<=== observer ===>
"CTELESCO",\
"Telesco, C. M.",\
"Space Science Laboratory",\
"NASA Marshall Space Flight Center",\
"",\
"Mail Code ES-63",\
"",\
"Huntsville AL 35812",\
"USA",\
"0010205 5447723",\
"0010205 5447754",\
"telesco@ssl.msfc.nasa.gov"

<=== proposal ===>
"HI_Z_PT2",1,4,\
{"starburst galaxies","galaxy formation","irregular galaxies"},\
{"U. Klaas","A. Moorwood","H. Hippelein"}

<=== title ===>
Blue Radio Galaxies at Intermediate Redshifts:
Part 2

<=== abstract ===>
SCIENTIFIC ABSTRACT
We propose to use ISOPHOT at 24, 64, and 100 um and ISOCAM at 15 um to study
galaxies at z > 0.1 which, based on their blue colors, are thought to be
undergoing bursts of star formation.  Most of these galaxies were discovered
as radio sources in the deep 1.4 GHz surveys.  Many have complex optical
morphologies suggesting that they are interacting and merging systems,
although other explanations such as jet-induced star formation have been put
forward.  These galaxies are thought to account for the excess, or "upturn,"
in the 1.4 GHz radio source counts detected at flux densities below a few
milliJanskys.  Our study will show if there exist significant obscured
populations of young stars in these galaxies, and it will substantially extend
our knowledge of the population of IR-luminous galaxies to the realm at z >
0.1 and possibly out to z = 1-2.  The total luminosities and dust color
temperatures will be determined from the fluxes at 64 and 100 um, where the
spectral energy distributions peak.  The 15, 24, and 64 um fluxes may indicate
the presence of active nuclei which produce a peak in this spectral region in
several local Seyfert archetypes.

OBSERVATION SUMMARY
We propose to observe 51 galaxies for an Autumn launch (exclusion hole in
Orion) or 58 galaxies for a Spring launch (exclusion hole in the Galactic
Center), most at 24, 64, and 100 um with PHOT and at 15 um with CAM, for a
total spacecraft time of 17 hours.  Five hours of this spacecraft time have
been contributed by Mission Scientist Alan Moorwood.  Most of the sources have
1.4 GHz flux densities of a few mJy, with expected 60 um flux densities of
greater than 100 mJy if the radio-infrared relation for local galaxies applies
to these distant ones.  Each of these brighter galaxies will be observed using
PHT filters C100, C60, and P25 and CAM filter LW3.  A smaller sample of
fainter galaxies, with expected 60 um flux densities greater than 30 mJy will
be observed only with C100, C60, and LW3.  The PHOT observations will employ
triangular chopping, and the CAM imaging will use 2x2 microscans.  Because
these galaxies are grouped in several small regions of the sky, we propose to
use concatenation to substantially reduce overhead.  In addition to the purely
scientific reasons mentioned in the abstract, the CAM images will verify
telescope pointing and aid in the assessment of cirrus contamination at the
longer wavelengths.

<=== scientific_justification ===>
Time table includes times of part 1 and 2!

Time distribution for autumn launch targets

		Team	top 40%		second 30%	last 30%
        	PHT : 	14534		15805		15316
		AFM :	10800		0		 7200
              total :   25334           15805           22516


Time distribution for spring launch targets

                PHT :	15435		20294		 9771
		AFM :	10800		0		 7200
              total :   26235           20294           16971


For a detailed scientific justification, please see part 1 of proposal
Astronomers are striving to formulate a comprehensive description of the
evolution of galaxies.  A key element of this quest is the search for, and
detailed study of, galaxies at great distances.  By examining galaxies as a
function of redshift, and hence lookback time, we should be able to piece
together the scenario that has led to the currently observed Universe.  The
actual discovery of distant galaxies (i.e., those at z > 0.1) is difficult and
challenging.  Deep surveys at radio wavelengths followed by visual imaging and
spectroscopy of the radio sources has proven to be very effective for finding
distant galaxies.  With this approach, galaxies have been discovered at z > 2.
Many of these radio galaxies appear to be giant ellipticals undergoing
"passive" stellar evolution, defined as the normal aging of the previously
formed dominant stellar population (Lilly and Longair 1984; Kron, Koo, and
Wi

