<=== observer ===>
"EVDISHOE",\
"van Dishoeck, E.F.",\
"",\
"Leiden Observatory",\
"",\
"P.O. Box 9513",\
"2300 RA",\
"Leiden",\
"The Netherlands",\
"31 71 275874",\
"31 71 275819",\
"ewine@strwchem.leidenuniv.nl"
<=== proposal ===>
"MOLSPEC", 1, 2,\
{"abundances",\
"molecular clouds",\
"young stellar objects",\
"star formation"},\
{"Th. De Graauw",\
"SRON Groningen",\
"P.O.-Box 800",\
"9700 AV Groningen",\
"The Netherlands",\
"thijsdg@sron.rug.nl",\
"F.P. Helmich",\
"Leiden Observatory",\
"SRON Groningen",\
"P.O.-Box 9513",\
"2300 RA Leiden",\
"The Netherlands",\
"fph@strw.leidenuniv.",\
"J.H. Black",\
"Steward Observatory",\
"Univ. of Arizona",\
"Tucson AZ85721",\
"USA",\
"black@as.arizona.edu"}
<=== title ===>
MOLECULAR SPECTROSCOPY OF GAS-PHASE SPECIES:
A PILOT STUDY WITH THE SWS
<=== abstract ===>
SCIENTIFIC ABSTRACT
We propose to use the ISO-SWS to observe a number of lines of
gas-phase interstellar and circumstellar molecules in the 2.5-45
micron range. The objective is to study the abundance and
excitation of these species in a variety of sources and to assess their
diagnostic capabilities both for the chemical and physical conditions.
Key molecules for observation are H2, HD, H2O, OH, CO2, C2H2, HCCCCH and CH3.
We propose to carry out a significant fraction of these observations at the
beginning of the ISO mission so that the results can be fed back into the
other SWS observations. The total amount of time for this proposal is
29.75 hours in case of the Sagittarius hole (spring launch) and 29.25 hours
in case of the Orion hole (autumn launch).
The proposal is divided into three parts:
1. Absorption line studies of vibration-rotation lines of gas-phase
interstellar molecules. Most of the observing time
will be spent on this part of the proposal, and it is the gas-phase
complement of the Whittet et al. dust proposal.
The emphasis will be on molecules which have bands in the wavelength region
covered by the Fabry-Perot. The most important species are CO2, which is
expected to be a sensitive diagnostic of grain-surface chemistry; CH3, which
is an important cornerstone of the carbon chemistry network; and C2H2
(acetylene) and HCCCCH (di-acetylene), which are both good chemical and
temperature diagnostics. These molecules (and their isotopes) cannot be
observed through millimeter emission lines, and most of their infrared lines
lie in wavelength regions that are not observable from the ground. In
addition, for most lines of sight observations of the principal rotational
lines of H2 and in some cases HD will be attempted. Molecules such as C2H,
HCN, SO2 and SiS have already been detected through millimeter observations,
but the infrared absorption lines will give valuable complementary information
on the excitation. A few more complex organic molecules such as ethane will be
searched for in only 1-2 sources. The H2, HD, CO2 and H2O observations toward
Orion IRc2 or SgrA-W will be performed in collaboration with the Garching
group. In order to constrain the elemental abundances, we have added
observations of the fine-structure lines of O I, C II, Fe II, Fe I, Si II and
S I.
2. Absorption lines of H2, CO2, CH3, C2H2 and HCCCCH with the Fabry-Perot
toward IRC +10216.
3. Emission line studies of H2, HD, OH and H2O pure rotational lines and
atomic fine structure lines in selected objects. The amount of time for this
part will be about 4-5 hours.
The emphasis is here on the diagnostic capabilities of these molecules
in a variety of objects (including shocks, PDRs, and star-forming
regions), for comparison with excitation models already developed by the
authors.
OBSERVATION SUMMARY
The lines and bands of the various molecules that we propose to observe are
summarized in the Tables at the end of the Scientific Justification section.
For the absorption and circumstellar part, the integration times are such that
a S/N of at least 100 (but often significantly more) on the continuum is
reached with the grating. For the Fabry-Perot, the required S/N on the
continuum is typically 50-100, and occasionally up to 200 (H2 and CO2 toward
W3IRS5, IRC+10216). The grating observations will be observed in parallel with
the Fabry-Perot observations using SWS AOT07. Complementary observations of
the OH, H2O, O and HD lines at longer wavelengths will be made with the
Fabry-Perot LWS AOT04. The integration time per LWS line is taken to be 2 min,
so that a S/N>100 on the continuum is reached for all sources (using 3 res
elements on either side of the line with 4 spectral samples per resolution
element in the fast scanning mode).
