<=== observer ===>
"JVDHULST",\
"van der Hulst, J.M.",\
"",\
"Kapteyn Astronomical Institute",\
"",\
"P.O. Box 800",\
"9700 AV",\
"Groningen",\
"The Netherlands",\
"31 50 634054",\
"31 50 636100",\
"vdhulst@astro.rug.nl"
<=== proposal ===>
"ISM_LGR1", 1, 4,\
{"diffuse interstellar medium",\
"HII regions",\
"star formation",\
"molecular clouds",\
"normal galaxies",\
"Magellanic Clouds"},\
{"T. de Graauw",\
"L.B.F.M. Waters",\
"F.P. Israel",\
"P.P. van der Werf",\
"R. Laureijs",\
"M. Joubert",\
"J.P. Baluteau"}
<=== title ===>
Spectral Study of the Interstellar Medium and Star Formation
in Nearby Galaxies: Physical Conditions and Composition. Part 1 of 2
<=== abstract ===>
SCIENTIFIC ABSTRACT
Spectral studies of the interstellar medium (ISM) in the galaxies in
the Local Group, will enable us to probe the physical conditions and
composition of the ISM in and around star forming regions.
Fine-structure lines of several species in the infrared give us a unique
opportunity to determine temperature, density, chemical composition and
energy balance of the gas, while solid state features and transitions of
molecular hydrogen directly measure the amount of dust and state of the
molecular gas in the vicinity of the HII regions.
The strength of the major cooling lines of [CII] and [OI] will
constrain the different models for photo dissociation; especially the
[CII] emission arising from photo-dissociated gas at the molecular cloud
surfaces is very useful for probing the warm, dense molecular cloud
surfaces around star forming regions. Away from star forming regions,
the [CII] line emission can be used to probe the energy balance in the
cooler ISM.
Solid state emission features of dust (due to PAHs, such as the 11.3
mu feature), and the quadrupole transitions of radiatively excited,
hot H_2, will be used to measure the dust properties and physical
state of the molecular gas surrounding the star forming regions. These,
combined with the information from the cooling lines of [CII] and [OI],
and the fine structure lines from the HII regions themselves will enable
us to build self consistent models describing the physical conditions in
and around star forming regions, including the dissociation and heating
of the molecular clouds and dust. To get a large range in physical
properties of the surrounding molecular material we will select both
known HII regions and a few embedded star formation regions found in the
IRAS survey of the Magellanic Clouds.
To obtain information about the cool molecular gas observations of
the 17 mu line of H_2 are planned in a companion SOT proposal by
R. Laureijs et al. The 17 mu line of cool H_2 will be faint
and will be tried in two specific lines of sight. Photo dissociation
region (PDR) models for the LMC HII regions, indicate that the line may
be stronger than in Galactic HII regions because of the lower dust
content and hence the greater penetration of the UV radiation field into
the molecular clouds. A search for other molecular lines will be made
along the same line of sight.
The selected objects are the brightest HII regions in the LMC, SMC
and M33. The LMC and SMC regions have been selected in coordination
with members of the other ISO consortia (ISOCAM, ISOPHOT, LWS ans SOT)
to ensure maximum overlap with proposed observations for the other ISO
instruments. The regions in the Magellanic Clouds fall in three
categories: diffuse, extended HII regions such as 30 Doradus, compact
and high excitation regions such as N88 and N81 and a couple of hot and
cool molecular clouds (LIRS 36, LIRS 49 and SMC-B1#1). The seven HII
regions in M33 have been chosen to ensure a wide range in galactocentric
radius and hence metallicity and physical conditions.
OBSERVATION SUMMARY
The main instruments used for this spectroscopic study of
extragalactic HII regions and the ISM in nearby galaxies will be the
SWS, the LWS and ISOPHOT-S. The SWS and LWS are to be used in grating
scanning mode. The total observing time for this program is around 40
hours.
The first observations will be complete grating scans of 30 Doradus
and NGC 604. Quick reduction of these spectra will show whether the
choice of lines and estimated line strengths of the proposed study are
correct. These results will determine the detailed observing strategy.
The selected lines for the other HII region study are given below (table
3) and will be observed in individual grating settings in the case of
the SWS. The lines are spread out in such a way over the short
wavelength and over the long wavelength section of the SWS that most
lines can be observed simultaneously thus improving the observing
efficience greatly. The LWS will be used in full grating scan mode as
this is not less efficient than having about 6 separate grating
settings. Coverage of the HII regions in the Magellanic Clouds with LWS
is provided by a complementary LWS proposal by P. Cox et al.
At each position not covered by other proposals we will take an
ISOPHOT-S exposure to get a low resolution spectrum between 2.5 and 12
mu for measuring broad spectral features such as those from PAH's.
