<=== observer ===>
"HVOELK",\
"Voelk, H.J.",\
"",\
"Max-Planck-Institut fuer Kernphysik",\
"Saupfercheckweg 1",\
"103980",\
"D-69029",\
"Heidelberg",\
"Germany",\
" 496221516295",\
" 496221516324",\
"vlk@vampi.mpi-hd.mpg.de"
<=== proposal ===>
"VIRGO1",1,4,\
{"galaxy clusters","normal galaxies","irregular galaxies"},\
{"Hippelein, H.","Leech, K.","Metcalfe, L.",\
"Skaley, D.","Tuffs, R.J.","Xu, C."}
<=== title ===>
Statistical Sample of Late-Type Galaxies from the VIRGO Cluster
Part 1
<=== abstract ===>
SCIENTIFIC ABSTRACT
We propose to study a complete volume-limited unbiased sample of 118 spiral,
irregular and dwarf galaxies from the VIRGO cluster in the 40 - 220 micron
spectral range with ISOPHOT. The completeness limit of Bt = 18 magnitude
corresponds to the maximum (confusion limited) depth the instrument can achieve,
allowing a complete dynamic range in star-formation activity to be measured. In
parallel, wherever instrument sensitivity permits, we propose a degree of
spectro-photometric resolution which by far exceeds that of IRAS, to provide a
basis for distinguishing between dust components of different temperatures and
grain size distributions in the galaxian interstellar media. These FIR
observations will furthermore spatially resolve the central region from the disk
for the giant spirals with diameters exceeding a few arcminutes. This should
allow a distinction between FIR activity in the centres and the disks for about
half the galaxies in the sample. Using LWS, we further propose to survey a
subsample of 50 spiral galaxies with integrated blue magnitudes Bt < 14.5 for
emission in the [CII] 158 micron fine structure line.
OBSERVATION SUMMARY
It is proposed to make the FIR continuum measurements at diffraction-limited
angular resolutions with the PHT-C200 array in the C120, C160 and C200 filters,
and with the C100 array in the C60, C70 and C100 filters. These filters provide
the widest spectral range with an even spectral sampling. The use of the C60 and
C100 micron filters will facilitate a cross calibration with the IRAS all sky
survey. Irregular and dwarf galaxies will only be observed in the wide-band C60,
C100 and C160 filters. Photometry for the fainter targets will be made using the
PHT22 AOT with the focal plane chopper operating in it's "triangular" waveform
mode. This should enable us to reach the confusion limit due to foreground
cirrus of a few mJy rms at 100 micron, sufficient to detect a Bt = 18 magnitude
VIRGO dwarf galaxy with a predicted FIR flux density of the order of 10 mJy. To
provide optimum protection against confusion in the 120 - 200 micron spectral
range, small spatially oversampled scans through each source will be performed
using the PHT32 AOT. Use of the PHT32 AOT is also necessary to measure spatially
integrated flux densities from the disks of brighter spiral galaxies whose
spatial extent exceeds the unvignetted field of view of ISO. The close pair
VCC1673 and VCC1676 will be covered by common rasters.
Exposure times in each ISOPHOT filter were selected in the range 8 - 64s
according to the integrated blue magnitude of the galaxy and whether it had
been detected by IRAS. The limiting sensitivity of the survey, corresponding to
the longest integrations in the broad band C60, C100 and C160 filters, is
approximately 10mJy (3 sigma). Table A in the scientific justification section
(below) tabulates exposure times in each filter, the spacecraft raster, and
the coordinates for each AOT execution on a target galaxy (observations of
background are not included) in this part of the proposal.
The measured ratios of galaxian fluxes and brightnesses to the (generally much
brighter) background from zodiacal- and broad-scale cirrus emission will be
calibrated by concatenating observations of galaxies in a particular region to
absolute photometric measurements of the background using the PHT25 AOT in the
same 6 PHT-C filters. East of 12h 42m, where visibility is poor for a spring
launch at the limit of the launch window, concatenations are <= 1.1 hours.
The LWS survey will be in the grating mode to reach a (3 sigma) limiting line
flux of approximately 3.10**(-17)Wm**(-2). Details of the observations with LWS
of the subsample of 50 spiral galaxies are described in part 5 of this proposal.
We also request to receive the data from the remaining LWS detectors not used
to scan the [CII] line. These could give information about the spectrum of
the background to validate the calibration of the PHT-C spectrophotometry. In
the case of the very brightest galaxies this additional LWS data might
furthermore provide detailed information about the spectrum of the galaxy
itself - this would be used to validate the method adopted to distinguish dust
components of different temperatures from the PHT-C spectrophotometry.
