<=== observer ===>
"LVIGROUX",\
"Vigroux, L.",\
"Service d'Astrophysique, DAPNIA",\
"C. E. Saclay",\
"Orme des Merisiers",\
"",\
"91191",\
"Gif-sur-Yvette CEDEX",\
"France",\
" 33169083912",\
" 33169086577",\
"vigroux@sapvxg.saclay.cea.fr"
<=== proposal ===>
"CAMSPIR",\
1,\
4,\
{"normal galaxies","Magellanic Clouds","compact galaxies","dust properties",\
"HII regions"},\
{"C.Bonoli","F.Boulanger","J.Lequeux","M.Sauvage",\
"F.Viallefond","A.Bosma","D.Cesarsky"}
<=== title ===>
Broad band Imaging of an extragalactic HII region sample .
<=== abstract ===>
SCIENTIFIC ABSTRACT:
We propose a coherent program to study HII regions in
selected normal (non-interacting, non-starburst, non-AGN) galaxies in the
near- to far-IR in coordination with the ISOPHOT, the LWS and the SOT
consortia. The present part of the proposal consists in imaging all the
targets in two filters: LW 2 (5.0-8.5 micrometers) and LW 3 (12-18
micrometers). Emission in LW 2 will be dominated by IR emission bands and
emission in LW 3 by hot dust. The nature and physics of both components
are not well understood, and the IRAS 12 micrometer filter did not allow
a clear separation between them. However IRAS and other observations have shown
that the intensity of the IR bands and to some extent of hot dust (with
respect to colder dust) are affected by the UV radiation field and by
metallicity, and also that the IR band carrier(s) (PAHs or related large
molecules) are easily frozen on bigger grains or liberated from them. The
planned observations will allow a much better understanding of these
phenomena. Together with the other coordinated ISO observations and
complementary ground-based observations they will yield a more complete picture
of the physics of dust and possibly a full understanding of the thermal
balance of dust and gas in galaxies. The chosen targets span a large range
of properties and of distances, starting from the Magellanic Clouds where
very detailed studies will be possible and including more distant galaxies.
OBSERVATION SUMMARY
The observations combine the beam switching mode between the central region and
a reference point, far away from the galaxy, and a raster map with some
overlap between successive images. Filters LW2 and LW3 are used in every
case. The integration time is 2 sec. The expected sensitivity is a S/N ratio =
3 at the limit of the IRAS maps of extended galaxies.
<=== scientific_justification ===>
Time distribution for autumn launch targets:
team top 40% second 30% last 30%
CAM: 10000 19600 51400
Total: 10000 19600 51400
Time distribution for spring launch targets:
team top 40% second 30% last 30%
CAM: 10000 19200 51400
Total: 10000 19200 51400
<=== autumn_launch_targets ===>
1, "CAM03", 3.0, "N", "M31 REF", 00.70014, 41.18381, 1950, 0., 0., 900, 0
2, "CAM03", 3.0, "N", "M31 D478", 00.67278, 41.12667, 1950, 0., 0., 900, 0
3, "CAM03", 3.0, "N", "M31 D268", 00.65750, 40.84972, 1950, 0., 0., 900, 0
4, "CAM03", 3.0, "N", "M31 D192", 00.65208, 40.51250, 1950, 0., 0., 900, 0
5, "CAM03", 3.0, "N", "M31 D395", 00.66644, 41.01611, 1950, 0., 0., 900, 0
6, "CAM03", 3.0, "N", "M31 D535", 00.68111, 41.13694, 1950, 0., 0., 900, 0
7, "CAM03", 3.0, "N", "M31 D478S",00.67250, 41.10000, 1950, 0., 0., 900, 0
8, "CAM03", 3.0, "N", "M31 D307", 00.63892, 40.92889, 1950, 0., 0., 900, 0
9, "CAM03", 3.0, "N", "M31 D321", 00.66111, 40.81944, 1950, 0., 0., 900, 0
10,"CAM01", 3.0, "N", "SMC 1 ", 00.73172, -73.62361, 1950, 0., 0.,2800, 0
11,"CAM01", 3.0, "N", "SMC 2 ", 00.77097, -73.50000, 1950, 0., 0.,2800, 0
12,"CAM01", 3.0, "N", "SMC H15 ", 00.77311, -73.65278, 1950, 0., 0., 900, 0
13,"CAM01", 3.0, "N", "SMC L36 ", 00.74736, -73.37583, 1950, 0., 0., 900, 0