<=== autumn_launch_targets ===>
1, "PHT22", 2.0, "N", "54W008", 0.22122, 15.81175, 1950, 0., 0., 817, 2
2, "PHT03", 2.0, "N", "54W008", 0.22122, 15.81175, 1950, 0., 0., 238, 3
3, "CAM01", 2.0, "N", "54W008", 0.22122, 15.81175, 1950, 0., 0., 148, 4
4, "PHT22", 2.0, "N", "54W013", 0.22771, 16.19128, 1950, 0., 0., 657, 5
5, "PHT03", 2.0, "N", "54W013", 0.22771, 16.19128, 1950, 0., 0., 238, 6
6, "CAM01", 2.0, "N", "54W013", 0.22771, 16.19128, 1950, 0., 0., 148, 7
7, "PHT22", 2.0, "N", "54W018", 0.23051, 15.89178, 1950, 0., 0., 657, 8
8, "PHT03", 2.0, "N", "54W018", 0.23051, 15.89178, 1950, 0., 0., 238, 9
9, "CAM01", 2.0, "N", "54W018", 0.23051, 15.89178, 1950, 0., 0., 148, 10
10, "PHT22", 2.0, "N", "54W034", 0.23906, 16.11814, 1950, 0., 0., 657, 11
11, "PHT03", 2.0, "N", "54W034", 0.23906, 16.11814, 1950, 0., 0., 238, 12
12, "CAM01", 2.0, "N", "54W034", 0.23906, 16.11814, 1950, 0., 0., 148, 13
13, "PHT22", 2.0, "N", "54W036", 0.24060, 15.38153, 1950, 0., 0., 657, 14
14, "PHT03", 2.0, "N", "54W036", 0.24060, 15.38153, 1950, 0., 0., 238, 15
15, "CAM01", 2.0, "N", "54W036", 0.24060, 15.38153, 1950, 0., 0., 148, 16
16, "PHT22", 2.0, "N", "54W050", 0.25009, 15.21328, 1950, 0., 0., 657, 17
17, "PHT03", 2.0, "N", "54W050", 0.25009, 15.21328, 1950, 0., 0., 238, 18
18, "CAM01", 2.0, "N", "54W050", 0.25009, 15.21328, 1950, 0., 0., 148, 19
19, "PHT22", 2.0, "N", "54W052", 0.25159, 15.90731, 1950, 0., 0., 657, 20
20, "PHT03", 2.0, "N", "54W052", 0.25159, 15.90731, 1950, 0., 0., 238, 21
21, "CAM01", 2.0, "N", "54W052", 0.25159, 15.90731, 1950, 0., 0., 148, 22
22, "PHT22", 2.0, "N", "54W053", 0.25170, 15.51550, 1950, 0., 0., 657, 23
23, "PHT03", 2.0, "N", "54W053", 0.25170, 15.51550, 1950, 0., 0., 238, 24
24, "CAM01", 2.0, "N", "54W053", 0.25170, 15.51550, 1950, 0., 0., 148, 0
25, "PHT22", 2.0, "N", "54W057", 0.25264, 16.57689, 1950, 0., 0., 817, 26
26, "PHT03", 2.0, "N", "54W057", 0.25264, 16.57689, 1950, 0., 0., 238, 27
27, "CAM01", 2.0, "N", "54W057", 0.25264, 16.57689, 1950, 0., 0., 148, 28
28, "PHT22", 2.0, "N", "54W065", 0.25881, 16.32111, 1950, 0., 0., 657, 29
29, "PHT03", 2.0, "N", "54W065", 0.25881, 16.32111, 1950, 0., 0., 238, 30
30, "CAM01", 2.0, "N", "54W065", 0.25881, 16.32111, 1950, 0., 0., 148, 31
31, "PHT22", 2.0, "N", "54W067", 0.25970, 16.34797, 1950, 0., 0., 657, 32
32, "PHT03", 2.0, "N", "54W067", 0.25970, 16.34797, 1950, 0., 0., 238, 33
33, "CAM01", 2.0, "N", "54W067", 0.25970, 16.34797, 1950, 0., 0., 148, 34
34, "PHT22", 2.0, "N", "54W068", 0.25973, 16.54797, 1950, 0., 0., 657, 35
35, "PHT03", 2.0, "N", "54W068", 0.25973, 16.54797, 1950, 0., 0., 238, 36
36, "CAM01", 2.0, "N", "54W068", 0.25973, 16.54797, 1950, 0., 0., 148, 37
37, "PHT22", 2.0, "N", "54W071", 0.26157, 16.49361, 1950, 0., 0., 657, 38
38, "PHT03", 2.0, "N", "54W071", 0.26157, 16.49361, 1950, 0., 0., 238, 39
39, "CAM01", 2.0, "N", "54W071", 0.26157, 16.49361, 1950, 0., 0., 148, 40
40, "PHT22", 2.0, "N", "54W072", 0.26175, 16.44586, 1950, 0., 0., 657, 41
41, "PHT03", 2.0, "N", "54W072", 0.26175, 16.44586, 1950, 0., 0., 238, 42
42, "CAM01", 2.0, "N", "54W072", 0.26175, 16.44586, 1950, 0., 0., 148, 43
43, "PHT22", 2.0, "N", "54W081", 0.26719, 15.69742, 1950, 0., 0., 657, 44
44, "PHT03", 2.0, "N", "54W081", 0.26719, 15.69742, 1950, 0., 0., 238, 45
45, "CAM01", 2.0, "N", "54W081", 0.26719, 15.69742, 1950, 0., 0., 148, 0