For the emission part, the requested S/N varies from 10 (H2 lines at 2 mu) to
>100 (H2 lines at 17, 28 mu). A few of the strongest lines will also be
observed with the Fabry Perot. At longer wavelengths, a complete medium
resolution line scan with the LWS AOT01 will be taken for IC 63, IC 443 and
DR21 FIR1. In addition, for IC 443 and DR21, LWS Fabry-Perot measurements of
lines of OH, H2O, HD and O will made with AOT04, whereas OH, HD and O lines
will be observed for HH 7. The integration time per LWS line is again taken to
be 2 min, resulting in S/N>10 on the expected line strength. Note that the
predicted strengths of the H2O and OH lines are particularly uncertain, due to
unknown abundances, excitation effects and beam filling factors. Concatenation
is required for all SWS AOT02 and AOT07 observations to ensure that the
orientation/position angle of the SWS slit on the source is the same. It is
recommended for SWS and LWS observations on the same source to save overhead
for slewing. Please contact the PI in case of scheduling problems due to
long integration times.
<=== scientific_justification ===>
Time distribution for autumn launch targets:
TEAM: total top 40% second 30% last 30%
SWS : 105300 63005 28177 14118
Time distribution for spring launch targets:
TEAM: total top 40% second 30% last 30%
SWS : 107100 53302 34717 19081
Autumn Launch
Name RA Dec epoch Solar AOT Grade Time
Conc.
1 Sgr A-W IRS3 17 42 28.9 -28 59 14 1950.0 N SWS07 1 15281 2
2 Sgr A-W IRS3 17 42 28.9 -28 59 14 1950.0 N SWS07 1 4165 3
3 Sgr A-W IRS3 17 42 28.9 -28 59 14 1950.0 N LWS04 1 2420 0
4 W3 IRS5 02 21 53.4 +61 52 21 1950.0 N SWS07 1 16021 5
5 W3 IRS5 02 21 53.4 +61 52 21 1950.0 N LWS01 1 500 6
6 W3 IRS5 02 21 53.4 +61 52 21 1950.0 N LWS04 1 3620 0
7 GL 2591 NIRS01 20 27 35.8 +40 01 14 1950.0 N SWS07 1 19418 8
8 GL 2591 NIRS01 20 27 35.8 +40 01 14 1950.0 N LWS04 1 1580 0
9 S 140 IRS1 22 17 41.08 +63 03 41.6 1950.0 N SWS07 2 8791 10
10 S 140 IRS1 22 17 41.08 +63 03 41.6 1950.0 N LWS04 2 1580 0
11 GL 2136 18 19 36.6 -13 31 40 1950.0 N SWS07 2 7049 12
12 GL 2136 18 19 36.6 -13 31 40 1950.0 N LWS04 2 1580 0
13 NGC 7538 IRS9 23 11 52.8 +61 10 59 1950.0 N SWS07 3 4705 14
14 NGC 7538 IRS9 23 11 52.8 +61 10 59 1950.0 N LWS04 3 1580 0
15 DR 21 FIR1 20 37 13.4 +42 13 57 1950.0 N SWS02 2 2512 16
16 DR 21 FIR1 20 37 13.4 +42 13 57 1950.0 N SWS07 2 1442 17
17 DR 21 FIR1 20 37 13.4 +42 13 57 1950.0 N LWS01 2 500 18
18 DR 21 FIR1 20 37 13.4 +42 13 57 1950.0 N LWS04 2 1401 0
19 IC 63 00 55 58.0 +60 37 07 1950.0 N SWS02 2 2822 20
20 IC 63 00 55 58.0 +60 37 07 1950.0 N LWS01 2 500 0
21 W51 Main 19 21 26.2 +14 24 43 1950.0 N SWS02 3 1958 22
22 W51 Main 19 21 26.2 +14 24 43 1950.0 N SWS07 3 3226 0
23 IRC +10216 09 45 14.8 +13 30 40 1950.0 N SWS07 3 2649 0
Spring Launch
1 Orion IRc2 05 32 46.8 -05 24 25 1950.0 N SWS07 1 14902 0
2 W3 IRS5 02 21 53.4 +61 52 21 1950.0 N SWS07 1 16021 3
3 W3 IRS5 02 21 53.4 +61 52 21 1950.0 N LWS01 1 500 4
4 W3 IRS5 02 21 53.4 +61 52 21 1950.0 N LWS04 1 3620 0
5 NGC 2024 IRS2 05 39 14.27 -01 55 59 1950.0 N SWS07 2 13824 6
6 NGC 2024 IRS2 05 39 14.27 -01 55 59 1950.0 N LWS04 2 1820 0