14,"CAM01", 3.0, "N", "SMC L49 ", 00.77581, -73.36389, 1950, 0., 0., 900, 0
15,"CAM01", 3.0, "N", "M33 SW ", 01.51389, 30.33333, 1950, 0., 0.,3600, 0
16,"CAM04", 3.0, "N", "N891 Cen", 02.32350, 42.12000, 1950, 0., 0.,7200, 0
17,"CAM01", 3.0, "N", "N891 dis", 02.32350, 42.12000, 1950, 0., 0.,1600, 0
18,"CAM01", 3.0, "N", "N1365 ", 03.52833, -36.30500, 1950, 0., 0.,3600, 0
19,"CAM01", 2.0, "N", "LMCstrip", 05.40000, -70.00000, 1950, 0., 0.,12600, 0
20,"CAM01", 3.0, "N", "LMC N159", 05.67167, -69.83333, 1950, 0., 0.,3400, 0
21,"CAM01", 3.0, "N", "LMC N4 ", 04.86800, -67.00555, 1950, 0., 0.,1000, 0
22,"CAM01", 3.0, "N", "LMC SN87", 05.59722, -69.29944, 1950, 0., 0., 800, 0
23,"CAM01", 3.0, "N", "LMC N11a", 04.92667, -66.58000, 1950, 0., 0.,2800, 0
29,"CAM01", 3.0, "N", "LMC N11b", 04.95333, -66.48000, 1950, 0., 0.,1600, 0
30,"CAM01", 3.0, "N", "LMC N11c", 04.98000, -66.28000, 1950, 0., 0.,2800, 0
24,"CAM01", 3.0, "N", "N4736 ", 12.80883, 41.39333, 1950, 0., 0.,1800, 0
25,"CAM01", 1.0, "N", "M51 ", 13.46267, 47.45500, 1950, 0., 0.,4800, 0
26,"CAM01", 1.0, "N", "M101Earm", 14.34722, 54.63333, 1950, 0., 0.,5200, 0
27,"CAM01", 2.0, "N", "M83 ", 13.56961, -29.61333, 1950, 0., 0.,7000, 0
28,"CAM01", 3.0, "N", "N6744 ", 19.08388, -63.93833, 1950, 0., 0.,4800, 0
<=== spring_launch_targets ===>
1, "CAM03", 3.0, "N", "M31 REF", 00.70014, 41.18381, 1950, 0., 0., 900, 0
2, "CAM03", 3.0, "N", "M31 D478", 00.67278, 41.12667, 1950, 0., 0., 900, 0
3, "CAM03", 3.0, "N", "M31 D268", 00.65750, 40.84972, 1950, 0., 0., 900, 0
4, "CAM03", 3.0, "N", "M31 D192", 00.65208, 40.51250, 1950, 0., 0., 900, 0
5, "CAM03", 3.0, "N", "M31 D395", 00.66644, 41.01611, 1950, 0., 0., 900, 0
6, "CAM03", 3.0, "N", "M31 D535", 00.68111, 41.13694, 1950, 0., 0., 900, 0
7, "CAM03", 3.0, "N", "M31 D478S",00.67250, 41.10000, 1950, 0., 0., 900, 0
8, "CAM03", 3.0, "N", "M31 D307", 00.63892, 40.92889, 1950, 0., 0., 900, 0
9, "CAM03", 3.0, "N", "M31 D321", 00.66111, 40.81944, 1950, 0., 0., 900, 0
10,"CAM01", 3.0, "N", "SMC 1 ", 00.73172, -73.62361, 1950, 0., 0.,2800, 0
11,"CAM01", 3.0, "N", "SMC 2 ", 00.77097, -73.50000, 1950, 0., 0.,2800, 0
12,"CAM01", 3.0, "N", "SMC H15 ", 00.77311, -73.65278, 1950, 0., 0., 900, 0
13,"CAM01", 3.0, "N", "SMC L36 ", 00.74736, -73.37583, 1950, 0., 0., 900, 0
14,"CAM01", 3.0, "N", "SMC L49 ", 00.77581, -73.36389, 1950, 0., 0., 900, 0
15,"CAM01", 3.0, "N", "M33 SW ", 01.51389, 30.33333, 1950, 0., 0.,3600, 0
16,"CAM04", 3.0, "N", "N891 Cen", 02.32350, 42.12000, 1950, 0., 0.,7200, 0
17,"CAM01", 3.0, "N", "N891 dis", 02.32350, 42.12000, 1950, 0., 0.,1600, 0
18,"CAM01", 3.0, "N", "N1365 ", 03.52833, -36.30500, 1950, 0., 0.,3600, 0
19,"CAM01", 1.0, "N", "LMCstrip", 05.40000, -70.00000, 1950, 0., 0.,12600, 0
20,"CAM01", 3.0, "N", "LMC N159", 05.67167, -69.83333, 1950, 0., 0.,3400, 0
21,"CAM01", 3.0, "N", "LMC N4 ", 04.86800, -67.00555, 1950, 0., 0.,1000, 0
22,"CAM01", 3.0, "N", "LMC SN87", 05.59722, -69.29944, 1950, 0., 0., 800, 0
23,"CAM01", 3.0, "N", "LMC N11a", 04.92667, -66.58000, 1950, 0., 0.,2800, 0
30,"CAM01", 3.0, "N", "LMC N11b", 04.95333, -66.48000, 1950, 0., 0.,1600, 0
31,"CAM01", 3.0, "N", "LMC N11c", 04.98000, -66.28000, 1950, 0., 0.,2800, 0
24,"CAM01", 3.0, "N", "N4736 ", 12.80883, 41.39333, 1950, 0., 0.,1800, 0
25,"CAM01", 1.0, "N", "M51 ", 13.46267, 47.45500, 1950, 0., 0.,4800, 0
26,"CAM01", 1.0, "N", "M101Earm", 14.34722, 54.63333, 1950, 0., 0.,5200, 0
27,"CAM01", 3.0, "N", "N2841 ", 09.30972, 51.18833, 1950, 0., 0.,4800, 0
28,"CAM01", 2.0, "N", "M81 ", 09.85833, 69.30550, 1950, 0., 0.,4800, 0
29,"CAM01", 2.0, "N", "IZW18 ", 09.56750, 55.24333, 1950, 0., 0.,1800, 0