<=== spring_launch_targets ===>
1, "PHT22", 2.0, "N", "54W008", 0.22122, 15.81175, 1950, 0., 0., 817, 2
2, "PHT03", 2.0, "N", "54W008", 0.22122, 15.81175, 1950, 0., 0., 238, 3
3, "CAM01", 2.0, "N", "54W008", 0.22122, 15.81175, 1950, 0., 0., 148, 4
4, "PHT22", 2.0, "N", "54W013", 0.22771, 16.19128, 1950, 0., 0., 657, 5
5, "PHT03", 2.0, "N", "54W013", 0.22771, 16.19128, 1950, 0., 0., 238, 6
6, "CAM01", 2.0, "N", "54W013", 0.22771, 16.19128, 1950, 0., 0., 148, 7
7, "PHT22", 2.0, "N", "54W018", 0.23051, 15.89178, 1950, 0., 0., 657, 8
8, "PHT03", 2.0, "N", "54W018", 0.23051, 15.89178, 1950, 0., 0., 238, 9
9, "CAM01", 2.0, "N", "54W018", 0.23051, 15.89178, 1950, 0., 0., 148, 10
10, "PHT22", 2.0, "N", "54W034", 0.23906, 16.11814, 1950, 0., 0., 657, 11
11, "PHT03", 2.0, "N", "54W034", 0.23906, 16.11814, 1950, 0., 0., 238, 12
12, "CAM01", 2.0, "N", "54W034", 0.23906, 16.11814, 1950, 0., 0., 148, 13
13, "PHT22", 2.0, "N", "54W036", 0.24060, 15.38153, 1950, 0., 0., 657, 14
14, "PHT03", 2.0, "N", "54W036", 0.24060, 15.38153, 1950, 0., 0., 238, 15
15, "CAM01", 2.0, "N", "54W036", 0.24060, 15.38153, 1950, 0., 0., 148, 16
16, "PHT22", 2.0, "N", "54W050", 0.25009, 15.21328, 1950, 0., 0., 657, 17
17, "PHT03", 2.0, "N", "54W050", 0.25009, 15.21328, 1950, 0., 0., 238, 18
18, "CAM01", 2.0, "N", "54W050", 0.25009, 15.21328, 1950, 0., 0., 148, 19
19, "PHT22", 2.0, "N", "54W052", 0.25159, 15.90731, 1950, 0., 0., 657, 20
20, "PHT03", 2.0, "N", "54W052", 0.25159, 15.90731, 1950, 0., 0., 238, 21
21, "CAM01", 2.0, "N", "54W052", 0.25159, 15.90731, 1950, 0., 0., 148, 22
22, "PHT22", 2.0, "N", "54W053", 0.25170, 15.51550, 1950, 0., 0., 657, 23
23, "PHT03", 2.0, "N", "54W053", 0.25170, 15.51550, 1950, 0., 0., 238, 24
24, "CAM01", 2.0, "N", "54W053", 0.25170, 15.51550, 1950, 0., 0., 148, 0
25, "PHT22", 2.0, "N", "54W057", 0.25264, 16.57689, 1950, 0., 0., 657, 26
26, "PHT03", 2.0, "N", "54W057", 0.25264, 16.57689, 1950, 0., 0., 238, 27
27, "CAM01", 2.0, "N", "54W057", 0.25264, 16.57689, 1950, 0., 0., 148, 28
28, "PHT22", 3.0, "N", "54W065", 0.25881, 16.32111, 1950, 0., 0., 817, 29
29, "PHT03", 3.0, "N", "54W065", 0.25881, 16.32111, 1950, 0., 0., 238, 30
30, "CAM01", 3.0, "N", "54W065", 0.25881, 16.32111, 1950, 0., 0., 148, 31
31, "PHT22", 3.0, "N", "54W067", 0.25970, 16.34797, 1950, 0., 0., 657, 32
32, "PHT03", 3.0, "N", "54W067", 0.25970, 16.34797, 1950, 0., 0., 238, 33
33, "CAM01", 3.0, "N", "54W067", 0.25970, 16.34797, 1950, 0., 0., 148, 34