7 GL 989 06 38 24.9 +09 32 29 1950.0 N SWS07 1 7842 8
8 GL 989 06 38 24.9 +09 32 29 1950.0 N LWS04 1 1580 0
9 GL 961 W(+E) 06 31 58.81 +04 15 06.8 1950.0 N SWS07 2 7339 0
10 GL 890 06 08 21.4 -06 12 27 1950.0 N SWS07 3 5556 11
11 GL 890 06 08 21.4 -06 12 27 1950.0 N LWS04 3 1580 0
12 GL 490 03 23 38.9 +58 36 33 1950.0 N SWS07 3 7716 13
13 GL 490 03 23 38.9 +58 36 33 1950.0 N LWS04 3 1580 0
14 HH 7 03 26 03.0 +31 05 10 1950.0 N SWS02 2 4552 15
15 HH 7 03 26 03.0 +31 05 10 1950.0 N SWS07 2 2040 16
16 HH 7 03 26 03.0 +31 05 10 1950.0 N LWS04 2 1820 0
17 IC 63 00 55 58.0 +60 37 07 1950.0 N SWS02 2 2822 18
18 IC 63 00 55 58.0 +60 37 07 1950.0 N LWS01 2 500 0
19 IC 443 G 06 13 41.0 +22 33 10 1950.0 N SWS02 1 3320 20
20 IC 443 G 06 13 41.0 +22 33 10 1950.0 N SWS07 1 1766 21
21 IC 443 G 06 13 41.0 +22 33 10 1950.0 N LWS01 1 500 22
22 IC 443 G 06 13 41.0 +22 33 10 1950.0 N LWS04 1 3251 0
23 IRC +10216 09 45 14.8 +13 30 40 1950.0 N SWS07 3 2649 0
COORDINATES (1950)
==================
IC 63 00 55 58 +60 37 07
W3 IRS5 02 21 53.4 +61 52 21
GL 490 03 23 38.9 +58 36 33
HH 7 03 26 03 +31 05 10
Orion IRc2 05 32 46.8 -05 24 25
NGC 2024 IRS2 05 39 14.27 -01 55 59
GL 890 06 08 21.4 -06 12 27
IC 443G 06 13 41.0 +22 33 10
GL 961 W(+E) 06 31 58.81 +04 15 06.8
GL 989 06 38 24.9 +09 32 29
IRC+10216 09 45 14.8 +13 30 40
Sgr A-W IRS3 17 42 28.9 -28 59 14
GL 2136 18 19 36.6 -13 31 40
W51 Main 19 21 26.2 +14 24 43
GL 2591 NIRS01 20 27 35.8 +40 01 14
DR 21 FIR1 20 37 13.4 +42 13 57
S 140 IRS1 22 17 41.08 +63 03 41.6
NGC 7538 IRS9 23 11 52.8 +61 10 59
SUMMARY ABSORPTION LINES
=========================
Sagittarius hole
=========================================================
Source Total time (hr) Priority
---------------------------------------------------------
Orion IRc2 4.1 1*
W3IRS5 5.6 1
N2264 = GL989 2.6 1
N2024 IRS2 4.3 2
GL 961 2.0 2
GL 890 2.0 3
GL 490 2.6 3
----------------------------------------------------------
Orion hole
=========================================================
Source Total time (hr) Priority
---------------------------------------------------------
Sgr A-W 6.1 1*
W3IRS5 5.6 1
GL 2591 5.8 1
GL 2136 2.4 2
S140 2.9 2
N7538 IRS9 1.7 3
-----------------------------------------------------------
* H2, HD, H2O and CO2 observations in collaboration with
Garching group
ABSORPTION PART: Sagittarius hole
==================================
================================================================================
Lambda Line/ Orion W3IRS5 N2024 N2264 GL961 GL490 GL890
Band IRc2 GL989
--------------------------------------------------------------------------------
Grating:
2.64-2.73 H2O v1+v3 + + + + - + -
3.20-3.40 CH4 v3 + - - - - - -
4.20-4.32 CO2 v3 + + + + + + -
5.70-6.60 H2O + H218O v2; + + + + + + +
NH3; H2CO; CS2
6.89-6.99 HDO v2; C2H4 v12 + + + + + + +
7.47-7.77 CH4 v4 + + + + + + +
12.08-12.20 CH3CH3 + + + - + + +
12.20-12.30 H2 S(2) Gar + + + + + +
13.30-13.50 SiS + + - - - - -
13.60-13.80 C2H2 v2 + + + + + + +
13.90-14.20 HCN v2 + + + + + + +
14.30-15.60 CO2 v2 + + + + + + +
15.80-16.00 HCCCCH v8 + + + + + + +
16.00-16.52 CH3 v2 + + + + + + +
16.99-17.07 H2 S(1) Gar + + + + + +
18.00-19.00 SO2 v2 + + + + + + -
