OBSERVER:
=========
OBSID: SDRAPATZ
PI: S. Drapatz
Address: Max-Planck-Institut fuer extraterrestrische Physik
Giessenbachstrasse 1
D-85740 Garching
Germany
Phone: 49 / 89 / 3299-3880
Fax: 49 / 89 / 3299-3569
E-Mail: timmer%mpeis1@mpe.mpe-garching.mpg.de
PROPOSAL:
=========
PROPIDs: MPEWARM1, MPEWARM2 (part 1 and 2)
Keywords: circumstellar envelopes, young stellar objects,
HII regions, supernova remnants, molecular clouds
Co-Is: T. de Graauw, B. Draine, R. Genzel, D. Hollenbach,
A. Moorwood, E. Oliva, J. Puget, A. Sternberg, R.
Timmermann, P. van der Werf, E. van Dishoeck
TITLE:
======
Physical and Chemical Conditions in Dense, Warm Interstellar Gas
SCIENTIFIC ABSTRACT:
====================
The warm (100 - 5000 K), dense (n(H_2) > 10^3 cm^-3) interstellar
medium is a decisive component of the whole interstellar medium
and is closely coupled to key processes like star formation and
evolution. It is heated through a wide variety of astrophysi-
cally important processes such as shocks of various types, X-ray
irradiation, UV irradiation of interface regions near HII regions,
and stellar radiation in the environment of young objects. A
rich variety of lines in the IR and submm wavelength region
will provide a unique opportunity to investigate the physics,
chemistry and interrelation of corresponding phenomena by multi-
line spectroscopy of various molecules, atoms and ions. However,
since allmost all lines cannot be observed from ground based
telescopes or even from an airborne observatory (KAO) ISO would
offer the first and only possibility for this investigation.
We have selected four classes of objects each representing
different processes that heat the gas:
(1.) photon-dominated regions at the interfaces of HII regions
(including reflection nebulae),
(2.) shocks of various types: strong shocks (J-type) in
supernova remnants and moderate or weak shocks (also C-type)
in outflow sources,
(3.) embedded sources (star formation) where dust is radiatively
heated by the central source and gas is heated by dust, and
(4.) regions of X-ray excitation.
For each class a small number of prototypical, bright sources
and a set of spectral lines in the ISO wavelength range has been
selected. The set of radiative transitions is selected thus that
a maximum of information can be gained for each individual class
of objects. Much emphasis is placed on the observation of (faint)
important lines rather than on mapping because of time
constraints by the faintness of some of the crucial lines. Using
these sources as a kind of templates we also establish a set of
crucial lines with which different processes can be distinguished.
The primary target lines for all four classes are the rotational
transitions of H_2 in order to study directly the bulk of the
warm gas. Through observation of rotational transitions in
oxygen-bearing species such as OH, H_2O, and H_2^{18}O, and O_2,
the oxygen chemistry in interstellar clouds will be studied for
the first time via direct determination of all important
reactants rather than by default. Most of these molecules serve
also as a major coolant and therefore their abundances have a
great impact on the energy balance of the warm molecular gas.
This balance is also determined by the cooling of fine-structure
lines where their contribution will be studied through a set of
diagnostically useful transitions.
We also propose the observation of a few selected rovibrational
transitions in molecular ions that become quite abundant in
objects where the gas is excited through X-ray irradiation.
This unique possibility will enable us to get a handle on that
process. In a few objects where the gas is cold (T < 30 K)
absorption measurements will be performed. The study of the
lowest rotational transitions of H_2 and HD will provide a first
and accurate determination of their total column density in this
general environment. These observations are closely related to
the emission measurements mentioned above. Furthermore, a series
of transitions in the first fundamental band of H_2O, H_2^{18}O,
CH_4, and CO_2 will be observed. Since a detailed scientific
proposal would by far exceed the granted space we include a
list of lines for each class of objects in the scientific
justification.
OBSERVATION SUMMARY:
====================
We plan to take advantage of the spectroscopic capabilities of
ISO over its full wavelength range, using the following AOTs:
SWS: Medium and high resolution spectroscopy with the AOTs
SWS01, SWS02, SWS06, SWS07
LWS: Medium resolution full grating scans and high resolution
line scans with AOTs LWS01, LWS04
A detailed description of our observing strategy and outline of
integration times exceeds the limits of this abstract.
Time distribution for autumn launch targets:
--------------------------------------------------
Team Total top 40% second 30% last 30%
SWS 269087 105379 84224 79484
AFM 10800 10800 0 0
JLP 18764 7488 7488 3744
TDG 0 0 0 0
--------------------------------------------------
total 298607 123667 91712 83228
Time distribution for spring launch targets:
--------------------------------------------------
Team Total top 40% second 30% last 30%
SWS 275579 110054 84874 80651
AFM 10800 10800 0 0
JLP 18764 7488 7488 3744
TDG 7200 7200 0 0
--------------------------------------------------
total 312299 135542 92362 84395
The following two tables contain the targets in their specific
templates that will be observed for the Orion hole and the
Galactic center visibility holes, respectively. The numbers
specify the total observation time in hours.