<=== scientific_justification ===>
The sample of 118 galaxies for ISOPHOT was selected from the Virgo Cluster
Catalogue (VCC) of Bingelli et. al. (1985; AJ 1681), which is complete to
Bt = 18 magnitude. Only galaxies classified as cluster members in the updated
classification of Binggeli et al. (1993; preprint) were included. The sample
for the ISO observations consists of two subsamples. The cluster- core subsample
comprises of all 26 spiral VCC galaxies later than S0 having Bt < 14.5, and the
19 fainter late-type VCC galaxies having 14.5 <= Bt < 18 from the inner core of
VIRGO (within 2 degrees projected angle from M87), essentially from within the
"atmosphere" of M87. The cluster-periphery subsample comprises of all 73 spiral,
irregular and dwarf VCC galaxies later than S0 having Bt < 18 from the cluster
periphery (at least 4 degrees from the position of maximum galaxy surface
density), essentially equivalent to galaxies from the field. The periphery
subsample is roughly equally divided between dwarfs and irregulars on the one
hand, and giant spirals on the other, and should provide unbiased statistical
information on a variety of FIR properties, also at low luminosities. The two
subsamples will allow unbiased comparisons and contrasts between the infrared
activity and morphologies of cluster core galaxies and galaxies essentially
selected from the field. This should provide physical insight into the various
types of infrared phenomena discovered in the last decade, notably those related
to the star-formation activity. Correlations with physical processes manifest at
other wavelengths will enable the unfolding of the main evolutionary
characteristics of these phenomena.
Complementary observations in the CAM 5-8.5 and 12-17 micron bands of the 26
cluster core spirals and the entire cluster periphery sample of ISOPHOT are
being proposed by the ISOCAM consortium in a separate proposal. The SWS
consortium, also in a separate proposal, is proposing to spectrally scan the
remaining four giant spirals with Bt < 14.5 using LWS. Obviously, the superior
spatial resolution of CAM of about 6 arcseconds (corresponding to a few hundred
parsecs at the distance of the cluster) is sufficient to separate the core
region from the disk - at least as far as the warmer dust not covered by the
ISOPHOT FIR observations is concerned. Among other structural informations this
will place the best constraints on infrared emission powered, or triggered by
a discrete non-stellar source at the dynamical centres of galaxies, such as an
accreting super-massive object.
The [CII] cooling line will probe not only photodissociation regions associated
with massive star formation, but also the quiescent diffuse HI component of the
interstellar medium. The combination of [CII] line fluxes and the FIR continuum
with hydrogen recombination line fluxes, NIR continuum from old stellar
populations, HI, CO, as well as radio (synchrotron), UV and X-ray measurements
will provide detailed information on the structure and energy balance of the ISM
in disks of galaxies, as well as their current and past star-formation activity.