19.00-20.50 SO2 v2 + + + + + + -
26.70-27.20 C2H v2 + + + - - - -
28.00-29.00 H2 S(0) Gar + + + + + +
37.20-39.60 CH3OH + + + - - + +
Fabry-Perot:
12.16029 CH3CH3 + + + - - - -
12.14071 CH3CH3 + - - - - - -
12.27861 H2 S(2) Gar + + + - + -
13.42141 SiS R(0) + + - - - - -
13.37866 SiS R(4) + - - - - - -
13.33702 SiS R(8) + + - - - - -
13.70978 C2H2 Q + + + - - - -
13.73068 13CCH2 Q + + + - - - -
14.16050 H13CN Q + - + - - - -
14.98085 CO2 Q + + + + + + +
14.82709 CO2 R(8) + + + - - - -
14.74999 CO2 R(14) - + + - - - -
14.72352 CO2 R(16) + - - - - - -
15.41933 13CO2* + + - - - - -
15.92600 HCCCCH Q + + + - - - -
15.91882 HCCCCH R(0) + + - - - - -
15.84489 HCCCCH R(10) + + - - - - -
16.00080 CH3 R(0,0) + + - - - - -
16.49670 CH3 Q + + + - - - -
17.03483 H2 S(1) Gar + + + + + +
19.75600 SO2 + - - - - - -
19.87900 SO2 + + - - - - -
23.03376 HD R(4) Gar + - - - - -
24.0424 Fe I Gar + + - - - -
25.2490 S I Gar + + - - - -
25.9402 o-H2O Gar + + - - - -
25.9882 Fe II Gar + + + - - -
27.1 C2H + - - - - - -
28.21883 H2 S(0) Gar + + + + + +
28.50197 HD R(3) Gar + + - - - -
28.9138 p-H2O Gar + + - - - +
28.94 OH 7/2-5/2 Gar + - - - - -
29.8366 o-H2O Gar + + - - - -
31.7715 o-H2O Gar + + + - + +
34.6294 OH 5/2-3/2 Gar + + + - + +
34.8140 Si II Gar + + + - - -
35.4710 p-H2O Gar + - - - - -
37.4749 o-H2O Gar + - - - - -
37.70155 HD R(2) Gar + + - - - -
37.51946 CH3OH R1 + + + - - - -
38.93579 CH3OH P1 + + + - - - -
40.6904 o-H2O Gar + + - - + +
43.3393 o-H2O Gar + - - - - -
LWS Fabry Perot:
112.07251 HD R(0) Bal + vD vD - - -
119.4417 OH 5/2-3/2 Bal + + + Cox + +
84.4204 OH 7/2-5/2 Bal + + + - + +
65.2789 OH 9/2-7/2 Bal + - - - - -
163.1243 OH 3/2-1/2 Bal + + + - + +
98.7369 OH 5/2-3/2 Bal + + - - - -
71.2158 OH 7/2-5/2 Bal + - - - - -
79.1817 OH 1/2-3/2 Bal + + - - - -
96.3122 OH 3/2-5/2 Bal + - - - - -
53.3513 OH 3/2-3/2 Bal + - - - - -
48.8168 OH 5/2-5/2 Bal + - - - - -
120.1726 18OH 5/2-3/2 Bal + - - - - -
180.4880 o-H2O 2_21-2_12 Bal + + + - + +
179.5265 o-H2O 2_12-1_01 Bal + + + Cox + +
174.6264 o-H2O 3_03-2_12 Bal + + + - + +
136.4944 o-H2O 3_30-3_21 Bal + - - - - -
134.9346 o-H2O 5_14-5_05 Bal + - - - - -
113.5366 o-H2O 4_14-3_03 Bal + - - - - -
108.0730 o-H2O 2_21-1_10 Bal + + + Cox + +
99.4924 o-H2O 5_05-4_14 Bal + - - - - -
78.7414 o-H2O 4_23-3_12 Bal + - - - - -
82.0304 o-H2O 6_16-5_05 Bal + - - - - -
75.3804 o-H2O 3_21-2_12 Bal + + + Cox + +
66.4372 o_H2O 3_30-2_21 Bal + - - - - -
156.1930 p-H2O 3_22-3_13 Bal + - - - - -
138.5272 p-H2O 3_13-2_02 Bal + - - Cox - -
126.7126 p-H2O 3_31-3_22 Bal - - - - - -
100.9828 p-H2O 2_20-1_11 Bal + + + Cox + +
181.0512 o-H218O 2_12-1_01 Bal + + + Cox + +
109.3470 o-H218O 2_21-1_10 Bal + - - - - -
102.0044 p-H218O 2_20-1_11 Bal + - - - - -
63.1700 O I 1-2 Bal - + + - + +
145.5255 O I 0-1 Bal - + + - + +
157.7410 C II Bal - + + - + +
==============================================================================
ABSORPTION PART: Orion hole
==================================
================================================================================
Lambda Line/ Sgr A-W W3IRS5 GL2591 S140 GL2136 N7538
Band IRS1 IRS9