autumn launch targets:
----------------------
Object Priority
------------------------------------------------------------------
1 2 3
------------------------------------------------------------------
PDR: M17 7.53 2.00 1.00
S140 4.04
S106 4.04
------------------------------------------------------------------
Refl. Nebulae: NGC 7023 2.35 2.11
R Cr A 3.17
IC 1396 3.17
------------------------------------------------------------------
Shocks: DR 21 9.20
RCW 103 3.94
Cep A 8.89
W 28 A2 6.60
M 8E IRS1 2.29
------------------------------------------------------------------
Emb. Sources: W3 (OH) 2.90
W51 IRS 2 1.90
NGC 7538 IRS1 2.90
------------------------------------------------------------------
X-Ray heat. Sources: RCW 103 2.08
SN 1987A 2.20
SS 433 2.20
------------------------------------------------------------------
Absorp. Spectr.: Sgr A West 2.86 2.86
W51 IRS2 2.30
Sgr B2 1.40 1.00
------------------------------------------------------------------
spring launch targets:
----------------------
Object Priority
------------------------- ----------------------------------------
1 2 3
------------------------------------------------------------------
PDR: Orion 8.04
DR 21 2.65
S106 4.04
------------------------------------------------------------------
Refl. Nebulae: NGC 1977 4.28
NGC 2023 3.60
Parsamyan 18 2.11
------------------------------------------------------------------
Shocks: Orion BN/KL 8.72 2.03
IC 443 5.54
DR 21 7.57
Cep A 7.29
------------------------------------------------------------------
Emb. Sources: W3 (OH) 1.90
NGC 2170 IRS2 2.90
T Tau 2.90
NGC 7538 IRS1 1.90
------------------------------------------------------------------
X-Ray heat. Sources: IC 443 2.20
SN 1987A 2.20
Crab Nebula 2.08
SS 433 2.20
------------------------------------------------------------------
Absorp. Spectr.: Orion IRc2 2.30
NGC 2170 IRS2 2.30
W51 IRS2 2.86
------------------------------------------------------------------
The following tables specify the lines that will be observed for
different templates. The integration times have been calculated
such that at least a S/N ratio of 20 is achieved for each
individual line. For fainter lines such as the H2 v=0->0 S(0)
transition where the integration times would become much too
long the integration time has been limited to 1200 sec (in
special cases 3600 sec).
Table 1: Lines to be observed for PDRs near bright
HII regions.
____________________________________________________
Line lambda AOT
[mu]
----------------------------------------------------
H_2 28.2188 SWS07
H_2 9.6649 SWS02
H_2 8.0251 SWS02
H_2 17.0348 SWS07
H_2 4.6933 SWS02
H_2 12.2786 SWS02
[SiII] 34.8160 SWS07
H_2 6.9095 SWS02
H_2 3.8451 SWS02
[FeIII] 22.93 SWS02
H_2 5.5097 SWS02
H_2 4.1801 SWS02
[NeIII] 15.55 SWS02
H_2 2.6262 SWS02
H_2 2.8017 SWS02
H_2 2.5503 SWS02
H_2 2.72 SWS02
HI n=13->9 14.1831 SWS02
OH 34.6035 SWS07
H_2O 40.6909 SWS07
H_2O 28.9137 SWS07
[FeII] 25.9882 SWS07
HI n=6->5 7.4599 SWS02
HD 112.1076 LWS04
[NII] 121.8981 LWS04
[CII] 157.740 LWS04
H_2O 113.54 LWS04
H_2O 125.35 LWS04
H_2O 179.53 LWS04
H_2^18O 181.05 LWS04
LWS scan (selected sources) 45-180 LWS01
---------------------------------------------------
Table 2: Lines to be observed for reflection nebulae.
____________________________________________________
Line lambda AOT
[mu]
----------------------------------------------------
H_2 28.2188 SWS02
H_2 9.6649 SWS02
H_2 8.0251 SWS02
H_2 17.0348 SWS02
H_2 6.9095 SWS02
H_2 12.2786 SWS02
[SiII] 34.8160 SWS02
OH 34.6035 SWS07
H_2O 40.6909 SWS07
H_2O 28.9137 SWS07
HI n=6->5 7.4599 SWS02
H_2 2.6262 SWS02
H_2 2.8017 SWS02
H_2 2.5503 SWS02
H_2 2.72 SWS02
HI n=13->9 14.1831 SWS02
HD 112.1076 LWS04
[NII] 121.8981 LWS04
[CII] 157.740 LWS04
H_2O 113.54 LWS04
H_2O 125.35 LWS04
H_2O 179.53 LWS04
H_2^18O 181.05 LWS04
LWS scan (selected sources) 45-180 LWS01
---------------------------------------------------
Table 3: Individual lines to be observed for shocked
molecular gas.
____________________________________________________
Line lambda AOT
[mu]
----------------------------------------------------
H_2 28.2188 SWS07
HD 10.8719 SWS02
H_2 17.0348 SWS07
H_2 4.1809 SWS02
H_2 3.8451 SWS02
H_2 12.2786 SWS02
[SiII] 34.8160 SWS02
H_2 9.6649 SWS02
H_2O 35.4259 SWS07
H_2 8.0251 SWS02
H_2O 29.8366 SWS07
H_2 6.9095 SWS02
[SI] 25.2490 SWS02
H_2 5.5111 SWS02
HD 19.4326 SWS02
H_2 4.6924 SWS02
[FeII] 25.9882 SWS02
HD 28.5063 SWS07
HD 12.4812 SWS02
HD 37.7074 SWS07
HD 11.5915 SWS02
HD 23.0309 SWS02
H_2 3.23 SWS02
HD 16.8947 SWS02
[NiII] 6.634 SWS02
HD 15.0218 SWS02
H_2 2.6262 SWS02
H_2 2.8017 SWS02
H_2 3.00 SWS02
HD 13.5980 SWS02
H_2 2.553 SWS02
OH 34.6035 SWS07
OH 28.940 SWS07
HI n=6->5 7.4599 SWS02
H_2O 40.3367 SWS07
H_2O 31.7720 SWS07
OH 43.949 SWS02
HI n=7->6 12.3719 SWS02
H_2O 45.1114 SWS02
H_2O 43.3393 SWS02
H_2O 40.6909 SWS07
OH 44.666 SWS02
OH 39.514 SWS07
HI n=8->6 7.5025 SWS02
[NeII] 12.8149 SWS02
[NiI] 7.505 SWS02
OH 24.642 SWS07
H_3^+ 3.9530 SWS02
[SiVIII] 18.45 SWS02
HeH^+ 3.61 SWS02
[FeI] 24.04 SWS07
^12CO 4.6 SWS06
O_2 165.4113 LWS04
LWS scan (selected sources) 45-180 LWS01
H_2O 43.3407 SWS02
H_2O 71.5396 LWS04
H_2O 71.9467 LWS04
H_2O 74.9445 LWS04
H_2O 99.4926 SWS07
H_2O 96.1710 SWS07
H_2O 49.2817 LWS04
H_2O 28.9137 SWS07
H_2O 121.721 LWS04
H_2^18O 41.1599 SWS07
H_2O (not Orion) 125.524 LWS04
H_2O (not Orion) 113.538 LWS04
H_2O 179.527 LWS04
H_2^18O 181.049 LWS04
H_2O (not Orion) 82.031 LWS04
[SiI] 129.68 LWS04
[SiI] 68.474 LWS04
CH 149.091 LWS04
CH 149.390 LWS04
NH_3 124.91 LWS04
NH_3 124.88 LWS04
NH_3 124.80 LWS04
NH_3 124.65 LWS04
OH 163.121 LWS04
OH 163.396 LWS04
OH 119.441 LWS04
OH 119.234 LWS04
^18OH 120.172 LWS04
^18OH 119.966 LWS04
----------------------------------------------------
Table 4: Lines to be observed for shocked gas in the
ionized parts of SNRs.