The efficiency of ISOPHOT-S is such that a very short exposure of 2
minutes provides sufficient signal to noise.
Similarly we will take short PHOT exposures at 25, 60, 100 and 160
mu (PHOT-P2 in P25, PHOT-C1 in C60 and C100 and PHOT-C2 in C160) and
a short CAM exposure on those positions not covered by other proposals.
Exposures of 2 - 4 minutes each are sufficient and add little extra to
the total observing time for this program. These will provide
information about the distribution of emission in the field of view and
about the IR spectrum (i.e. dust temperature) of the HII regions under
study.
<=== scientific_justification ===>
Time distribution for spring launch targets:
Team top 40% second 30% last 30%
SWS: 53390 36058 51512
Time distribution for autumn launch targets:
Team top 40% second 30% last 30%
SWS: 57157 39801 49512
Table 1. Positions and source names
---------------------------------------------------------------------------
No. RA Dec source name
1950
1 05 38 54.2 -69 08 00 30 Doradus #1
2 05 38 56.0 -69 07 13.9 30 Doradus #2
3 05 39 06.5 -69 06 40 30 Doradus #3
4 05 39 14.7 -69 06 46.7 30 Doradus #4
5 05 40 31 -69 46 09 N 159-5
6 05 37 48 -69 02 00 N 157
7 04 57 10 -66 27 54 N 11A
8 05 54 41 -69 15 39 N 83B
9 05 39 44 -69 39 10 N 160A1
10 05 39 46.1 -69 38 56 N 160A2
11 05 39 44.4 -69 38 51.4 N 160A3
12 04 52 06 -69 29 30 N 79A
13 04 52 03 -67 00 20 N 4A
14 00 57 27 -72 26 36 N 66
15 00 43 29 -73 21 23 N 12
16 00 46 36 -73 22 16 N 27
17 01 22 55 -73 24 53 N 88
18 01 07 41 -73 28 05 N 81
19 00 46 33 -73 21 50 LIRS 49
20 00 44 51 -73 22 33 LIRS 36
21 00 43 42 -73 35 10 SMC-B1#1
22 01 31 44 30 31 44 NGC 604
23 01 30 45 30 26 08 NGC 595
24 01 29 56 30 23 35 NGC 588
25 01 30 23 30 23 19 NGC 592
26 01 30 27 30 41 21 IC 132
27 01 30 27 30 37 30 IC 133
28 01 31 06 30 30 00 IC 142
---------------------------------------------------------------------------
Table 2a. Source list for autumn launch
--------------------------------------
No. Name Priority AOT time LWS CAM PHT
--------------------------------------
1 30 Doradus#1 1 SWS06 6600 + + + full scan
1 PHT40 128
1 PHT25 192
1 PHT05 64
2 30 Doradus#2 1 SWS02 2757 +
1 PHT40 128
1 PHT25 192
1 PHT05 64
3 30 Doradus#3 1 PHT25 372
1 PHT05 64
4 30 Doradus#4 2 SWS02 2757 +
2 PHT40 128
2 PHT25 192
2 PHT05 64
5 N 159-5 1 SWS02 3600 + +
1 CAM01 180
6 N 157 2 SWS02 3600 + +
2 PHT40 128
2 PHT25 192
2 PHT05 64
2 CAM01 180
7 N 11A 1 SWS02 3600 + + +
8 N 83B 2 SWS02 3600 + +
2 CAM01 180
9 N 160A1 1 SWS02 3600 + +
1 CAM01 180
10 N 160A2 1 SWS02 3600 + +
1 CAM01 180
11 N 160A3 1 SWS02 3600
1 CAM01 180
12 N 79A 3 SWS02 3600 + +
3 PHT40 128
3 PHT25 192
3 PHT05 64
3 CAM01 180
13 N 4A 3 SWS02 3600 + + +
3 PHT40 128
3 PHT25 192
3 PHT05 64
14 N 66 1 SWS02 3600 + + +
1 PHT40 128
1 PHT25 192
1 PHT05 64