Table A: Summary of pointing directions, exposure times and rasters for each
galaxy observation in part 1 (for both spring and autumn launches):
-----------------------------------------------------------------------------
osn #vcc ra(1950) dec(1950) aot exposure times (s) at ny nz
60 70 100 120 160 200um
-----------------------------------------------------------------------------
1 26 12 8 7.2 14 55 30 PHT22 64 0 64 0 0 0 1 1
2 26 12 8 7.2 14 55 30 PHT32 0 0 0 0 16 0 3 1
3 4 12 5 57.6 15 22 30 PHT22 64 0 64 0 0 0 1 1
4 4 12 5 57.6 15 22 30 PHT32 0 0 0 0 16 0 3 1
5 1 12 5 46.8 13 57 42 PHT22 8 0 8 0 0 0 1 1
6 1 12 5 46.8 13 57 42 PHT32 0 0 0 0 16 0 3 1
7 17 12 7 28.8 14 38 24 PHT22 16 0 16 0 0 0 1 1
8 17 12 7 28.8 14 38 24 PHT32 0 0 0 0 16 0 3 1
9 81 12 10 53.4 15 3 0 PHT22 16 16 16 0 0 0 1 1
10 81 12 10 53.4 15 3 0 PHT32 0 0 0 16 16 16 3 1
11 87 12 11 7.8 15 43 54 PHT22 16 16 16 0 0 0 1 1
12 87 12 11 7.8 15 43 54 PHT32 0 0 0 16 16 16 3 1
19 92 12 11 15.6 15 10 48 PHT32 8 8 8 0 0 0 7 3
20 92 12 11 15.6 15 10 48 PHT32 0 0 0 8 8 8 8 2
21 24 12 8 3.0 12 2 18 PHT22 8 0 8 0 0 0 1 1
22 24 12 8 3.0 12 2 18 PHT32 0 0 0 0 16 0 3 1
29 66 12 10 13.8 11 8 48 PHT32 8 8 8 0 0 0 4 2
30 66 12 10 13.8 11 8 48 PHT32 0 0 0 8 8 8 5 1
31 171 12 13 25.8 8 39 6 PHT22 64 0 64 0 0 0 1 1
32 171 12 13 25.8 8 39 6 PHT32 0 0 0 0 16 0 3 1
33 159 12 13 8.4 8 33 48 PHT22 16 0 16 0 0 0 1 1
34 159 12 13 8.4 8 33 48 PHT32 0 0 0 0 16 0 3 1
35 207 12 14 15.0 8 19 42 PHT22 64 0 64 0 0 0 1 1
36 207 12 14 15.0 8 19 42 PHT32 0 0 0 0 16 0 3 1
37 425 12 18 3.0 8 28 48 PHT22 64 0 64 0 0 0 1 1
38 425 12 18 3.0 8 28 48 PHT32 0 0 0 0 16 0 3 1
39 318 12 16 30.0 9 8 6 PHT22 8 8 8 0 0 0 1 1
40 318 12 16 30.0 9 8 6 PHT32 0 0 0 8 8 16 3 1
41 169 12 13 23.4 9 55 36 PHT22 32 0 32 0 0 0 1 1
42 169 12 13 23.4 9 55 36 PHT32 0 0 0 0 16 0 3 1
43 130 12 12 31.2 10 1 54 PHT22 32 0 32 0 0 0 1 1
44 130 12 12 31.2 10 1 54 PHT32 0 0 0 0 16 0 3 1
45 152 12 12 58.2 9 51 48 PHT22 8 8 8 0 0 0 1 1
46 152 12 12 58.2 9 51 48 PHT32 0 0 0 8 8 8 3 1
59 666 12 21 14.4 17 4 6 PHT22 32 0 32 0 0 0 1 1
60 666 12 21 14.4 17 4 6 PHT32 0 0 0 0 16 0 3 1
61 1257 12 27 33.6 17 40 36 PHT22 32 0 32 0 0 0 1 1
62 1257 12 27 33.6 17 40 36 PHT32 0 0 0 0 16 0 3 1
63 857 12 23 24.6 18 29 24 PHT32 8 8 8 0 0 0 3 1
64 857 12 23 24.6 18 29 24 PHT32 0 0 0 8 8 8 4 1
65 655 12 21 6.0 17 49 6 PHT22 8 8 8 0 0 0 1 1
66 655 12 21 6.0 17 49 6 PHT32 0 0 0 8 8 16 3 1
67 459 12 18 39.6 17 54 54 PHT22 8 0 8 0 0 0 1 1
68 459 12 18 39.6 17 54 54 PHT32 0 0 0 0 16 0 3 1
69 460 12 18 41.4 18 39 42 PHT32 8 8 8 0 0 0 4 1
70 460 12 18 41.4 18 39 42 PHT32 0 0 0 8 8 8 5 1
71 1110 12 25 58.2 17 21 42 PHT32 8 8 8 0 0 0 4 2
72 1110 12 25 58.2 17 21 42 PHT32 0 0 0 8 8 8 6 1
73 1047 12 25 21.6 12 34 12 PHT22 8 8 8 0 0 0 1 1
74 1047 12 25 21.6 12 34 12 PHT32 0 0 0 8 8 16 3 1
75 1003 12 24 54.0 11 23 6 PHT32 8 8 8 0 0 0 6 2
76 1003 12 24 54.0 11 23 6 PHT32 0 0 0 8 8 8 7 2
77 1217 12 27 11.4 11 40 42 PHT22 8 8 8 0 0 0 1 1
78 1217 12 27 11.4 11 40 42 PHT32 0 0 0 8 8 16 3 1
79 692 12 21 29.4 12 28 54 PHT32 8 8 8 0 0 0 3 1
80 692 12 21 29.4 12 28 54 PHT32 0 0 0 8 8 8 3 1
81 664 12 21 12.0 12 45 18 PHT22 8 8 8 0 0 0 1 1