--------------------------------------------------------------------------------
Grating:
2.64-2.73 H2O v1+v3 - + + + + -
4.20-4.32 CO2 v3 + + + + + +
5.70-6.60 H2O + H218O v2; + + + + + +
NH3; H2CO; CS2
6.89-6.99 HDO v2; C2H4 v12 + + + + + +
7.47-7.77 CH4 v4 + + + + + +
12.08-12.20 CH3CH3 + + + + + +
12.20-12.30 H2 S(2) + + + + + +
13.30-13.50 SiS - + + - - -
13.60-13.80 C2H2 v2 + + + + + +
13.90-14.20 HCN v2 + + + + + +
14.30-15.60 CO2 v2 + + + + + +
15.80-16.00 HCCCCH v8 + + + + + +
16.00-16.52 CH3 v2 + + + + + +
16.99-17.07 H2 S(1) + + + + + +
18.00-19.00 SO2 v2 + + + + + +
19.00-20.50 SO2 v2 + + + + + +
26.70-27.20 C2H v2 + + + - - -
28.00-29.00 H2 S(0) + + + + + +
37.20-39.60 CH3OH + + + + + +
Fabry-Perot:
12.16029 CH3CH3 + + + - - -
12.14071 CH3CH3 - - - - - -
12.27861 H2 S(2) + + + + + -
13.42141 SiS R(0) - + + - - -
13.37866 SiS R(4) - - - - - -
13.33702 SiS R(8) - + + - - -
13.70978 C2H2 Q + + + + - -
13.73068 13CCH2 Q + + + - - -
14.16050 H13CN Q + - + - - -
14.98085 CO2 Q + + + + + -
14.82709 CO2 R(8) + + + - - -
14.74999 CO2 R(14) - + - - - -
14.72352 CO2 R(16) + - + - - -
15.41933 13CO2* + + + - - -
15.92600 HCCCCH Q + + + + - -
15.91882 HCCCCH R(0) - + - - - -
15.84489 HCCCCH R(10) - + - - - -
16.00080 CH3 R(0,0) - + - - - -
16.49670 CH3 Q + + + + - -
17.03483 H2 S(1) + + + + + +
19.75600 SO2 - - - - - -
19.87900 SO2 - + - - - -
23.03376 HD R(4) + + + - - -
24.0424 Fe I - + + - - -
25.2490 S I - + + - - -
25.9402 o-H2O - + + - - -
25.9882 Fe II - + + + - -
27.1 C2H - - + - - -
28.21883 H2 S(0) + + + + + +
28.50197 HD R(3) - + + - - -
28.9138 p-H2O - + + - - +
28.94 OH 7/2-5/2 - + - - - -
29.8366 o-H2O - + - - - -
31.7715 o-H2O - + + + + +
34.6294 OH 5/2-3/2 - + + + + +
34.8140 Si II - + + + - -
35.4710 p-H2O - + - - - -
37.4749 o-H2O - + - - - -
37.70155 HD R(2) + + + - - -
37.51946 CH3OH R1 + + + - - -
38.93579 CH3OH P1 - + - - - -
40.6904 o-H2O - + + + + +
43.3393 o-H2O - + - - - -
LWS Fabry Perot:
112.07251 HD R(0) + + + + + +
119.4417 OH 5/2-3/2 + Cox Cox + +
84.4204 OH 7/2-5/2 + + + + +
65.2789 OH 9/2-7/2 + - - - -
163.1243 OH 3/2-1/2 + + + + +
98.7369 OH 5/2-3/2 + - + + +
71.2158 OH 7/2-5/2 + - - - -
79.1817 OH 1/2-3/2 + - + + +
96.3122 OH 3/2-5/2 + - - - -
53.3513 OH 3/2-3/2 + - - - -
48.8168 OH 5/2-5/2 + - - - -
120.1726 18OH 5/2-3/2 + - - - -
180.4880 o-H2O 2_21-2_12 + + + + +
179.5265 o-H2O 2_12-1_01 + Cox Cox + +
174.6264 o-H2O 3_03-2_12 + + + + +
136.4944 o-H2O 3_30-3_21 + + + - -
134.9346 o-H2O 5_14-5_05 + + - - -
113.5366 o-H2O 4_14-3_03 + + + - -
108.0730 o-H2O 2_21-1_10 + Cox Cox + +
99.4924 o-H2O 5_05-4_14 + - - - -
78.7414 o-H2O 4_23-3_12 + + - - -
82.0304 o-H2O 6_16-5_05 + - - - -
75.3804 o-H2O 3_21-2_12 + Cox Cox + +
66.4372 o_H2O 3_30-2_21 + + + - -
156.1930 p-H2O 3_22-3_13 + + + - -
138.5272 p-H2O 3_13-2_02 + Cox Cox - -
126.7126 p-H2O 3_31-3_22 + + - - -
100.9828 p-H2O 2_20-1_11 + Cox Cox + +
181.0512 o-H218O 2_12-1_01 + Cox Cox + +
109.3470 o-H218O 2_21-1_10 + + + - -
102.0044 p-H218O 2_20-1_11 + - - - -
63.1700 O I 1-2 + - - - -
145.5255 O I 0-1 + - - - -
157.7410 C II + - - - -
==============================================================================
SUMMARY EMISSION LINES