____________________________________________________
Line lambda AOT
[mu]
----------------------------------------------------
[FeII] 5.339 SWS02
[FeII] 17.9533 SWS02
[ArIII] 8.9910 SWS02
[FeII] 35.3491 SWS02
[PII] 32.87 SWS02
[NeIII] 36.02 SWS02
[FeIII] 33.04 SWS02
[NeVI] 7.642 SWS02
[FeI] 24.04 SWS02
[MgV] 5.609 SWS02
[SIII] 33.482 SWS02
[SIV] 10.5105 SWS02
[NeIII] 15.55 SWS02
[ArII] 6.9853 SWS02
[FII] 29.33 SWS02
[NiI] 7.505 SWS02
[NiIII] 7.347 SWS02
[NeII] 12.8149 SWS02
[SiII] 34.8160 SWS02
[OIV] 25.87 SWS02
[MgIV] 4.487 SWS02
[NiII] 6.634 SWS02
[SI] 25.2490 SWS02
[ClII] 33.281 SWS02
[ClI] 11.3333 SWS02
[SiIX] 2.584 SWS02
[ClII] 14.3678 SWS02
[NeV] 14.32 SWS02
HI Br alpha 4.0423 SWS02
[SIII] 18.7129 SWS02
[FI] 24.745 SWS02
[FeII] 25.9882 SWS02
[FeIII] 22.93 SWS02
[ArIII] 21.84 SWS02
[NeV] 24.28 SWS02
[SiIX] 3.92 SWS02
[NII] 121.8981 LWS04
[CII] 157.740 LWS04
[OIII] 88.356 LWS04
[OIII] 51.815 LWS04
[SiI] 129.68 LWS04
[SiI] 68.474 LWS04
[NIII] 57.317 LWS04
-----------------------------------------------------
Table 5: Lines to be observed for gas heated by embedded
objects.
____________________________________________________
Line lambda AOT
[mu]
----------------------------------------------------
H_2 28.2188 SWS07
H_2 1) 17.0302 SWS02
H_2 6.9095 SWS02
H_2 3.23 SWS02
H_2 1) 12.2786 SWS02
H_2O 40.6909 SWS07
H_2 9.6649 SWS02
OH 2) 34.6035 SWS07
HI Pf alpha 2) 7.46 SWS02
H_2O 29.8366 SWS07
H_2O 2) 31.7720 SWS07
H_2O 45.1114 SWS02
HD 112.1076 LWS04
HD 56.2114 LWS04
H_2^18O 41.1599 SWS07
H_2O 49.2817 LWS04
H_2O 2) 28.9137 SWS07
H_2O 99.4926 SWS07
H_2O 96.1710 SWS07
H_2O 121.721 LWS04
H_2^18O 41.1599 SWS07
H_2O (not Orion) 125.524 LWS04
H_2O (not Orion) 113.538 LWS04
H_2O 179.527 LWS04
H_2^18O 181.049 LWS04
H_2O (not Orion) 82.031 LWS04
CH 149.091 LWS04
CH 149.390 LWS04
NH_3 124.91 LWS04
NH_3 124.88 LWS04
NH_3 124.80 LWS04
NH_3 124.65 LWS04
OH 2) 163.121 LWS04
OH 2) 163.396 LWS04
OH 119.441 LWS04
OH 119.234 LWS04
^18OH 120.172 LWS04
^18OH 119.966 LWS04
O_2 165.4113 LWS04
LWS scan (selected sources) 45-180 LWS01
-----------------------------------------------------
1) SWS07 for T Tau
2) not for T Tau
Table 6: Lines to be observed for X-ray excited gas.
____________________________________________________
Line lambda AOT
[mu]
----------------------------------------------------
H_2 9.6649 SWS02
[SiII] 34.8160 SWS02
H_2O 40.3367 SWS02
H_2O 39.3991 SWS02
[OIV] 25.87 SWS02
HI Br alpha 4.051 SWS02
H_2 4.6946 SWS02
[SiVIII] 18.45 SWS02
HeH^+ 3.61 SWS02
H_3^+ 16.331 SWS02
H_3^+ 3.953 SWS02
[NII] 121.898 LWS04
[CII] 157.740 LWS04
----------------------------------------------------
Table 7: Lines observed for absorption spectroscopy.