82 664 12 21 12.0 12 45 18 PHT32 0 0 0 8 8 16 3 1
83 836 12 23 13.8 12 56 18 PHT32 8 8 8 0 0 0 4 1
84 836 12 23 13.8 12 56 18 PHT32 0 0 0 8 8 8 5 1
85 912 12 24 0.0 12 53 18 PHT32 8 8 8 0 0 0 3 1
86 912 12 24 0.0 12 53 18 PHT32 0 0 0 8 8 8 3 1
87 984 12 24 42.0 13 0 42 PHT32 8 8 8 0 0 0 3 1
88 984 12 24 42.0 13 0 42 PHT32 0 0 0 8 8 16 3 1
89 1043 12 25 13.8 13 17 6 PHT32 8 8 8 0 0 0 6 2
90 1043 12 25 13.8 13 17 6 PHT32 0 0 0 8 8 8 7 2
91 873 12 23 34.8 13 23 24 PHT32 8 8 8 0 0 0 3 1
92 873 12 23 34.8 13 23 24 PHT32 0 0 0 8 8 8 4 1
-----------------------------------------------------------------------------
Table B: Time distribution for spring launch targets (full VIRGO proposal):
Team top 40% second 30% last 30%
PHT : 39302 17116 0
SOT : 24004 20276 0
total : 63306 37392 0
Table C: Time distribution for autumn launch targets (full VIRGO proposal):
Team top 40% second 30% last 30%
PHT : 39302 17116 0
SOT : 24004 20276 0
total : 63306 37392 0
<=== autumn_launch_targets ===>
1, "PHT22", 1.0, "N", "VCC0026", 12.13533, 14.92500, 1950, 0., 0., 584, 2
2, "PHT32", 1.0, "N", "VCC0026", 12.13533, 14.92500, 1950, 0., 0., 114, 3
3, "PHT22", 1.0, "N", "VCC0004", 12.09933, 15.37500, 1950, 0., 0., 424, 4
4, "PHT32", 1.0, "N", "VCC0004", 12.09933, 15.37500, 1950, 0., 0., 114, 5
5, "PHT22", 1.0, "N", "VCC0001", 12.09633, 13.96167, 1950, 0., 0., 200, 6
6, "PHT32", 1.0, "N", "VCC0001", 12.09633, 13.96167, 1950, 0., 0., 114, 7
7, "PHT22", 1.0, "N", "VCC0017", 12.12467, 14.64000, 1950, 0., 0., 232, 8
8, "PHT32", 1.0, "N", "VCC0017", 12.12467, 14.64000, 1950, 0., 0., 114, 9
9, "PHT22", 1.0, "N", "VCC0081", 12.18150, 15.05000, 1950, 0., 0., 271, 10
10, "PHT32", 1.0, "N", "VCC0081", 12.18150, 15.05000, 1950, 0., 0., 275, 11
11, "PHT22", 1.0, "N", "VCC0087", 12.18550, 15.73167, 1950, 0., 0., 271, 12
12, "PHT32", 1.0, "N", "VCC0087", 12.18550, 15.73167, 1950, 0., 0., 275, 13
13, "PHT25", 1.0, "N", "VBACK01", 12.18283, 15.79111, 1950, 0., 0., 160, 14
14, "PHT25", 1.0, "N", "VBACK01", 12.18283, 15.79111, 1950, 0., 0., 158, 15
15, "PHT25", 1.0, "N", "VBACK01", 12.18283, 15.79111, 1950, 0., 0., 156, 16
16, "PHT25", 1.0, "N", "VBACK01", 12.18283, 15.79111, 1950, 0., 0., 60, 17
17, "PHT25", 1.0, "N", "VBACK01", 12.18283, 15.79111, 1950, 0., 0., 48, 18
18, "PHT25", 1.0, "N", "VBACK01", 12.18283, 15.79111, 1950, 0., 0., 54, 19
19, "PHT32", 1.0, "N", "VCC0092", 12.18767, 15.18000, 1950, 0., 0.,1150, 20
20, "PHT32", 1.0, "N", "VCC0092", 12.18767, 15.18000, 1950, 0., 0., 812, 0
21, "PHT22", 1.0, "N", "VCC0024", 12.13417, 12.03833, 1950, 0., 0., 360, 22
22, "PHT32", 1.0, "N", "VCC0024", 12.13417, 12.03833, 1950, 0., 0., 114, 23
23, "PHT25", 1.0, "N", "VBACK02", 12.11408, 12.09389, 1950, 0., 0., 160, 24
24, "PHT25", 1.0, "N", "VBACK02", 12.11408, 12.09389, 1950, 0., 0., 158, 25
25, "PHT25", 1.0, "N", "VBACK02", 12.11408, 12.09389, 1950, 0., 0., 156, 26
26, "PHT25", 1.0, "N", "VBACK02", 12.11408, 12.09389, 1950, 0., 0., 60, 27
27, "PHT25", 1.0, "N", "VBACK02", 12.11408, 12.09389, 1950, 0., 0., 48, 28
28, "PHT25", 1.0, "N", "VBACK02", 12.11408, 12.09389, 1950, 0., 0., 54, 29
29, "PHT32", 1.0, "N", "VCC0066", 12.17050, 11.14667, 1950, 0., 0., 541, 30