=========================
Sagittarius hole
=========================================================
Source Total time (hr) Priority
---------------------------------------------------------
IC 443 G 2.5 1
HH 7 2.3 2
IC 63 0.9 2
----------------------------------------------------------
Orion hole
=========================================================
Source Total time (hr) Priority
---------------------------------------------------------
DR21 FIR1 1.6 2
IC 63 0.9 2
W51 Main 1.4 3
-----------------------------------------------------------
EMISSION PART: Sagittarius hole
==================================
================================================================================
Lambda Line HH7 IC63 IC443
--------------------------------------------------------------------------------
Grating:
2.5510 H2 (2,1) Q(1) + + +
2.5698 H2 (2,1) Q(3) + - +
2.6040 H2 (2,1) Q(5) + - +
2.6269 H2 (1,0) O(2) + + +
2.8025 H2 (1,0) O(3) + + +
3.84675 H2 S(13) + - +
4.18128 H2 S(11) + - +
4.69461 H2 S(9) + - +
5.51116 H2 S(7) + - +
6.10856 H2 S(6) + - +
6.90952 H2 S(5) + - +
8.02505 H2 S(4) + - +
9.66491 H2 S(3) + - +
12.27861 H2 S(2) + + +
15.25104 HD R(7) - - +
16.89381 HD R(6) + - +
17.03483 H2 S(1) + + +
19.43100 HD R(5) + - +
23.03376 HD R(4) + - +
24.0424 Fe I + + +
25.2490 S I + + +
25.9882 Fe II + + +
28.21883 H2 S(0) + + +
28.50197 HD R(3) + - +
28.94 OH 7/2 -- 5/2 + - +
34.6294 OH 5/2 -- 3/2 + - +
34.8140 Si II + + +
37.70155 HD R(2) + - +
Fabry-Perot:
17.03483 H2 S(1) + - +
24.0424 Fe I - - -
25.2490 S I - - -
25.9402 o-H2O 5_41 - 4_14 - - +
25.9882 Fe II - - -
28.21883 H2 S(0) - - -
28.50197 HD R(3) - - -
28.9138 p-H2O 4_40 - 3_13 - - +
28.94 OH 7/2 -- 5/2 - - -
29.8366 o-H2O 7_25 - 6_16 - - +
31.7715 o-H2O 4_41 - 3_12 - - +
34.6294 OH 5/2 -- 3/2 - - -
34.8140 Si II - - -
35.4710 p-H2O 5_33 - 4_04 - - +
37.70155 HD R(2) - - -
37.4749 o-H2O 14_1,14 - 13_0,13 - - +
40.6904 o-H2O 4_32 - 3_03 - - +
43.3393 o-H2O 12_1,12 - 11_0,11 - - +
LWS 01 45-200 mu - + -
LWS Fabry Perot:
112.07251 HD R(0) + - +
119.4417 OH 5/2-3/2 + - +
84.4204 OH 7/2-5/2 + - +
65.2789 OH 9/2-7/2 + - +
163.1243 OH 3/2-1/2 + - +
98.7369 OH 5/2-3/2 + - +
71.2158 OH 7/2-5/2 + - +
79.1817 OH 1/2-3/2 + - +
96.3122 OH 3/2-5/2 + - +
53.3513 OH 3/2-3/2 + - +
48.8168 OH 5/2-5/2 + - +
120.1726 18OH 5/2-3/2 + - +
180.4880 o-H2O 2_21-2_12 - - +
179.5265 o-H2O 2_12-1_01 - - +
174.6264 o-H2O 3_03-2_12 - - +
136.4944 o-H2O 3_30-3_21 - - +
134.9346 o-H2O 5_14-5_05 - - +
113.5366 o-H2O 4_14-3_03 - - +
108.0730 o-H2O 2_21-1_10 - - +
99.4924 o-H2O 5_05-4_14 - - +
78.7414 o-H2O 4_23-3_12 - - +
82.0304 o-H2O 6_16-5_05 - - +
75.3804 o-H2O 3_21-2_12 - - +
66.4372 o_H2O 3_30-2_21 - - +
156.1930 p-H2O 3_22-3_13 - - +
138.5272 p-H2O 3_13-2_02 - - +
126.7126 p-H2O 3_31-3_22 - - +
100.9828 p-H2O 2_20-1_11 - - +
181.0512 o-H218O 2_12-1_01 - - +
109.3470 o-H218O 2_21-1_10 - - +
102.0044 p-H218O 2_20-1_11 - - +
63.1700 O I 1-2 + - +
145.5255 O I 0-1 + - +
157.7410 C II + - +
==============================================================================
EMISSION PART: Orion hole
==================================