____________________________________________________
Line lambda AOT
[mu]
----------------------------------------------------
H_2 28.2188 SWS07
H_2 17.0348 SWS07
HD 112.1076 LWS04
O_2 165.4113 LWS04
H_2O 100.983 LWS04
H_2O 179.527 LWS04
H_2^18O 181.049 LWS04
____________________________________________________
CH_4 nu_4 band (not Orion) 7.40-7.65 SWS06
CH_4 nu_3 band (not Orion) 3.2-3.4 SWS06
----------------------------------------------------
AUTUMN LAUNCH TARGETS OF PROPOSAL SDRAPATZ.MPEWARM1:
====================================================
1, "SWS02", 1.,"N", "M17 pos1 ", 18.29214, -16.21778, 1950, 0.,0., 2388,2
2, "SWS07", 1.,"N", "M17 pos1 ", 18.29214, -16.21778, 1950, 0.,0., 2020,0
3, "LWS01", 1.,"N", "M17 pos2 ", 18.29156, -16.21361, 1950, 0.,0., 496,4
4, "LWS04", 1.,"N", "M17 pos2 ", 18.29156, -16.21361, 1950, 0.,0., 1830,0
5, "SWS02", 1.,"N", "M17 pos2 ", 18.29156, -16.21361, 1950, 0.,0., 2388,6
6, "SWS07", 1.,"N", "M17 pos2 ", 18.29156, -16.21361, 1950, 0.,0., 2020,0
7, "SWS02", 1.,"N", "M17 pos3 ", 18.29100, -16.22333, 1950, 0.,0., 2388,8
8, "SWS07", 1.,"N", "M17 pos3 ", 18.29100, -16.22333, 1950, 0.,0., 2020,0
9, "SWS02", 1.,"N", "M17 pos4 ", 18.29003, -16.23722, 1950, 0.,0., 2388,10
10, "SWS07", 1.,"N", "M17 pos4 ", 18.29003, -16.23722, 1950, 0.,0., 2020,0
11, "SWS01", 3.,"N", "M17 IRAM pos1 ", 18.29330, -16.22056, 1950, 0.,0., 1872,0
12, "SWS01", 1.,"N", "M17 IRAM pos2 ", 18.29292, -16.22333, 1950, 0.,0., 1872,0
13, "SWS01", 2.,"N", "M17 IRAM pos3 ", 18.29253, -16.22611, 1950, 0.,0., 1872,0
14, "SWS01", 1.,"N", "M17 IRAM pos4 ", 18.29214, -16.22889, 1950, 0.,0., 1872,0
15, "SWS01", 2.,"N", "M17 IRAM pos5 ", 18.29176, -16.23167, 1950, 0.,0., 1872,0
16, "SWS01", 1.,"N", "M17 IRAM pos6 ", 18.29138, -16.23444, 1950, 0.,0., 1872,0
17, "SWS01", 2.,"N", "M17 IRAM pos7 ", 18.29099, -16.23722, 1950, 0.,0., 1872,0
18, "SWS01", 1.,"N", "M17 IRAM pos8 ", 18.29060, -16.24000, 1950, 0.,0., 1872,0
19, "SWS01", 2.,"N", "M17 IRAM pos9 ", 18.29022, -16.24278, 1950, 0.,0., 1872,0
20, "SWS01", 3.,"N", "M17 IRAM pos10", 18.28983, -16.24556, 1950, 0.,0., 1872,0
21, "SWS02", 2.,"N", "S140 PDR ", 22.29306, +63.05028, 1950, 0.,0., 4308,0
22, "SWS07", 2.,"N", "S140 PDR ", 22.29306, +63.05028, 1950, 0.,0., 2028,25
23, "SWS02", 2.,"N", "S140 IRS1 ", 22.29475, +63.06167, 1950, 0.,0., 4308,0
24, "SWS07", 2.,"N", "S140 IRS1 ", 22.29475, +63.06167, 1950, 0.,0., 2028,0
25, "LWS04", 2.,"N", "S140 PDR ", 22.29306, +63.05028, 1950, 0.,0., 1830,0
26, "SWS02", 3.,"N", "S106 H2 ", 20.42642, +37.21167, 1950, 0.,0., 4308,27
27, "SWS07", 3.,"N", "S106 H2 ", 20.42642, +37.21167, 1950, 0.,0., 1830,0
28, "SWS02", 3.,"N", "S106 PDR ", 20.42578, +37.21278, 1950, 0.,0., 4308,29
29, "SWS07", 3.,"N", "S106 PDR ", 20.42578, +37.21278, 1950, 0.,0., 1830,0
31, "LWS04", 3.,"N", "S106 H2 ", 20.42642, +37.21167, 1950, 0.,0., 2326,0
32, "SWS02", 1.,"N", "NGC7023 pos1 ", 21.01561, +67.97361, 1950, 0.,0., 4500,0
33, "SWS07", 1.,"N", "NGC7023 pos1 ", 21.01561, +67.97361, 1950, 0.,0., 566,35
35, "LWS04", 1.,"N", "NGC7023 pos1 ", 21.01561, +67.97361, 1950, 0.,0., 1076,0
36, "SWS02", 1.,"N", "NGC7023 pos2 ", 21.01611, +67.96833, 1950, 0.,0., 2250,37
37, "SWS07", 1.,"N", "NGC7023 pos2 ", 21.01611, +67.96833, 1950, 0.,0., 566,0
38, "SWS02", 2.,"N", "NGC7023 pos2 ", 21.01611, +67.96833, 1950, 0.,0., 2250,0
39, "SWS02", 2.,"N", "NGC7023 pos3 ", 21.01441, +67.99583, 1950, 0.,0., 4500,40
40, "SWS07", 2.,"N", "NGC7023 pos3 ", 21.01441, +67.99583, 1950, 0.,0., 566,0