30, "PHT32", 1.0, "N", "VCC0066", 12.17050, 11.14667, 1950, 0., 0., 297, 0
31, "PHT22", 1.0, "N", "VCC0171", 12.22383, 8.65167, 1950, 0., 0., 584, 32
32, "PHT32", 1.0, "N", "VCC0171", 12.22383, 8.65167, 1950, 0., 0., 114, 33
33, "PHT22", 1.0, "N", "VCC0159", 12.21900, 8.56333, 1950, 0., 0., 232, 34
34, "PHT32", 1.0, "N", "VCC0159", 12.21900, 8.56333, 1950, 0., 0., 114, 35
35, "PHT22", 1.0, "N", "VCC0207", 12.23750, 8.32833, 1950, 0., 0., 424, 36
36, "PHT32", 1.0, "N", "VCC0207", 12.23750, 8.32833, 1950, 0., 0., 114, 37
37, "PHT22", 1.0, "N", "VCC0425", 12.30083, 8.48000, 1950, 0., 0., 424, 38
38, "PHT32", 1.0, "N", "VCC0425", 12.30083, 8.48000, 1950, 0., 0., 114, 39
39, "PHT22", 1.0, "N", "VCC0318", 12.27500, 9.13500, 1950, 0., 0., 223, 40
40, "PHT32", 1.0, "N", "VCC0318", 12.27500, 9.13500, 1950, 0., 0., 227, 41
41, "PHT22", 1.0, "N", "VCC0169", 12.22317, 9.92667, 1950, 0., 0., 296, 42
42, "PHT32", 1.0, "N", "VCC0169", 12.22317, 9.92667, 1950, 0., 0., 114, 43
43, "PHT22", 1.0, "N", "VCC0130", 12.20867, 10.03167, 1950, 0., 0., 296, 44
44, "PHT32", 1.0, "N", "VCC0130", 12.20867, 10.03167, 1950, 0., 0., 114, 45
45, "PHT22", 1.0, "N", "VCC0152", 12.21617, 9.86333, 1950, 0., 0., 223, 46
46, "PHT32", 1.0, "N", "VCC0152", 12.21617, 9.86333, 1950, 0., 0., 203, 47
47, "PHT25", 1.0, "N", "VBACK03", 12.18869, 8.76472, 1950, 0., 0., 160, 48
48, "PHT25", 1.0, "N", "VBACK03", 12.18869, 8.76472, 1950, 0., 0., 158, 49
49, "PHT25", 1.0, "N", "VBACK03", 12.18869, 8.76472, 1950, 0., 0., 156, 50
50, "PHT25", 1.0, "N", "VBACK03", 12.18869, 8.76472, 1950, 0., 0., 60, 51
51, "PHT25", 1.0, "N", "VBACK03", 12.18869, 8.76472, 1950, 0., 0., 48, 52
52, "PHT25", 1.0, "N", "VBACK03", 12.18869, 8.76472, 1950, 0., 0., 54, 0
53, "PHT25", 1.0, "N", "VBACK04", 12.37622, 18.00805, 1950, 0., 0., 320, 54
54, "PHT25", 1.0, "N", "VBACK04", 12.37622, 18.00805, 1950, 0., 0., 158, 55
55, "PHT25", 1.0, "N", "VBACK04", 12.37622, 18.00805, 1950, 0., 0., 156, 56
56, "PHT25", 1.0, "N", "VBACK04", 12.37622, 18.00805, 1950, 0., 0., 60, 57
57, "PHT25", 1.0, "N", "VBACK04", 12.37622, 18.00805, 1950, 0., 0., 48, 58
58, "PHT25", 1.0, "N", "VBACK04", 12.37622, 18.00805, 1950, 0., 0., 54, 59
59, "PHT22", 1.0, "N", "VCC0666", 12.35400, 17.06833, 1950, 0., 0., 296, 60
60, "PHT32", 1.0, "N", "VCC0666", 12.35400, 17.06833, 1950, 0., 0., 114, 61
61, "PHT22", 1.0, "N", "VCC1257", 12.45933, 17.67667, 1950, 0., 0., 296, 62
62, "PHT32", 1.0, "N", "VCC1257", 12.45933, 17.67667, 1950, 0., 0., 114, 63
63, "PHT32", 1.0, "N", "VCC0857", 12.39017, 18.49000, 1950, 0., 0., 307, 64
64, "PHT32", 1.0, "N", "VCC0857", 12.39017, 18.49000, 1950, 0., 0., 250, 65
65, "PHT22", 1.0, "N", "VCC0655", 12.35167, 17.81833, 1950, 0., 0., 223, 66
66, "PHT32", 1.0, "N", "VCC0655", 12.35167, 17.81833, 1950, 0., 0., 227, 67
67, "PHT22", 1.0, "N", "VCC0459", 12.31100, 17.91500, 1950, 0., 0., 200, 68
68, "PHT32", 1.0, "N", "VCC0459", 12.31100, 17.91500, 1950, 0., 0., 114, 69
69, "PHT32", 1.0, "N", "VCC0460", 12.31150, 18.66167, 1950, 0., 0., 354, 70
70, "PHT32", 1.0, "N", "VCC0460", 12.31150, 18.66167, 1950, 0., 0., 297, 71
71, "PHT32", 1.0, "N", "VCC1110", 12.43283, 17.36167, 1950, 0., 0., 541, 72
