_flg	L	6s	-	flux-growth convergence flag.
355	blk_fac	L	1hd	-	LCSB blocking factor (1, 2, 4, 8).
356	dist_edge_ns	L	%5d	arcsec	The distance from the source to the nearest North or South scan edge. The scan edge is defined by the great-circle interpolation between the 3-band coverage corners. The equatorial coordinates of the 3-band coverage corners are given in the Scan Information Table, referenced by the scan_key. The first character of the dist_edge_flg indicates to which edge the source is closer.
357	dist_edge_ew	L	%3d	arcsec	The distance from the source to the nearest East or West scan edge. The scan edge is defined by the great-circle interpolation between the 3-band coverage corners. The equatorial coordinates of the 3-band coverage corners are given in the Scan Information Table, referenced by the scan_key. The second character of the dist_edge_flg indicates to which edge the source is closer.
358	dist_edge_flg	L	%2s	-	flag indicating which edges ([n\|s][e\|w]) are nearest to src.
359	pts_key	L	10d	-	key to calibration scan point source WDB record. If the source has point source data (i.e. it is not an LCSB), this field will be set to the key of the record in the point source table containing the point source data. The point source data will also have the same date, hemisphere, scan, id keys.
360	mp_key	L	5d	-	key to minor planet prediction DB record. If a minor planet (asteroid) is predicted at this src's position, the field is set to the key of the record containing the minor planet prediction data (see the minor planet tbls). The minor planet data will also have the same date, hemisphere, scan, id keys.
361	scan_key	S	6d	-	key to scan data record in "scan DB". This field is set to the key of the record containing the corresponding scan data in the scan data table. The records will also have the same date, hemisphere, scan keys.
362	coadd_key	L	7d	-	key to coadd data record in "scan DB". This field is set to the key of the record containing the corresponding J, H, and K band coadd data in the coadd data table. The records will also have the same date, hemisphere, scan, coadd keys.
363	hemis	L	1s	-	hemisphere (N/S) of observation. "n" = North/Mt. Hopkins; "s" = South/CTIO.
364	date	L	yyyy-mm-dd	-	The observation reference date for this source expressed in ISO standard format. This is the UT day value at sunrise for the night on which the source was observed. Because it is possible for the UT day to change during a night of observations, the actual UT date for a source measurement can differ from date by one day. Use the Julian Day value (jdate) for a more accurate determination of the observation time of the source.
365	scan	L	3hd	-	scan number (unique within date).
366	coadd	L	03hd	-	3-digit coadd number (unique within scan).
367	id	L	6d	-	source ID number (unique within scan, coadd).
368	x_coadd	L	6.1f	arcsec	x (cross-scan) position (coadd coord.).
369	y_coadd	L	6.1f	arcsec	y (in-scan) position (coadd coord.).
370	j_subst2	L	6.1f	-	J residual background #2 (score).
371	h_subst2	L	6.1f	-	H residual background #2 (score).
372	k_subst2	L	6.1f	-	K residual background #2 (score).
373	j_back	L	6.1f	-	J coadd median background.
374	h_back	L	6.1f	-	H coadd median background.
375	k_back	L	6.1f	-	K coadd median background.
376	j_resid_ann	L	7.3f	DN	J residual annulus background median.
377	h_resid_ann	L	7.3f	DN	H residual annulus background median.
378	k_resid_ann	L	7.3f	DN	K residual annulus background median.
379	j_bndg_per	L	5d	arcsec	J banding Fourier Transf. period on this side of coadd.
380	j_bndg_amp	L	6.3f	DN	J banding maximum FT amplitude on this side of coadd.
381	h_bndg_per	L	5d	arcsec	H banding Fourier Transf. period on this side of coadd.
382	h_bndg_amp	L	6.3f	DN	H banding maximum FT amplitude on this side of coadd.
383	k_bndg_per	L	5d	arcsec	K banding Fourier Transf. period on this side of coadd.
384	k_bndg_amp	L	6.3f	DN	K banding maximum FT amplitude on this side of coadd.
385	j_seetrack	L	4.1f	-	J band seetracking score.
386	h_seetrack	L	4.1f	-	H band seetracking score.
387	k_seetrack	L	4.1f	-	K band seetracking score.
388	ext_key/cntr	S	9d	-	entry counter (key) number (unique within table).

[Last Updated: 2008 February 18; by T. Jarrett and R. Cutri]

Return to Section A4.3