15 N 12 3 SWS02 3600 + +
3 PHT40 128
3 PHT25 192
3 PHT05 64
3 CAM01 180
17 N 88 1 SWS02 3600 + +
1 CAM01 180
18 N 81 1 SWS02 3600 + +
1 CAM01 180
19 LIRS 49 1 SWS02 3600 + + +
1 PHT40 128
1 PHT25 192
1 PHT05 64
20 LIRS 36 2 SWS02 3600 + + +
2 PHT40 128
2 PHT25 192
2 PHT05 64
21 SMC-B1#1 1 SWS02 3600 + +
1 PHT40 128
1 PHT25 192
1 PHT05 64
1 CAM01 180
22 NGC 604 1 SWS06 6600 + + + full scan
1 LWS01 1200
1 PHT40 128
1 PHT25 192
1 PHT05 64
23 NGC 595 2 SWS02 6600 + + +
2 LWS01 1200
2 PHT40 128
2 PHT25 192
2 PHT05 64
24 NGC 588 2 SWS02 6600 + +
2 LWS01 1200
2 PHT40 128
2 PHT25 192
2 PHT05 64
2 CAM01 180
25 NGC 592 3 SWS02 6600 + +
3 LWS01 1200
3 PHT40 128
3 PHT25 192
3 PHT05 64
3 CAM01 180
27 IC 133 2 SWS02 6600 + + +
2 LWS01 1200
2 PHT40 128
2 PHT25 192
2 PHT05 64
28 IC 142 3 SWS02 6600 + +
3 LWS01 1200
3 PHT40 128
3 PHT25 192
3 PHT05 64
3 CAM01 180
--------------------------------------
Table 2b. Source list for spring launch
--------------------------------------
No. Name Priority AOT time LWS CAM PHT
--------------------------------------
1 30 Doradus#1 1 SWS06 6600 + + + full scan
1 PHT40 128
1 PHT25 192
1 PHT05 64
2 30 Doradus#2 1 SWS02 2974 +
1 PHT40 128
1 PHT25 192
1 PHT05 64
3 30 Doradus#3 1 PHT25 372 +
1 PHT05 64
4 30 Doradus#4 2 SWS02 2974 +
2 PHT40 128
2 PHT25 192
2 PHT05 64
5 N 159-5 1 SWS02 3600 + +
1 CAM01 180
6 N 157 3 SWS02 3600 + +
3 PHT40 128
3 PHT25 192
3 PHT05 64
3 CAM01 180
7 N 11A 1 SWS02 3600 + + +
8 N 83B 3 SWS02 3600 + +
3 CAM01 180
9 N 160A1 1 SWS02 3600 + +
1 CAM01 180
10 N 160A2 1 SWS02 3600 + +
1 CAM01 180
11 N 160A3 1 SWS02 3600
1 CAM01 180
12 N 79A 3 SWS02 3600 + +
3 PHT40 128
3 PHT25 192
3 PHT05 64
3 CAM01 180
13 N 4A 3 SWS02 3600 + + +
3 PHT40 128
3 PHT25 192
3 PHT05 64
14 N 66 2 SWS02 3600 + + +
2 PHT40 128
2 PHT25 192
2 PHT05 64
15 N 12 3 SWS02 3600 + +
3 PHT40 128
3 PHT25 192
3 PHT05 64
3 CAM01 180
16 N 27 3 SWS02 3600 + +
3 PHT40 128
3 PHT25 192
3 PHT05 64
3 CAM01 180
17 N 88 1 SWS02 3600 + +
1 CAM01 180
18 N 81 1 SWS02 3600 + +
1 CAM01 180
19 LIRS 49 1 SWS02 3600 + + +
1 PHT40 128
1 PHT25 192
1 PHT05 64
20 LIRS 36 2 SWS02 3600 + + +
2 PHT40 128
2 PHT25 192
2 PHT05 64
21 SMC-B1#1 1 SWS02 3600 + +
1 PHT40 128
1 PHT25 192
1 PHT05 64
1 CAM01 180
22 NGC 604 1 SWS06 6600 + + + full scan
1 LWS01 1200
1 PHT40 128
1 PHT25 192
1 PHT05 64
23 NGC 595 2 SWS02 6600 + + +
2 LWS01 1200
2 PHT40 128
2 PHT25 192
2 PHT05 64
24 NGC 588 2 SWS02 6600 + +
2 LWS01 1200
2 PHT40 128
2 PHT25 192
2 PHT05 64
2 CAM01 180
25 NGC 592 3 SWS02 6600 + +
3 LWS01 1200
3 PHT40 128
3 PHT25 192
3 PHT05 64
3 CAM01 180
26 IC 132 3 SWS02 6600 + +
3 LWS01 1200
3 PHT40 128
3 PHT25 192
3 PHT05 64
3 CAM01 180
27 IC 133 2 SWS02 6600 + + +
2 LWS01 1200
2 PHT40 128
2 PHT25 192
2 PHT05 64
28 IC 142 3 SWS02 6600 + +
3 LWS01 1200
3 PHT40 128
3 PHT25 192
3 PHT05 64
3 CAM01 180