72, "PHT32", 1.0, "N", "VCC1110", 12.43283, 17.36167, 1950, 0., 0., 344, 0
73, "PHT22", 1.0, "N", "VCC1047", 12.42267, 12.57000, 1950, 0., 0., 383, 74
74, "PHT32", 1.0, "N", "VCC1047", 12.42267, 12.57000, 1950, 0., 0., 227, 75
75, "PHT32", 1.0, "N", "VCC1003", 12.41500, 11.38500, 1950, 0., 0., 729, 76
76, "PHT32", 1.0, "N", "VCC1003", 12.41500, 11.38500, 1950, 0., 0., 718, 77
77, "PHT22", 1.0, "N", "VCC1217", 12.45317, 11.67833, 1950, 0., 0., 223, 78
78, "PHT32", 1.0, "N", "VCC1217", 12.45317, 11.67833, 1950, 0., 0., 227, 79
79, "PHT32", 1.0, "N", "VCC0692", 12.35817, 12.48167, 1950, 0., 0., 307, 80
80, "PHT32", 1.0, "N", "VCC0692", 12.35817, 12.48167, 1950, 0., 0., 203, 81
81, "PHT22", 1.0, "N", "VCC0664", 12.35333, 12.75500, 1950, 0., 0., 223, 82
82, "PHT32", 1.0, "N", "VCC0664", 12.35333, 12.75500, 1950, 0., 0., 227, 83
83, "PHT32", 1.0, "N", "VCC0836", 12.38717, 12.93833, 1950, 0., 0., 354, 84
84, "PHT32", 1.0, "N", "VCC0836", 12.38717, 12.93833, 1950, 0., 0., 297, 85
85, "PHT32", 1.0, "N", "VCC0912", 12.40000, 12.88833, 1950, 0., 0., 307, 86
86, "PHT32", 1.0, "N", "VCC0912", 12.40000, 12.88833, 1950, 0., 0., 203, 87
87, "PHT32", 1.0, "N", "VCC0984", 12.41167, 13.01167, 1950, 0., 0., 307, 88
88, "PHT32", 1.0, "N", "VCC0984", 12.41167, 13.01167, 1950, 0., 0., 227, 89
89, "PHT32", 1.0, "N", "VCC1043", 12.42050, 13.28500, 1950, 0., 0., 729, 90
90, "PHT32", 1.0, "N", "VCC1043", 12.42050, 13.28500, 1950, 0., 0., 718, 91
91, "PHT32", 1.0, "N", "VCC0873", 12.39300, 13.39000, 1950, 0., 0., 307, 92
92, "PHT32", 1.0, "N", "VCC0873", 12.39300, 13.39000, 1950, 0., 0., 250, 93
93, "PHT25", 1.0, "N", "VBACK05", 12.34903, 13.52778, 1950, 0., 0., 160, 94
94, "PHT25", 1.0, "N", "VBACK05", 12.34903, 13.52778, 1950, 0., 0., 158, 95
95, "PHT25", 1.0, "N", "VBACK05", 12.34903, 13.52778, 1950, 0., 0., 156, 96
96, "PHT25", 1.0, "N", "VBACK05", 12.34903, 13.52778, 1950, 0., 0., 60, 97
97, "PHT25", 1.0, "N", "VBACK05", 12.34903, 13.52778, 1950, 0., 0., 48, 98
98, "PHT25", 1.0, "N", "VBACK05", 12.34903, 13.52778, 1950, 0., 0., 54, 0
<=== spring_launch_targets ===>
1, "PHT22", 1.0, "N", "VCC0026", 12.13533, 14.92500, 1950, 0., 0., 584, 2
2, "PHT32", 1.0, "N", "VCC0026", 12.13533, 14.92500, 1950, 0., 0., 114, 3
3, "PHT22", 1.0, "N", "VCC0004", 12.09933, 15.37500, 1950, 0., 0., 424, 4
4, "PHT32", 1.0, "N", "VCC0004", 12.09933, 15.37500, 1950, 0., 0., 114, 5
5, "PHT22", 1.0, "N", "VCC0001", 12.09633, 13.96167, 1950, 0., 0., 200, 6
6, "PHT32", 1.0, "N", "VCC0001", 12.09633, 13.96167, 1950, 0., 0., 114, 7
7, "PHT22", 1.0, "N", "VCC0017", 12.12467, 14.64000, 1950, 0., 0., 232, 8
8, "PHT32", 1.0, "N", "VCC0017", 12.12467, 14.64000, 1950, 0., 0., 114, 9
9, "PHT22", 1.0, "N", "VCC0081", 12.18150, 15.05000, 1950, 0., 0., 271, 10
10, "PHT32", 1.0, "N", "VCC0081", 12.18150, 15.05000, 1950, 0., 0., 275, 11
11, "PHT22", 1.0, "N", "VCC0087", 12.18550, 15.73167, 1950, 0., 0., 271, 12
12, "PHT32", 1.0, "N", "VCC0087", 12.18550, 15.73167, 1950, 0., 0., 275, 13
13, "PHT25", 1.0, "N", "VBACK01", 12.18283, 15.79111, 1950, 0., 0., 160, 14
14, "PHT25", 1.0, "N", "VBACK01", 12.18283, 15.79111, 1950, 0., 0., 158, 15