41, "SWS02", 3.,"N", "RCrA pos1 ", 18.97597, -37.02806, 1950, 0.,0., 4300,0
42, "SWS07", 3.,"N", "RCrA pos1 ", 18.97597, -37.02806, 1950, 0.,0., 1400,0
43, "SWS02", 3.,"N", "RCrA pos2 ", 18.89444, -37.28806, 1950, 0.,0., 4300,0
44, "SWS07", 3.,"N", "RCrA pos2 ", 18.89444, -37.28806, 1950, 0.,0., 1400,0
45, "SWS02", 3.,"N", "IC1396A pos1 ", 21.59208, +57.28861, 1950, 0.,0., 4300,0
46, "SWS07", 3.,"N", "IC1396A pos1 ", 21.59208, +57.28861, 1950, 0.,0., 1400,0
47, "SWS02", 3.,"N", "IC1396A pos2 ", 21.58972, +57.29417, 1950, 0.,0., 4300,0
48, "SWS07", 3.,"N", "IC1396A pos2 ", 21.58972, +57.29417, 1950, 0.,0., 1400,0
49, "SWS02", 1.,"N", "DR21 west ", 20.61897, +42.14444, 1950, 0.,0., 3650,51
50, "SWS07", 1.,"N", "DR21 west ", 20.61897, +42.14444, 1950, 0.,0., 9400,0
51, "SWS07", 1.,"N", "DR21 west ", 20.61897, +42.14444, 1950, 0.,0., 650,53
53, "LWS04", 1.,"N", "DR21 west ", 20.61897, +42.14444, 1950, 0.,0., 5806,0
54, "SWS02", 1.,"N", "DR21 east ", 20.62278, +42.15278, 1950, 0.,0., 3650,56
55, "SWS07", 1.,"N", "DR21 east ", 20.62278, +42.15278, 1950, 0.,0., 9400,0
56, "SWS07", 1.,"N", "DR21 east ", 20.62278, +42.15278, 1950, 0.,0., 650,0
57, "SWS02", 1.,"N", "RCW103 H2 ", 16.23056, -50.98694, 1950, 0.,0., 9684,0
58, "SWS06", 1.,"N", "RCW103 H2 ", 16.23056, -50.98694, 1950, 0.,0., 739,0
59, "SWS02", 1.,"N", "RCW103 ion ", 16.22936, -50.97889, 1950, 0.,0., 3732,0
60, "SWS02", 2.,"N", "CepA Pk2 ", 22.90181, +61.76528, 1950, 0.,0., 7000,0
61, "SWS07", 2.,"N", "CepA Pk2 ", 22.90181, +61.76528, 1950, 0.,0., 5401,62
62, "SWS07", 2.,"N", "CepA Pk2 ", 22.90181, +61.76528, 1950, 0.,0., 739,0
63, "SWS02", 2.,"N", "CepA Pk4 ", 22.90603, +61.76667, 1950, 0.,0., 7000,0
64, "SWS07", 2.,"N", "CepA Pk4 ", 22.90603, +61.76667, 1950, 0.,0., 5401,65
65, "SWS07", 2.,"N", "CepA Pk4 ", 22.90603, +61.76667, 1950, 0.,0., 739,0
66, "LWS01", 2.,"N", "CepA Pk2 ", 22.90181, +61.76528, 1950, 0.,0., 496,67
67, "LWS04", 2.,"N", "CepA Pk2 ", 22.90181, +61.76528, 1950, 0.,0., 5310,0
68, "SWS02", 3.,"N", "W28 A2 ", 17.95750, -24.06611, 1950, 0.,0., 9492,0
69, "SWS02", 3.,"N", "W28 A2 ", 17.95750, -24.06611, 1950, 0.,0., 7769,0
70, "SWS07", 3.,"N", "W28 A2 ", 17.95750, -24.06611, 1950, 0.,0., 739,71
71, "LWS04", 3.,"N", "W28 A2 ", 17.95750, -24.06611, 1950, 0.,0., 5310,0
72, "SWS02", 3.,"N", "M8 E IRS1 ", 18.03025, -24.44806, 1950, 0.,0., 4000,0
73, "SWS07", 3.,"N", "M8 E IRS1 ", 18.03025, -24.44806, 1950, 0.,0., 3505,74
74, "SWS07", 3.,"N", "M8 E IRS1 ", 18.03025, -24.44806, 1950, 0.,0., 739,0
SPRING LAUNCH TARGETS OF PROPOSAL SDRAPATZ.MPEWARM1:
====================================================
1, "SWS02", 1.,"N", "theta1 Ori ", 05.54694, -05.42111, 1950, 0.,0., 2388,0
2, "SWS07", 1.,"N", "theta1 Ori ", 05.54694, -05.42111, 1950, 0.,0., 2508,0
3, "SWS02", 1.,"N", "Orion Bar Brga", 05.54775, -05.44806, 1950, 0.,0., 2388,0
4, "SWS07", 1.,"N", "Orion Bar Brga", 05.54775, -05.44806, 1950, 0.,0., 2508,0
5, "SWS02", 1.,"N", "Orion Bar H2S1", 05.54803, -05.45361, 1950, 0.,0., 2388,0
6, "SWS07", 1.,"N", "Orion Bar H2S1", 05.54803, -05.45361, 1950, 0.,0., 2508,0
8, "LWS04", 1.,"N", "Orion Bar H2S1", 05.54803, -05.45361, 1950, 0.,0., 2326,0
9, "SWS01", 3.,"N", "Orion Bar d1 ", 05.54847, -05.46194, 1950, 0.,0., 1872,0
10, "SWS01", 1.,"N", "Orion Bar d2 ", 05.54833, -05.45917, 1950, 0.,0., 1872,0
11, "SWS01", 2.,"N", "Orion Bar d3 ", 05.54819, -05.45639, 1950, 0.,0., 1872,0
12, "SWS01", 1.,"N", "Orion Bar H2S1", 05.54803, -05.45361, 1950, 0.,0., 1872,0
13, "SWS01", 2.,"N", "Orion Bar d5 ", 05.54789, -05.45083, 1950, 0.,0., 1872,0