--------------------------------------
---------------------------------------------------------------------------
Table 3. Lines and Spectral Ranges
---------------------------------------------------------------------------
No. Atom/Ion/ Trans. Wavelength Instr. AOT average integration times (sec)
Mol. (Range) LMC/SMC M33
Br alpha 4.04 micron SWS02 160 160
HeI 4.29 micron SWS02 160 640
ArII 6.98 micron SWS02 160 320
ArIII 8.99 micron SWS02 80 160
FEVII 9.51 micron SWS02 80 160
SIV 10.5 micron SWS02 160 320
NeII 12.8 micron SWS02 80 160
NeIII 15.6 micron SWS02 160 320
NeIII 36.0 micron SWS02 80 320
SIII 18.7 micron SWS02 80 320
SIII 33.6 micron SWS02 80 320
OIV 25.9 micron SWS02 80 80
FeII 26 micron SWS02 80 80
SiII 35 micron SWS02 80 320
OIII 52 micron LWS01 --
NIII 57 micron LWS01 |
OIII 88 micron LWS01 | full scan:
NII 122 micron LWS01 |
OI 63 micron LWS01 | - 1200
CII 158 micron LWS01 --
1-0 O(2) 2.63 micron SWS02 160 640
1-0 O(3) 2.80 micron SWS02 160 640
1-0 Q(1) 2.41 micron SWS02 640 640
2-1 Q(1) 2.55 micron SWS02 640 640
Silicate,PAH 9,11 micron PHT40 128 128
---------------------------------------------------------------------------
<=== autumn_launch_targets ===>
1, "SWS06",1.,"N", "30 Doradus#1", 5.64839, -69.13333, 1950,0.,0., 6600, 2
2, "PHT40",1.,"N", "30 Doradus#1", 5.64839, -69.13333, 1950,0.,0., 128, 3
3, "PHT25",1.,"N", "30 Doradus#1", 5.64839, -69.13333, 1950,0.,0., 192, 4
4, "PHT05",1.,"N", "30 Doradus#1", 5.64839, -69.13333, 1950,0.,0., 64, 0
5, "SWS02",1.,"N", "30 Doradus#2", 5.64889, -69.12053, 1950,0.,0., 2757, 6
6, "PHT40",1.,"N", "30 Doradus#2", 5.64889, -69.12053, 1950,0.,0., 128, 7
7, "PHT25",1.,"N", "30 Doradus#2", 5.64889, -69.12053, 1950,0.,0., 192, 8
8, "PHT05",1.,"N", "30 Doradus#2", 5.64889, -69.12053, 1950,0.,0., 64, 0
9, "PHT25",1.,"N", "30 Doradus#3", 5.65181, -69.11111, 1950,0.,0., 372, 10
10, "PHT05",1.,"N", "30 Doradus#3", 5.65191, -69.11111, 1950,0.,0., 64, 0
11, "SWS02",2.,"N", "30 Doradus#4", 5.65408, -69.11197, 1950,0.,0., 2757, 12
12, "PHT40",2.,"N", "30 Doradus#4", 5.65408, -69.11197, 1950,0.,0., 128, 13
13, "PHT25",2.,"N", "30 Doradus#4", 5.65408, -69.11197, 1950,0.,0., 192, 14
14, "PHT05",2.,"N", "30 Doradus#4", 5.65408, -69.11197, 1950,0.,0., 64, 0
15, "SWS02",1.,"N", "N 159-5 ", 5.67528, -69.76917, 1950,0.,0., 3600, 16
16, "CAM01",1.,"N", "N 159-5 ", 5.67528, -69.76917, 1950,0.,0., 180, 0
17, "SWS02",2.,"N", "N 157 ", 5.63000, -69.03333, 1950,0.,0., 3600, 18
18, "PHT40",2.,"N", "N 157 ", 5.63000, -69.03333, 1950,0.,0., 128, 19
19, "PHT25",2.,"N", "N 157 ", 5.63000, -69.03333, 1950,0.,0., 192, 20
20, "PHT05",2.,"N", "N 157 ", 5.63000, -69.03333, 1950,0.,0., 64, 21
21, "CAM01",2.,"N", "N 157 ", 5.63000, -69.03333, 1950,0.,0., 180, 0
22, "SWS02",1.,"N", "N 11A ", 4.95278, -66.46500, 1950,0.,0., 3600, 0