================================================================================
Lambda Line DR21 IC63 W51
FIR1 Main
--------------------------------------------------------------------------------
Grating:
2.5510 H2 (2,1) Q(1) + + +
2.5698 H2 (2,1) Q(3) + - +
2.6040 H2 (2,1) Q(5) + - +
2.6269 H2 (1,0) O(2) + + +
2.8025 H2 (1,0) O(3) + + +
3.84675 H2 S(13) + - +
4.18128 H2 S(11) + - +
4.69461 H2 S(9) + - +
5.51116 H2 S(7) + - +
6.10856 H2 S(6) + - +
6.90952 H2 S(5) + - +
8.02505 H2 S(4) + - +
9.66491 H2 S(3) + - +
12.27861 H2 S(2) + + +
15.25104 HD R(7) - - -
16.89381 HD R(6) - - -
17.03483 H2 S(1) + + +
19.43100 HD R(5) - - +
23.03376 HD R(4) + - +
24.0424 Fe I + + -
25.2490 S I + + -
25.9882 Fe II + + -
28.21883 H2 S(0) + + +
28.50197 HD R(3) + - +
28.94 OH 7/2 -- 5/2 - - -
34.6294 OH 5/2 -- 3/2 - - -
34.8140 Si II + + -
37.70155 HD R(2) + - +
Fabry-Perot:
17.03483 H2 S(1) - - +
24.0424 Fe I - - +
25.2490 S I - - +
25.9402 o-H2O 5_41 - 4_14 + - +
25.9882 Fe II - - +
28.21883 H2 S(0) - - +
28.50197 HD R(3) - - +
28.9138 p-H2O 4_40 - 3_13 + - +
28.94 OH 7/2 -- 5/2 + - +
29.8366 o-H2O 7_25 - 6_16 + - +
31.7715 o-H2O 4_41 - 3_12 + - +
34.6294 OH 5/2 -- 3/2 + - +
34.8140 Si II - - +
35.4710 p-H2O 5_33 - 4_04 + - +
37.70155 HD R(2) - - +
37.4749 o-H2O 14_1,14 - 13_0,13 + - +
40.6904 o-H2O 4_32 - 3_03 + - +
43.3393 o-H2O 12_1,12 - 11_0,11 + - +
LWS 01 45-200mu + + -
LWS Fabry Perot:
112.07251 HD R(0) + - -
119.4417 OH 5/2-3/2 + - -
84.4204 OH 7/2-5/2 + - -
65.2789 OH 9/2-7/2 - - -
163.1243 OH 3/2-1/2 + - -
98.7369 OH 5/2-3/2 - - -
71.2158 OH 7/2-5/2 - - -
79.1817 OH 1/2-3/2 - - -
96.3122 OH 3/2-5/2 - - -
53.3513 OH 3/2-3/2 - - -
48.8168 OH 5/2-5/2 - - -
120.1726 18OH 5/2-3/2 - - -
180.4880 o-H2O 2_21-2_12 + - -
179.5265 o-H2O 2_12-1_01 + - -
174.6264 o-H2O 3_03-2_12 + - -
136.4944 o-H2O 3_30-3_21 + - -
134.9346 o-H2O 5_14-5_05 - - -
113.5366 o-H2O 4_14-3_03 - - -
108.0730 o-H2O 2_21-1_10 + - -
99.4924 o-H2O 5_05-4_14 - - -
78.7414 o-H2O 4_23-3_12 - - -
82.0304 o-H2O 6_16-5_05 - - -
75.3804 o-H2O 3_21-2_12 + - -
66.4372 o_H2O 3_30-2_21 - - -
156.1930 p-H2O 3_22-3_13 - - -
138.5272 p-H2O 3_13-2_02 - - -
126.7126 p-H2O 3_31-3_22 - - -
100.9828 p-H2O 2_20-1_11 + - -
181.0512 o-H218O 2_12-1_01 + - -
109.3470 o-H218O 2_21-1_10 - - -
102.0044 p-H218O 2_20-1_11 - - -
63.1700 O I 1-2 - - -
145.5255 O I 0-1 - - -
157.7410 C II - - -
==============================================================================
CIRCUMSTELLAR PART: both holes
==================================
IRC +10 216
==================================
Lambda Line/Band
----------------------------------
Fabry-Perot:
12.27861 H2 S(2)
13.70332 C2H2
13.73068 13CCH2
14.97500 CO2* Q-branch
15.41933 13CO2* Q-branch
15.92600 HCCCCH* Q-branch
15.91882 HCCCCH R(0)
15.84489 HCCCCH R(10)
16.00080 CH3 R(0,0)
16.49670 CH3* Q-branch
17.03483 H2 S(1)
28.21883 H2 S(0)
==================================
<=== autumn_launch_targets ===>
1, "SWS07", 1.,"N", "Sgr A-W IRS3 ", 17.70803, -28.98722, 1950,0.,0.,15281, 2
2, "SWS07", 1.,"N", "Sgr A-W IRS3 ", 17.70803, -28.98722, 1950,0.,0., 4165, 3
3, "LWS04", 1.,"N", "Sgr A-W IRS3 ", 17.70803, -28.98722, 1950,0.,0., 2420, 0