15, "PHT25", 1.0, "N", "VBACK01", 12.18283, 15.79111, 1950, 0., 0., 156, 16
16, "PHT25", 1.0, "N", "VBACK01", 12.18283, 15.79111, 1950, 0., 0., 60, 17
17, "PHT25", 1.0, "N", "VBACK01", 12.18283, 15.79111, 1950, 0., 0., 48, 18
18, "PHT25", 1.0, "N", "VBACK01", 12.18283, 15.79111, 1950, 0., 0., 54, 19
19, "PHT32", 1.0, "N", "VCC0092", 12.18767, 15.18000, 1950, 0., 0.,1150, 20
20, "PHT32", 1.0, "N", "VCC0092", 12.18767, 15.18000, 1950, 0., 0., 812, 0
21, "PHT22", 1.0, "N", "VCC0024", 12.13417, 12.03833, 1950, 0., 0., 360, 22
22, "PHT32", 1.0, "N", "VCC0024", 12.13417, 12.03833, 1950, 0., 0., 114, 23
23, "PHT25", 1.0, "N", "VBACK02", 12.11408, 12.09389, 1950, 0., 0., 160, 24
24, "PHT25", 1.0, "N", "VBACK02", 12.11408, 12.09389, 1950, 0., 0., 158, 25
25, "PHT25", 1.0, "N", "VBACK02", 12.11408, 12.09389, 1950, 0., 0., 156, 26
26, "PHT25", 1.0, "N", "VBACK02", 12.11408, 12.09389, 1950, 0., 0., 60, 27
27, "PHT25", 1.0, "N", "VBACK02", 12.11408, 12.09389, 1950, 0., 0., 48, 28
28, "PHT25", 1.0, "N", "VBACK02", 12.11408, 12.09389, 1950, 0., 0., 54, 29
29, "PHT32", 1.0, "N", "VCC0066", 12.17050, 11.14667, 1950, 0., 0., 541, 30
30, "PHT32", 1.0, "N", "VCC0066", 12.17050, 11.14667, 1950, 0., 0., 297, 0
31, "PHT22", 1.0, "N", "VCC0171", 12.22383, 8.65167, 1950, 0., 0., 584, 32
32, "PHT32", 1.0, "N", "VCC0171", 12.22383, 8.65167, 1950, 0., 0., 114, 33
33, "PHT22", 1.0, "N", "VCC0159", 12.21900, 8.56333, 1950, 0., 0., 232, 34
34, "PHT32", 1.0, "N", "VCC0159", 12.21900, 8.56333, 1950, 0., 0., 114, 35
35, "PHT22", 1.0, "N", "VCC0207", 12.23750, 8.32833, 1950, 0., 0., 424, 36
36, "PHT32", 1.0, "N", "VCC0207", 12.23750, 8.32833, 1950, 0., 0., 114, 37
37, "PHT22", 1.0, "N", "VCC0425", 12.30083, 8.48000, 1950, 0., 0., 424, 38
38, "PHT32", 1.0, "N", "VCC0425", 12.30083, 8.48000, 1950, 0., 0., 114, 39
39, "PHT22", 1.0, "N", "VCC0318", 12.27500, 9.13500, 1950, 0., 0., 223, 40
40, "PHT32", 1.0, "N", "VCC0318", 12.27500, 9.13500, 1950, 0., 0., 227, 41
41, "PHT22", 1.0, "N", "VCC0169", 12.22317, 9.92667, 1950, 0., 0., 296, 42
42, "PHT32", 1.0, "N", "VCC0169", 12.22317, 9.92667, 1950, 0., 0., 114, 43
43, "PHT22", 1.0, "N", "VCC0130", 12.20867, 10.03167, 1950, 0., 0., 296, 44
44, "PHT32", 1.0, "N", "VCC0130", 12.20867, 10.03167, 1950, 0., 0., 114, 45
45, "PHT22", 1.0, "N", "VCC0152", 12.21617, 9.86333, 1950, 0., 0., 223, 46
46, "PHT32", 1.0, "N", "VCC0152", 12.21617, 9.86333, 1950, 0., 0., 203, 47
47, "PHT25", 1.0, "N", "VBACK03", 12.18869, 8.76472, 1950, 0., 0., 160, 48
48, "PHT25", 1.0, "N", "VBACK03", 12.18869, 8.76472, 1950, 0., 0., 158, 49
49, "PHT25", 1.0, "N", "VBACK03", 12.18869, 8.76472, 1950, 0., 0., 156, 50
50, "PHT25", 1.0, "N", "VBACK03", 12.18869, 8.76472, 1950, 0., 0., 60, 51
51, "PHT25", 1.0, "N", "VBACK03", 12.18869, 8.76472, 1950, 0., 0., 48, 52
52, "PHT25", 1.0, "N", "VBACK03", 12.18869, 8.76472, 1950, 0., 0., 54, 0
53, "PHT25", 1.0, "N", "VBACK04", 12.37622, 18.00805, 1950, 0., 0., 320, 54
54, "PHT25", 1.0, "N", "VBACK04", 12.37622, 18.00805, 1950, 0., 0., 158, 55
55, "PHT25", 1.0, "N", "VBACK04", 12.37622, 18.00805, 1950, 0., 0., 156, 56
56, "PHT25", 1.0, "N", "VBACK04", 12.37622, 18.00805, 1950, 0., 0., 60, 57