23, "SWS02",2.,"N", "N 83B ", 5.91139, -69.26083, 1950,0.,0., 3600, 24
24, "CAM01",2.,"N", "N 83B ", 5.91139, -69.26083, 1950,0.,0., 180, 0
25, "SWS02",1.,"N", "N 160A1 ", 5.66222, -69.65278, 1950,0.,0., 3600, 26
26, "CAM01",1.,"N", "N 160A1 ", 5.66222, -69.65278, 1950,0.,0., 180, 0
27, "SWS02",1.,"N", "N 160A2 ", 5.66281, -69.64889, 1950,0.,0., 3600, 28
28, "CAM01",1.,"N", "N 160A2 ", 5.66281, -69.64889, 1950,0.,0., 180, 0
29, "SWS02",1.,"N", "N 160A3 ", 5.66233, -69.64761, 1950,0.,0., 3600, 30
30, "CAM01",1.,"N", "N 160A3 ", 5.66233, -69.64761, 1950,0.,0., 180, 0
31, "SWS02",3.,"N", "N 79A ", 4.86833, -69.49167, 1950,0.,0., 3600, 32
32, "PHT40",3.,"N", "N 79A ", 4.86833, -69.49167, 1950,0.,0., 128, 33
33, "PHT25",3.,"N", "N 79A ", 4.86833, -69.49167, 1950,0.,0., 192, 34
34, "PHT05",3.,"N", "N 79A ", 4.86833, -69.49167, 1950,0.,0., 64, 35
35, "CAM01",3.,"N", "N 79A ", 4.86833, -69.49167, 1950,0.,0., 180, 0
36, "SWS02",3.,"N", "N 4A ", 4.86750, -67.00556, 1950,0.,0., 3600, 37
37, "PHT40",3.,"N", "N 4A ", 4.86750, -67.00556, 1950,0.,0., 128, 38
38, "PHT25",3.,"N", "N 4A ", 4.86750, -67.00556, 1950,0.,0., 192, 39
39, "PHT05",3.,"N", "N 4A ", 4.86750, -67.00556, 1950,0.,0., 64, 40
40, "SWS02",1.,"N", "N 66 ", 0.95750, -72.44333, 1950,0.,0., 3600, 41
41, "PHT40",1.,"N", "N 66 ", 0.95750, -72.44333, 1950,0.,0., 128, 42
42, "PHT25",1.,"N", "N 66 ", 0.95750, -72.44333, 1950,0.,0., 192, 43
43, "PHT05",1.,"N", "N 66 ", 0.95750, -72.44333, 1950,0.,0., 64, 0
44, "SWS02",3.,"N", "N 12 ", 0.72472, -73.35639, 1950,0.,0., 3600, 45
45, "PHT40",3.,"N", "N 12 ", 0.72472, -73.35639, 1950,0.,0., 128, 46
46, "PHT25",3.,"N", "N 12 ", 0.72472, -73.35639, 1950,0.,0., 192, 47
47, "PHT05",3.,"N", "N 12 ", 0.72472, -73.35639, 1950,0.,0., 64, 48
48, "CAM01",3.,"N", "N 12 ", 0.72472, -73.35639, 1950,0.,0., 180, 0
49, "SWS02",1.,"N", "N 88 ", 1.38194, -73.41472, 1950,0.,0., 3600, 50
50, "CAM01",1.,"N", "N 88 ", 1.38194, -73.41472, 1950,0.,0., 180, 0
51, "SWS02",1.,"N", "N 81 ", 1.12806, -73.46806, 1950,0.,0., 3600, 52
52, "CAM01",1.,"N", "N 81 ", 1.12806, -73.46806, 1950,0.,0., 180, 0
53, "SWS02",1.,"N", "LIRS 49 ", 0.77583, -73.36389, 1950,0.,0., 3600, 54
54, "PHT40",1.,"N", "LIRS 49 ", 0.77583, -73.36389, 1950,0.,0., 128, 55
55, "PHT25",1.,"N", "LIRS 49 ", 0.77583, -73.36389, 1950,0.,0., 192, 56
56, "PHT05",1.,"N", "LIRS 49 ", 0.77583, -73.36389, 1950,0.,0., 64, 57
57, "SWS02",2.,"N", "LIRS 36 ", 0.74750, -73.37583, 1950,0.,0., 3600, 58
58, "PHT40",2.,"N", "LIRS 36 ", 0.74750, -73.37583, 1950,0.,0., 128, 59
59, "PHT25",2.,"N", "LIRS 36 ", 0.74750, -73.37583, 1950,0.,0., 192, 60
60, "PHT05",2.,"N", "LIRS 36 ", 0.74750, -73.37583, 1950,0.,0., 64, 61
61, "SWS02",1.,"N", "SMC-B1#1 ", 0.72833, -73.58611, 1950,0.,0., 3600, 62
62, "PHT40",1.,"N", "SMC-B1#1 ", 0.72833, -73.58611, 1950,0.,0., 128, 63