14, "SWS01", 1.,"N", "Orion Bar Brga", 05.54775, -05.44806, 1950, 0.,0., 1872,0
15, "SWS01", 2.,"N", "Orion Bar d7 ", 05.54758, -05.44528, 1950, 0.,0., 1872,0
16, "SWS01", 1.,"N", "Orion Bar d8 ", 05.54744, -05.44250, 1950, 0.,0., 1872,0
17, "SWS01", 2.,"N", "Orion Bar d9 ", 05.54731, -05.43972, 1950, 0.,0., 1872,0
18, "SWS01", 3.,"N", "Orion Bar d10 ", 05.54714, -05.43694, 1950, 0.,0., 1872,0
19, "SWS02", 3.,"N", "DR 21 PDR ", 20.62236, +42.15139, 1950, 0.,0., 3444,0
20, "SWS07", 3.,"N", "DR 21 PDR ", 20.62236, +42.15139, 1950, 0.,0., 6099,0
21, "SWS02", 2.,"N", "S140 PDR ", 22.29306, +63.05028, 1950, 0.,0., 4308,0
22, "SWS07", 2.,"N", "S140 PDR ", 22.29306, +63.05028, 1950, 0.,0., 2028,0
23, "SWS02", 2.,"N", "S140 IRS1 ", 22.29475, +63.06167, 1950, 0.,0., 4308,0
24, "SWS07", 2.,"N", "S140 IRS1 ", 22.29475, +63.06167, 1950, 0.,0., 2028,0
25, "LWS04", 2.,"N", "S140 PDR ", 22.29306, +63.05028, 1950, 0.,0., 1830,0
26, "SWS02", 1.,"N", "NGC 1977 FIR ", 05.54556, -04.95000, 1950, 0.,0., 2004,32
27, "SWS07", 1.,"N", "NGC 1977 FIR ", 05.54556, -04.95000, 1950, 0.,0., 2796,0
28, "SWS02", 1.,"N", "NGC 1977 6cm ", 05.54667, -04.91667, 1950, 0.,0., 2004,0
29, "SWS07", 1.,"N", "NGC 1977 6cm ", 05.54667, -04.91667, 1950, 0.,0., 2796,0
30, "SWS02", 1.,"N", "NGC 1977 HCO+ ", 05.54333, -04.96667, 1950, 0.,0., 2004,0
31, "SWS07", 1.,"N", "NGC 1977 HCO+ ", 05.54333, -04.96667, 1950, 0.,0., 2796,0
32, "LWS01", 1.,"N", "NGC 1977 FIR ", 05.54556, -04.95000, 1950, 0.,0., 496,33
33, "LWS04", 1.,"N", "NGC 1977 FIR ", 05.54556, -04.95000, 1950, 0.,0., 580,0
34, "SWS02", 2.,"N", "NGC 2023 star ", 05.65167, -02.28278, 1950, 0.,0., 2004,35
35, "SWS07", 2.,"N", "NGC 2023 star ", 05.65167, -02.27278, 1950, 0.,0., 1980,0
36, "SWS02", 2.,"N", "NGC 2023 H2 ", 05.65242, -02.30028, 1950, 0.,0., 2004,37
37, "SWS07", 2.,"N", "NGC 2023 H2 ", 05.65242, -02.30028, 1950, 0.,0., 1980,0
38, "SWS02", 2.,"N", "NGC 2023 CO ", 05.65306, -02.29917, 1950, 0.,0., 2004,39
39, "SWS07", 2.,"N", "NGC 2023 CO ", 05.65306, -02.29917, 1950, 0.,0., 1980,40
40, "LWS01", 2.,"N", "NGC 2023 CO ", 05.65306, -02.29917, 1950, 0.,0., 496,41
41, "LWS04", 2.,"N", "NGC 2023 CO ", 05.65306, -02.29917, 1950, 0.,0., 580,0
42, "SWS02", 3.,"N", "Parsamyan 18 ", 06.95439, -07.70111, 1950, 0.,0., 4500,0
43, "SWS07", 3.,"N", "Parsamyan 18 ", 06.95439, -07.70111, 1950, 0.,0., 3098,0
44, "SWS02", 1.,"N", "Orion Pk1 ", 05.54617, -05.40056, 1950, 0.,0., 2580,46
45, "SWS07", 1.,"N", "Orion Pk1 ", 05.54617, -05.40056, 1950, 0.,0., 7143,0
46, "SWS07", 1.,"N", "Orion Pk1 ", 05.54617, -05.40056, 1950, 0.,0., 739,0
47, "SWS02", 1.,"N", "Orion IRc2 ", 05.54633, -05.40694, 1950, 0.,0., 2580,49
48, "SWS07", 1.,"N", "Orion IRc2 ", 05.54633, -05.40694, 1950, 0.,0., 7143,0
49, "SWS06", 1.,"N", "Orion IRc2 ", 05.54633, -05.40694, 1950, 0.,0., 739,53
50, "SWS02", 1.,"N", "Orion Pk2 ", 05.54675, -05.40944, 1950, 0.,0., 2580,52
51, "SWS07", 1.,"N", "Orion Pk2 ", 05.54675, -05.40944, 1950, 0.,0., 7143,0
52, "SWS07", 1.,"N", "Orion Pk2 ", 05.54675, -05.40944, 1950, 0.,0., 739,0
53, "LWS04", 1.,"N", "Orion IRc2 ", 05.54633, -05.40694, 1950, 0.,0., 420,0
54, "SWS02", 1.,"N", "IC443 H2 pos1 ", 06.22889, +22.44806, 1950, 0.,0., 9684,0
55, "SWS06", 1.,"N", "IC443 H2 pos1 ", 06.22889, +22.44806, 1950, 0.,0., 739,0
56, "SWS02", 1.,"N", "IC443 H2 pos2 ", 06.24489, +22.38444, 1950, 0.,0., 9684,0
57, "SWS06", 1.,"N", "IC443 H2 pos2 ", 06.24489, +22.38444, 1950, 0.,0., 739,0
58, "LWS04", 1.,"N", "IC443 H2 pos2 ", 06.24489, +22.38444, 1950, 0.,0., 5310,0