57, "PHT25", 1.0, "N", "VBACK04", 12.37622, 18.00805, 1950, 0., 0., 48, 58
58, "PHT25", 1.0, "N", "VBACK04", 12.37622, 18.00805, 1950, 0., 0., 54, 59
59, "PHT22", 1.0, "N", "VCC0666", 12.35400, 17.06833, 1950, 0., 0., 296, 60
60, "PHT32", 1.0, "N", "VCC0666", 12.35400, 17.06833, 1950, 0., 0., 114, 61
61, "PHT22", 1.0, "N", "VCC1257", 12.45933, 17.67667, 1950, 0., 0., 296, 62
62, "PHT32", 1.0, "N", "VCC1257", 12.45933, 17.67667, 1950, 0., 0., 114, 63
63, "PHT32", 1.0, "N", "VCC0857", 12.39017, 18.49000, 1950, 0., 0., 307, 64
64, "PHT32", 1.0, "N", "VCC0857", 12.39017, 18.49000, 1950, 0., 0., 250, 65
65, "PHT22", 1.0, "N", "VCC0655", 12.35167, 17.81833, 1950, 0., 0., 223, 66
66, "PHT32", 1.0, "N", "VCC0655", 12.35167, 17.81833, 1950, 0., 0., 227, 67
67, "PHT22", 1.0, "N", "VCC0459", 12.31100, 17.91500, 1950, 0., 0., 200, 68
68, "PHT32", 1.0, "N", "VCC0459", 12.31100, 17.91500, 1950, 0., 0., 114, 69
69, "PHT32", 1.0, "N", "VCC0460", 12.31150, 18.66167, 1950, 0., 0., 354, 70
70, "PHT32", 1.0, "N", "VCC0460", 12.31150, 18.66167, 1950, 0., 0., 297, 71
71, "PHT32", 1.0, "N", "VCC1110", 12.43283, 17.36167, 1950, 0., 0., 541, 72
72, "PHT32", 1.0, "N", "VCC1110", 12.43283, 17.36167, 1950, 0., 0., 344, 0
73, "PHT22", 1.0, "N", "VCC1047", 12.42267, 12.57000, 1950, 0., 0., 383, 74
74, "PHT32", 1.0, "N", "VCC1047", 12.42267, 12.57000, 1950, 0., 0., 227, 75
75, "PHT32", 1.0, "N", "VCC1003", 12.41500, 11.38500, 1950, 0., 0., 729, 76
76, "PHT32", 1.0, "N", "VCC1003", 12.41500, 11.38500, 1950, 0., 0., 718, 77
77, "PHT22", 1.0, "N", "VCC1217", 12.45317, 11.67833, 1950, 0., 0., 223, 78
78, "PHT32", 1.0, "N", "VCC1217", 12.45317, 11.67833, 1950, 0., 0., 227, 79
79, "PHT32", 1.0, "N", "VCC0692", 12.35817, 12.48167, 1950, 0., 0., 307, 80
80, "PHT32", 1.0, "N", "VCC0692", 12.35817, 12.48167, 1950, 0., 0., 203, 81
81, "PHT22", 1.0, "N", "VCC0664", 12.35333, 12.75500, 1950, 0., 0., 223, 82
82, "PHT32", 1.0, "N", "VCC0664", 12.35333, 12.75500, 1950, 0., 0., 227, 83
83, "PHT32", 1.0, "N", "VCC0836", 12.38717, 12.93833, 1950, 0., 0., 354, 84
84, "PHT32", 1.0, "N", "VCC0836", 12.38717, 12.93833, 1950, 0., 0., 297, 85
85, "PHT32", 1.0, "N", "VCC0912", 12.40000, 12.88833, 1950, 0., 0., 307, 86
86, "PHT32", 1.0, "N", "VCC0912", 12.40000, 12.88833, 1950, 0., 0., 203, 87
87, "PHT32", 1.0, "N", "VCC0984", 12.41167, 13.01167, 1950, 0., 0., 307, 88
88, "PHT32", 1.0, "N", "VCC0984", 12.41167, 13.01167, 1950, 0., 0., 227, 89
89, "PHT32", 1.0, "N", "VCC1043", 12.42050, 13.28500, 1950, 0., 0., 729, 90
90, "PHT32", 1.0, "N", "VCC1043", 12.42050, 13.28500, 1950, 0., 0., 718, 91
91, "PHT32", 1.0, "N", "VCC0873", 12.39300, 13.39000, 1950, 0., 0., 307, 92
92, "PHT32", 1.0, "N", "VCC0873", 12.39300, 13.39000, 1950, 0., 0., 250, 93
93, "PHT25", 1.0, "N", "VBACK05", 12.34903, 13.52778, 1950, 0., 0., 160, 94
94, "PHT25", 1.0, "N", "VBACK05", 12.34903, 13.52778, 1950, 0., 0., 158, 95
95, "PHT25", 1.0, "N", "VBACK05", 12.34903, 13.52778, 1950, 0., 0., 156, 96
96, "PHT25", 1.0, "N", "VBACK05", 12.34903, 13.52778, 1950, 0., 0., 60, 97
97, "PHT25", 1.0, "N", "VBACK05", 12.34903, 13.52778, 1950, 0., 0., 48, 98
98, "PHT25", 1.0, "N", "VBACK05", 12.34903, 13.52778, 1950, 0., 0., 54, 0