63, "PHT25",1.,"N", "SMC-B1#1 ", 0.72833, -73.58611, 1950,0.,0., 192, 64
64, "PHT05",1.,"N", "SMC-B1#1 ", 0.72833, -73.58611, 1950,0.,0., 64, 65
65, "CAM01",1.,"N", "SMC-B1#1 ", 0.72833, -73.58611, 1950,0.,0., 180, 0
66, "SWS06",1.,"N", "NGC 604 ", 1.52889, 30.52889, 1950,0.,0., 6600, 67
67, "LWS01",1.,"N", "NGC 604 ", 1.52889, 30.52889, 1950,0.,0., 1200, 68
68, "PHT40",1.,"N", "NGC 604 ", 1.52889, 30.52889, 1950,0.,0., 128, 69
69, "PHT25",1.,"N", "NGC 604 ", 1.52889, 30.52889, 1950,0.,0., 192, 70
70, "PHT05",1.,"N", "NGC 604 ", 1.52889, 30.52889, 1950,0.,0., 64, 0
71, "SWS02",2.,"N", "NGC 595 ", 1.51250, 30.43556, 1950,0.,0., 6600, 72
72, "LWS01",2.,"N", "NGC 595 ", 1.51250, 30.43556, 1950,0.,0., 1200, 73
73, "PHT40",2.,"N", "NGC 595 ", 1.51250, 30.43556, 1950,0.,0., 128, 74
74, "PHT25",2.,"N", "NGC 595 ", 1.51250, 30.43556, 1950,0.,0., 192, 75
75, "PHT05",2.,"N", "NGC 595 ", 1.51250, 30.43556, 1950,0.,0., 64, 0
76, "SWS02",2.,"N", "NGC 588 ", 1.49889, 30.39306, 1950,0.,0., 6600, 77
77, "LWS01",2.,"N", "NGC 588 ", 1.49889, 30.39306, 1950,0.,0., 1200, 78
78, "PHT40",2.,"N", "NGC 588 ", 1.49889, 30.39306, 1950,0.,0., 128, 79
79, "PHT25",2.,"N", "NGC 588 ", 1.49889, 30.39306, 1950,0.,0., 192, 80
80, "PHT05",2.,"N", "NGC 588 ", 1.49889, 30.39306, 1950,0.,0., 64, 81
81, "CAM01",2.,"N", "NGC 588 ", 1.49889, 30.39306, 1950,0.,0., 180, 0
82, "SWS02",3.,"N", "NGC 592 ", 1.50639, 30.38861, 1950,0.,0., 6600, 83
83, "LWS01",3.,"N", "NGC 592 ", 1.50639, 30.38861, 1950,0.,0., 1200, 84
84, "PHT40",3.,"N", "NGC 592 ", 1.50639, 30.38861, 1950,0.,0., 128, 85
85, "PHT25",3.,"N", "NGC 592 ", 1.50639, 30.38861, 1950,0.,0., 192, 86
86, "PHT05",3.,"N", "NGC 592 ", 1.50639, 30.38861, 1950,0.,0., 64, 87
87, "CAM01",3.,"N", "NGC 592 ", 1.50639, 30.38861, 1950,0.,0., 180, 0
<=== spring_launch_targets ===>
1, "SWS06",1.,"N", "30 Doradus#1", 5.64839, -69.13333, 1950,0.,0., 6600, 2
2, "PHT40",1.,"N", "30 Doradus#1", 5.64839, -69.13333, 1950,0.,0., 128, 3
3, "PHT25",1.,"N", "30 Doradus#1", 5.64839, -69.13333, 1950,0.,0., 192, 4
4, "PHT05",1.,"N", "30 Doradus#1", 5.64839, -69.13333, 1950,0.,0., 64, 0
5, "SWS02",1.,"N", "30 Doradus#2", 5.64889, -69.12053, 1950,0.,0., 2974, 6
6, "PHT40",1.,"N", "30 Doradus#2", 5.64889, -69.12053, 1950,0.,0., 128, 7
7, "PHT25",1.,"N", "30 Doradus#2", 5.64889, -69.12053, 1950,0.,0., 192, 8
8, "PHT05",1.,"N", "30 Doradus#2", 5.64889, -69.12053, 1950,0.,0., 64, 0
9, "PHT25",1.,"N", "30 Doradus#3", 5.65181, -69.11111, 1950,0.,0., 372, 10
10, "PHT05",1.,"N", "30 Doradus#3", 5.65191, -69.11111, 1950,0.,0., 64, 0
11, "SWS02",2.,"N", "30 Doradus#4", 5.65408, -69.11197, 1950,0.,0., 2974, 12
12, "PHT40",2.,"N", "30 Doradus#4", 5.65408, -69.11197, 1950,0.,0., 128, 13
13, "PHT25",2.,"N", "30 Doradus#4", 5.65408, -69.11197, 1950,0.,0., 192, 14