4, "SWS07", 1.,"N", "W3 IRS5 ", 2.36483, 61.87250, 1950,0.,0.,16021, 5
5, "LWS01", 1.,"N", "W3 IRS5 ", 2.36483, 61.87250, 1950,0.,0., 500, 6
6, "LWS04", 1.,"N", "W3 IRS5 ", 2.36483, 61.87250, 1950,0.,0., 3620, 0
7, "SWS07", 1.,"N", "GL 2591 NIRS01", 20.45994, 40.02056, 1950,0.,0.,19418, 8
8, "LWS04", 1.,"N", "GL 2591 NIRS01", 20.45994, 40.02056, 1950,0.,0., 1580, 0
9, "SWS07", 2.,"N", "S 140 IRS1 ", 22.29474, 63.06156, 1950,0.,0., 8791,10
10, "LWS04", 2.,"N", "S 140 IRS1 ", 22.29474, 63.06156, 1950,0.,0., 1580, 0
11, "SWS07", 2.,"N", "GL 2136 ", 18.32683, -13.52778, 1950,0.,0., 7049,12
12, "LWS04", 2.,"N", "GL 2136 ", 18.32683, -13.52778, 1950,0.,0., 1580, 0
13, "SWS07", 3.,"N", "NGC 7538 IRS9 ", 23.19800, 61.18306, 1950,0.,0., 4705,14
14, "LWS04", 3.,"N", "NGC 7538 IRS9 ", 23.19800, 61.18306, 1950,0.,0., 1580, 0
15, "SWS02", 2.,"N", "DR 21 FIR1 ", 20.62039, 42.23250, 1950,0.,0., 2512,16
16, "SWS07", 2.,"N", "DR 21 FIR1 ", 20.62039, 42.23250, 1950,0.,0., 1442,17
17, "LWS01", 2.,"N", "DR 21 FIR1 ", 20.62039, 42.23250, 1950,0.,0., 500,18
18, "LWS04", 2.,"N", "DR 21 FIR1 ", 20.62039, 42.23250, 1950,0.,0., 1401, 0
19, "SWS02", 2.,"N", "IC 63 ", 0.93278, 60.61861, 1950,0.,0., 2822,20
20, "LWS01", 2.,"N", "IC 63 ", 0.93278, 60.61861, 1950,0.,0., 500, 0
21, "SWS02", 3.,"N", "W51 Main ", 19.35728, 14.41194, 1950,0.,0., 1958,22
22, "SWS07", 3.,"N", "W51 Main ", 19.35728, 14.41194, 1950,0.,0., 3226, 0
23, "SWS07", 3.,"N", "IRC +10216 ", 9.75411, 13.51111, 1950,0.,0., 2649, 0
<=== spring_launch_targets ===>
1, "SWS07", 1.,"N", "Orion IRc2 ", 5.54633, -5.40694, 1950,0.,0.,14902, 0
2, "SWS07", 1.,"N", "W3 IRS5 ", 2.36483, 61.87250, 1950,0.,0.,16021, 3
3, "LWS01", 1.,"N", "W3 IRS5 ", 2.36483, 61.87250, 1950,0.,0., 500, 4
4, "LWS04", 1.,"N", "W3 IRS5 ", 2.36483, 61.87250, 1950,0.,0., 3620, 0
5, "SWS07", 2.,"N", "NGC 2024 IRS2 ", 5.65396, -1.93306, 1950,0.,0.,13824, 6
6, "LWS04", 2.,"N", "NGC 2024 IRS2 ", 5.65396, -1.93306, 1950,0.,0., 1820, 0
7, "SWS07", 1.,"N", "GL 989 ", 6.64025, 9.54139, 1950,0.,0., 7842, 8
8, "LWS04", 1.,"N", "GL 989 ", 6.64025, 9.54139, 1950,0.,0., 1580, 0
9, "SWS07", 2.,"N", "GL 961 W(+E) ", 6.53300, 4.25189, 1950,0.,0., 7339, 0
10, "SWS07", 3.,"N", "GL 890 ", 6.13928, -6.20750, 1950,0.,0., 5556,11
11, "LWS04", 3.,"N", "GL 890 ", 6.13928, -6.20750, 1950,0.,0., 1580, 0
12, "SWS07", 3.,"N", "GL 490 ", 3.39414, 58.60917, 1950,0.,0., 7716,13
13, "LWS04", 3.,"N", "GL 490 ", 3.39414, 58.60917, 1950,0.,0., 1580, 0
14, "SWS02", 2.,"N", "HH 7 ", 3.43417, 31.08611, 1950,0.,0., 4552,15
15, "SWS07", 2.,"N", "HH 7 ", 3.43417, 31.08611, 1950,0.,0., 2040,16
16, "LWS04", 2.,"N", "HH 7 ", 3.43417, 31.08611, 1950,0.,0., 1820, 0
17, "SWS02", 2.,"N", "IC 63 ", 0.93278, 60.61861, 1950,0.,0., 2822,18
18, "LWS01", 2.,"N", "IC 63 ", 0.93278, 60.61861, 1950,0.,0., 500, 0
19, "SWS02", 1.,"N", "IC 443 G ", 6.22806, 22.55278, 1950,0.,0., 3320,20
20, "SWS07", 1.,"N", "IC 443 G ", 6.22806, 22.55278, 1950,0.,0., 1766,21
21, "LWS01", 1.,"N", "IC 443 G ", 6.22806, 22.55278, 1950,0.,0., 500,22
22, "LWS04", 1.,"N", "IC 443 G ", 6.22806, 22.55278, 1950,0.,0., 3251, 0
23, "SWS07", 3.,"N", "IRC +10216 ", 9.75411, 13.51111, 1950,0.,0., 2649, 0