59, "LWS01", 1.,"N", "IC443 H2 pos2 ", 06.24489, +22.38444, 1950, 0.,0., 496,0
60, "SWS02", 1.,"N", "IC443 ion ", 06.24236, +22.90150, 1950, 0.,0., 3732,61
61, "LWS01", 1.,"N", "IC443 ion ", 06.24236, +22.90150, 1950, 0.,0., 496,0
62, "SWS02", 2.,"N", "DR21 west ", 20.61897, +42.14444, 1950, 0.,0., 3650,64
63, "SWS07", 2.,"N", "DR21 west ", 20.61897, +42.14444, 1950, 0.,0., 9400,0
64, "SWS07", 2.,"N", "DR21 west ", 20.61897, +42.14444, 1950, 0.,0., 650,0
65, "SWS02", 2.,"N", "DR21 east ", 20.62278, +42.15278, 1950, 0.,0., 3650,67
66, "SWS07", 2.,"N", "DR21 east ", 20.62278, +42.15278, 1950, 0.,0., 9400,0
67, "SWS07", 2.,"N", "DR21 east ", 20.62278, +42.15278, 1950, 0.,0., 650,0
68, "SWS02", 3.,"N", "CepA Pk2 ", 22.90181, +61.76528, 1950, 0.,0., 7000,0
69, "SWS07", 3.,"N", "CepA Pk2 ", 22.90181, +61.76528, 1950, 0.,0., 5401,70
70, "SWS07", 3.,"N", "CepA Pk2 ", 22.90181, +61.76528, 1950, 0.,0., 739,0
71, "SWS02", 3.,"N", "CepA Pk4 ", 22.90603, +61.76667, 1950, 0.,0., 7000,0
72, "SWS07", 3.,"N", "CepA Pk4 ", 22.90603, +61.76667, 1950, 0.,0., 5401,73
73, "SWS07", 3.,"N", "CepA Pk4 ", 22.90603, +61.76667, 1950, 0.,0., 739,0
AUTUMN LAUNCH TARGETS OF PROPOSAL SDRAPATZ.MPEWARM2:
====================================================
1, "SWS02", 1.,"N", "W3(OH) ", 02.38806, +61.65000, 1950, 0.,0., 1236,3
2, "SWS07", 1.,"N", "W3(OH) ", 02.38806, +61.65000, 1950, 0.,0., 5606,0
3, "LWS04", 1.,"N", "W3(OH) ", 02.38806, +61.64500, 1950, 0.,0., 3190,0
4, "SWS07", 1.,"N", "W51 IRS2 ", 19.35622, +14.42028, 1950, 0.,0., 6842,0
5, "SWS02", 3.,"N", "NGC 7538 IRS1 ", 23.19358, +61.19806, 1950, 0.,0., 1236,0
6, "SWS07", 3.,"N", "NGC 7538 IRS1 ", 23.19358, +61.19806, 1950, 0.,0., 5606,0
8, "LWS04", 3.,"N", "NGC 7538 IRS1 ", 23.19358, +61.19806, 1950, 0.,0., 3686,0
9, "SWS02", 1.,"N", "RCW103 H2 ", 16.23056, -50.98694, 1950, 0.,0., 7476,0
10, "LWS01", 1.,"N", "RCW103 H2 ", 16.23056, -50.98694, 1950, 0.,0., 496,11
11, "LWS04", 1.,"N", "RCW103 H2 ", 16.23056, -50.98694, 1950, 0.,0., 476,0
12, "SWS02", 2.,"N", "SN1987A ", 05.59725, -69.29944, 1950, 0.,0., 7476,13
13, "LWS01", 2.,"N", "SN1987A ", 05.59725, -69.29944, 1950, 0.,0., 496,0
14, "SWS02", 2.,"N", "SS 433 knot5 ", 19.09167, +04.82778, 1950, 0.,0., 3738,15
15, "LWS01", 2.,"N", "SS 433 knot5 ", 19.09167, +04.82778, 1950, 0.,0., 496,0
16, "SWS02", 2.,"N", "SS 433 knot3 ", 19.10972, +05.04167, 1950, 0.,0., 3738,17
17, "LWS01", 2.,"N", "SS 433 knot3 ", 19.10972, +05.04167, 1950, 0.,0., 496,0
18, "LWS04", 1.,"N", "Sgr B2 ", 17.73617, -28.36722, 1950, 0.,0., 2000,0
19, "SWS07", 1.,"N", "Sgr B2 ", 17.73617, -28.36722, 1950, 0.,0., 3040,0
20, "SWS07", 2.,"N", "Sgr A West 1 ", 17.70767, -28.98861, 1950, 0.,0.,10280,0
22, "SWS07", 1.,"N", "W51 IRS2 ", 19.35622, +14.42028, 1950, 0.,0., 8280,0
23, "LWS04", 2.,"N", "Sgr B2 ", 17.73617, -28.36722, 1950, 0.,0., 3600,0
SPRING LAUNCH TARGETS OF PROPOSAL SDRAPATZ.MPEWARM2:
====================================================
1, "SWS02", 1.,"N", "W3(OH) ", 02.38806, +61.65000, 1950, 0.,0., 1236,2
2, "SWS07", 1.,"N", "W3(OH) ", 02.38806, +61.65000, 1950, 0.,0., 5606,0
3, "SWS02", 2.,"N", "NGC 2170 IRS2 ", 06.08872, -06.37333, 1950, 0.,0., 1236,4
4, "SWS07", 2.,"N", "NGC 2170 IRS2 ", 06.08872, -06.37333, 1950, 0.,0., 2185,0
6, "LWS04", 2.,"N", "NGC 2170 IRS2 ", 06.08872, -06.37333, 1950, 0.,0., 3686,0
7, "SWS02", 2.,"N", "NGC 2170 IRS3 ", 06.08933, -06.37500, 1950, 0.,0., 1236,8
8, "SWS07", 2.,"N", "NGC 2170 IRS3 ", 06.08933, -06.37500, 1950, 0.,0., 2185,0