14, "PHT05",2.,"N", "30 Doradus#4", 5.65408, -69.11197, 1950,0.,0., 64, 0
15, "SWS02",1.,"N", "N 159-5 ", 5.67528, -69.76917, 1950,0.,0., 3600, 16
16, "CAM01",1.,"N", "N 159-5 ", 5.67528, -69.76917, 1950,0.,0., 180, 0
17, "SWS02",3.,"N", "N 157 ", 5.63000, -69.03333, 1950,0.,0., 3600, 18
18, "PHT40",3.,"N", "N 157 ", 5.63000, -69.03333, 1950,0.,0., 128, 19
19, "PHT25",3.,"N", "N 157 ", 5.63000, -69.03333, 1950,0.,0., 192, 20
20, "PHT05",3.,"N", "N 157 ", 5.63000, -69.03333, 1950,0.,0., 64, 21
21, "CAM01",3.,"N", "N 157 ", 5.63000, -69.03333, 1950,0.,0., 180, 0
22, "SWS02",1.,"N", "N 11A ", 4.95278, -66.46500, 1950,0.,0., 3600, 0
23, "SWS02",3.,"N", "N 83B ", 5.91139, -69.26083, 1950,0.,0., 3600, 24
24, "CAM01",3.,"N", "N 83B ", 5.91139, -69.26083, 1950,0.,0., 180, 0
25, "SWS02",1.,"N", "N 160A1 ", 5.66222, -69.65278, 1950,0.,0., 3600, 26
26, "CAM01",1.,"N", "N 160A1 ", 5.66222, -69.65278, 1950,0.,0., 180, 0
27, "SWS02",1.,"N", "N 160A2 ", 5.66281, -69.64889, 1950,0.,0., 3600, 28
28, "CAM01",1.,"N", "N 160A2 ", 5.66281, -69.64889, 1950,0.,0., 180, 0
29, "SWS02",1.,"N", "N 160A3 ", 5.66233, -69.64761, 1950,0.,0., 3600, 30
30, "CAM01",1.,"N", "N 160A3 ", 5.66233, -69.64761, 1950,0.,0., 180, 0
31, "SWS02",3.,"N", "N 79A ", 4.86833, -69.49167, 1950,0.,0., 3600, 32
32, "PHT40",3.,"N", "N 79A ", 4.86833, -69.49167, 1950,0.,0., 128, 33
33, "PHT25",3.,"N", "N 79A ", 4.86833, -69.49167, 1950,0.,0., 192, 34
34, "PHT05",3.,"N", "N 79A ", 4.86833, -69.49167, 1950,0.,0., 64, 35
35, "CAM01",3.,"N", "N 79A ", 4.86833, -69.49167, 1950,0.,0., 180, 0
36, "SWS02",3.,"N", "N 4A ", 4.86750, -67.00556, 1950,0.,0., 3600, 37
37, "PHT40",3.,"N", "N 4A ", 4.86750, -67.00556, 1950,0.,0., 128, 38
38, "PHT25",3.,"N", "N 4A ", 4.86750, -67.00556, 1950,0.,0., 192, 39
39, "PHT05",3.,"N", "N 4A ", 4.86750, -67.00556, 1950,0.,0., 64, 40
40, "SWS02",2.,"N", "N 66 ", 0.95750, -72.44333, 1950,0.,0., 3600, 41
41, "PHT40",2.,"N", "N 66 ", 0.95750, -72.44333, 1950,0.,0., 128, 42
42, "PHT25",2.,"N", "N 66 ", 0.95750, -72.44333, 1950,0.,0., 192, 43
43, "PHT05",2.,"N", "N 66 ", 0.95750, -72.44333, 1950,0.,0., 64, 0
44, "SWS02",3.,"N", "N 12 ", 0.72472, -73.35639, 1950,0.,0., 3600, 45
45, "PHT40",3.,"N", "N 12 ", 0.72472, -73.35639, 1950,0.,0., 128, 46
46, "PHT25",3.,"N", "N 12 ", 0.72472, -73.35639, 1950,0.,0., 192, 47
47, "PHT05",3.,"N", "N 12 ", 0.72472, -73.35639, 1950,0.,0., 64, 48
48, "CAM01",3.,"N", "N 12 ", 0.72472, -73.35639, 1950,0.,0., 180, 0
49, "SWS02",3.,"N", "N 27 ", 0.77667, -73.37111, 1950,0.,0., 3600, 50
50, "PHT40",3.,"N", "N 27 ", 0.77667, -73.37111, 1950,0.,0., 128, 51
51, "PHT25",3.,"N", "N 27 ", 0.77667, -73.37111, 1950,0.,0., 192, 52
52, "PHT05",3.,"N", "N 27 ", 0.77667, -73.37111, 1950,0.,0., 64, 53
53, "CAM01",3.,"N", "N 27 ", 0.77667, -73.37111, 1950,0.,0., 180, 0