34, "PHT22", 3.0, "N", "54W068", 0.25973, 16.54797, 1950, 0., 0., 657, 35
35, "PHT03", 3.0, "N", "54W068", 0.25973, 16.54797, 1950, 0., 0., 238, 36
36, "CAM01", 3.0, "N", "54W068", 0.25973, 16.54797, 1950, 0., 0., 148, 37
37, "PHT22", 3.0, "N", "54W071", 0.26157, 16.49361, 1950, 0., 0., 657, 38
38, "PHT03", 3.0, "N", "54W071", 0.26157, 16.49361, 1950, 0., 0., 238, 39
39, "CAM01", 3.0, "N", "54W071", 0.26157, 16.49361, 1950, 0., 0., 148, 40
40, "PHT22", 3.0, "N", "54W072", 0.26175, 16.44586, 1950, 0., 0., 657, 41
41, "PHT03", 3.0, "N", "54W072", 0.26175, 16.44586, 1950, 0., 0., 238, 42
42, "CAM01", 3.0, "N", "54W072", 0.26175, 16.44586, 1950, 0., 0., 148, 43
43, "PHT22", 3.0, "N", "54W081", 0.26719, 15.69742, 1950, 0., 0., 657, 44
44, "PHT03", 3.0, "N", "54W081", 0.26719, 15.69742, 1950, 0., 0., 238, 45
45, "CAM01", 3.0, "N", "54W081", 0.26719, 15.69742, 1950, 0., 0., 148, 0
46, "PHT22", 1.0, "N", "55W226", 8.79326, 44.57786, 1950, 0., 0., 817, 47
47, "PHT03", 1.0, "N", "55W226", 8.79326, 44.57786, 1950, 0., 0., 238, 48
48, "CAM01", 1.0, "N", "55W226", 8.79326, 44.57786, 1950, 0., 0., 148, 0
49, "PHT22", 3.0, "N", "44.03", 8.66533, 44.72433, 1950, 0., 0., 1329, 50
50, "CAM01", 3.0, "N", "44.03", 8.66533, 44.72433, 1950, 0., 0., 148, 51
51, "PHT22", 3.0, "N", "44.02", 8.66916, 44.95783, 1950, 0., 0., 1169, 52
52, "CAM01", 3.0, "N", "44.02", 8.66916, 44.95783, 1950, 0., 0., 148, 53
53, "PHT22", 3.0, "N", "45.02", 8.67787, 45.00769, 1950, 0., 0., 1169, 54
54, "CAM01", 3.0, "N", "45.02", 8.67787, 45.00769, 1950, 0., 0., 148, 55
55, "PHT22", 3.0, "N", "44.10", 8.68639, 44.99817, 1950, 0., 0., 1169, 56
56, "CAM01", 3.0, "N", "44.10", 8.68639, 44.99817, 1950, 0., 0., 148, 57
57, "PHT22", 3.0, "N", "44.15", 8.68846, 44.94089, 1950, 0., 0., 1169, 58
58, "CAM01", 3.0, "N", "44.15", 8.68846, 44.94089, 1950, 0., 0., 148, 59
59, "PHT22", 3.0, "N", "44.28", 8.69483, 44.86706, 1950, 0., 0., 1329, 60
60, "CAM01", 3.0, "N", "44.28", 8.69483, 44.86706, 1950, 0., 0., 148, 61
61, "PHT22", 3.0, "N", "45.03", 8.69712, 45.06778, 1950, 0., 0., 1169, 62
62, "CAM01", 3.0, "N", "45.03", 8.69712, 45.06778, 1950, 0., 0., 148, 63
63, "PHT22", 3.0, "N", "44.12", 8.71103, 44.66889, 1950, 0., 0., 1169, 64
64, "CAM01", 3.0, "N", "44.12", 8.71103, 44.66889, 1950, 0., 0., 148, 65
65, "PHT22", 3.0, "N", "44.07", 8.72123, 44.74611, 1950, 0., 0., 1169, 66
66, "CAM01", 3.0, "N", "44.07", 8.72123, 44.74611, 1950, 0., 0., 148, 0