9, "SWS02", 2.,"N", "T Tau ", 04.31783, +19.41806, 1950, 0.,0., 1236,10
10, "SWS07", 2.,"N", "T Tau ", 04.31783, +19.41806, 1950, 0.,0., 5606,0
11, "LWS01", 2.,"N", "T Tau ", 04.31783, +19.41806, 1950, 0.,0., 496,12
12, "LWS04", 2.,"N", "T Tau ", 04.31783, +19.41806, 1950, 0.,0., 3190,0
13, "SWS02", 3.,"N", "NGC 7538 IRS1 ", 23.19358, +61.19806, 1950, 0.,0., 1236,14
14, "SWS07", 3.,"N", "NGC 7538 IRS1 ", 23.19358, +61.19806, 1950, 0.,0., 5606,0
15, "SWS02", 3.,"N", "SN1987A ", 05.59722, -69.29944, 1950, 0.,0., 7476,16
16, "LWS01", 3.,"N", "SN1987A ", 05.59722, -69.29944, 1950, 0.,0., 496,0
17, "SWS02", 3.,"N", "Crab pos1 ", 05.52483, +21.99944, 1950, 0.,0., 3738,0
18, "SWS02", 3.,"N", "Crab pos2 ", 05.52383, +21.97250, 1950, 0.,0., 3738,0
19, "SWS02", 1.,"N", "IC443 H2 pos2 ", 06.24489, +22.38444, 1950, 0.,0., 7476,0
20, "SWS02", 2.,"N", "SS 433 knot5 ", 19.09167, +04.82778, 1950, 0.,0., 3738,21
21, "LWS01", 2.,"N", "SS 433 knot5 ", 19.09167, +04.82778, 1950, 0.,0., 496,0
22, "SWS02", 2.,"N", "SS 433 knot3 ", 19.10972, +05.04167, 1950, 0.,0., 3738,23
23, "LWS01", 2.,"N", "SS 433 knot3 ", 19.10972, +05.04167, 1950, 0.,0., 496,0
24, "SWS07", 1.,"N", "Orion IRc2 ", 05.54633, -05.40694, 1950, 0.,0., 8280,0
25, "SWS07", 3.,"N", "NGC 2170 IRS3 ", 06.08933, -06.37500, 1950, 0.,0., 8280,0
26, "SWS07", 1.,"N", "W51 IRS2 ", 19.35622, +14.42028, 1950, 0.,0., 8280,0
27, "LWS04", 1.,"N", "W51 IRS2 ", 19.35622, +14.42028, 1950, 0.,0., 2000,0
28, "SWS07", 2.,"N", "Sgr A West 1 ", 17.70767, -28.98861, 1950, 0.,0., 420,0
29, "SWS02", 3.,"N", "Orion IRc2 map", 05.53855, -05.40750, 1950, 0.,0., 420,30
30, "SWS02", 3.,"N", "Orion IRc2 map", 05.54244, -05.40750, 1950, 0.,0., 260,31
31, "SWS02", 3.,"N", "Orion IRc2 map", 05.54633, -05.40750, 1950, 0.,0., 260,32
32, "SWS02", 3.,"N", "Orion IRc2 map", 05.55022, -05.40750, 1950, 0.,0., 260,33
33, "SWS02", 3.,"N", "Orion IRc2 map", 05.55411, -05.40750, 1950, 0.,0., 260,34
34, "SWS02", 3.,"N", "Orion IRc2 map", 05.53855, -05.40722, 1950, 0.,0., 260,35
35, "SWS02", 3.,"N", "Orion IRc2 map", 05.54244, -05.40722, 1950, 0.,0., 260,36
36, "SWS02", 3.,"N", "Orion IRc2 map", 05.54633, -05.40722, 1950, 0.,0., 260,37
37, "SWS02", 3.,"N", "Orion IRc2 map", 05.55022, -05.40722, 1950, 0.,0., 260,38
38, "SWS02", 3.,"N", "Orion IRc2 map", 05.55411, -05.40722, 1950, 0.,0., 260,39
39, "SWS02", 3.,"N", "Orion IRc2 map", 05.53855, -05.40694, 1950, 0.,0., 260,40
40, "SWS02", 3.,"N", "Orion IRc2 map", 05.54244, -05.40694, 1950, 0.,0., 260,41
41, "SWS02", 3.,"N", "Orion IRc2 map", 05.54633, -05.40694, 1950, 0.,0., 260,42
42, "SWS02", 3.,"N", "Orion IRc2 map", 05.55022, -05.40694, 1950, 0.,0., 260,43
43, "SWS02", 3.,"N", "Orion IRc2 map", 05.55411, -05.40694, 1950, 0.,0., 260,44
44, "SWS02", 3.,"N", "Orion IRc2 map", 05.53855, -05.40666, 1950, 0.,0., 260,45
45, "SWS02", 3.,"N", "Orion IRc2 map", 05.54244, -05.40666, 1950, 0.,0., 260,46
46, "SWS02", 3.,"N", "Orion IRc2 map", 05.54633, -05.40666, 1950, 0.,0., 260,47
47, "SWS02", 3.,"N", "Orion IRc2 map", 05.55022, -05.40666, 1950, 0.,0., 260,48
48, "SWS02", 3.,"N", "Orion IRc2 map", 05.55411, -05.40666, 1950, 0.,0., 260,49
49, "SWS02", 3.,"N", "Orion IRc2 map", 05.53855, -05.40638, 1950, 0.,0., 260,50
50, "SWS02", 3.,"N", "Orion IRc2 map", 05.54244, -05.40638, 1950, 0.,0., 260,51
51, "SWS02", 3.,"N", "Orion IRc2 map", 05.54633, -05.40638, 1950, 0.,0., 260,52
52, "SWS02", 3.,"N", "Orion IRc2 map", 05.55022, -05.40638, 1950, 0.,0., 260,53
53, "SWS02", 3.,"N", "Orion IRc2 map", 05.55411, -05.40638, 1950, 0.,0., 260,0