54, "SWS02",1.,"N", "N 88 ", 1.38194, -73.41472, 1950,0.,0., 3600, 55
55, "CAM01",1.,"N", "N 88 ", 1.38194, -73.41472, 1950,0.,0., 180, 0
56, "SWS02",1.,"N", "N 81 ", 1.12806, -73.46806, 1950,0.,0., 3600, 57
57, "CAM01",1.,"N", "N 81 ", 1.12806, -73.46806, 1950,0.,0., 180, 0
58, "SWS02",1.,"N", "LIRS 49 ", 0.77583, -73.36389, 1950,0.,0., 3600, 59
59, "PHT40",1.,"N", "LIRS 49 ", 0.77583, -73.36389, 1950,0.,0., 128, 60
60, "PHT25",1.,"N", "LIRS 49 ", 0.77583, -73.36389, 1950,0.,0., 192, 61
61, "PHT05",1.,"N", "LIRS 49 ", 0.77583, -73.36389, 1950,0.,0., 64, 62
62, "SWS02",2.,"N", "LIRS 36 ", 0.74750, -73.37583, 1950,0.,0., 3600, 63
63, "PHT40",2.,"N", "LIRS 36 ", 0.74750, -73.37583, 1950,0.,0., 128, 64
64, "PHT25",2.,"N", "LIRS 36 ", 0.74750, -73.37583, 1950,0.,0., 192, 65
65, "PHT05",2.,"N", "LIRS 36 ", 0.74750, -73.37583, 1950,0.,0., 64, 66
66, "SWS02",1.,"N", "SMC-B1#1 ", 0.72833, -73.58611, 1950,0.,0., 3600, 67
67, "PHT40",1.,"N", "SMC-B1#1 ", 0.72833, -73.58611, 1950,0.,0., 128, 68
68, "PHT25",1.,"N", "SMC-B1#1 ", 0.72833, -73.58611, 1950,0.,0., 192, 69
69, "PHT05",1.,"N", "SMC-B1#1 ", 0.72833, -73.58611, 1950,0.,0., 64, 70
70, "CAM01",1.,"N", "SMC-B1#1 ", 0.72833, -73.58611, 1950,0.,0., 180, 0
71, "SWS06",1.,"N", "NGC 604 ", 1.52889, 30.52889, 1950,0.,0., 6600, 72
72, "LWS01",1.,"N", "NGC 604 ", 1.52889, 30.52889, 1950,0.,0., 1200, 73
73, "PHT40",1.,"N", "NGC 604 ", 1.52889, 30.52889, 1950,0.,0., 128, 74
74, "PHT25",1.,"N", "NGC 604 ", 1.52889, 30.52889, 1950,0.,0., 192, 75
75, "PHT05",1.,"N", "NGC 604 ", 1.52889, 30.52889, 1950,0.,0., 64, 0
76, "SWS02",2.,"N", "NGC 595 ", 1.51250, 30.43556, 1950,0.,0., 6600, 77
77, "LWS01",2.,"N", "NGC 595 ", 1.51250, 30.43556, 1950,0.,0., 1200, 78
78, "PHT40",2.,"N", "NGC 595 ", 1.51250, 30.43556, 1950,0.,0., 128, 79
79, "PHT25",2.,"N", "NGC 595 ", 1.51250, 30.43556, 1950,0.,0., 192, 80
80, "PHT05",2.,"N", "NGC 595 ", 1.51250, 30.43556, 1950,0.,0., 64, 0
81, "SWS02",2.,"N", "NGC 588 ", 1.49889, 30.39306, 1950,0.,0., 6600, 82
82, "LWS01",2.,"N", "NGC 588 ", 1.49889, 30.39306, 1950,0.,0., 1200, 83
83, "PHT40",2.,"N", "NGC 588 ", 1.49889, 30.39306, 1950,0.,0., 128, 84
84, "PHT25",2.,"N", "NGC 588 ", 1.49889, 30.39306, 1950,0.,0., 192, 85
85, "PHT05",2.,"N", "NGC 588 ", 1.49889, 30.39306, 1950,0.,0., 64, 86
86, "CAM01",2.,"N", "NGC 588 ", 1.49889, 30.39306, 1950,0.,0., 180, 0
87, "SWS02",3.,"N", "NGC 592 ", 1.50639, 30.38861, 1950,0.,0., 6600, 88
88, "LWS01",3.,"N", "NGC 592 ", 1.50639, 30.38861, 1950,0.,0., 1200, 89
89, "PHT40",3.,"N", "NGC 592 ", 1.50639, 30.38861, 1950,0.,0., 128, 90
90, "PHT25",3.,"N", "NGC 592 ", 1.50639, 30.38861, 1950,0.,0., 192, 91
91, "PHT05",3.,"N", "NGC 592 ", 1.50639, 30.38861, 1950,0.,0., 64, 92
92, "CAM01",3.,"N", "NGC 592 ", 1.50639, 30.38861, 1950,0.,0., 180, 0