<=== observer ===>
"HWALKER",\
"Walker, H.J.",\
"Rutherford Appleton Laboratory",\
"Chilton",\
"Oxon",\
"",\
"OX11 0QX",\
"DIDCOT",\
"United Kingdom",\
"44 235 446490",\
"44 235 446667",\
"hjw@star.rl.ac.uk"
<=== proposal ===>
"P32B",1,3,\
{"stellar atmospheres","main sequence stars"},\
{"I. Heinrichsen"}
<=== title ===>
The infrared energy distributions of M dwarfs
<=== abstract ===>
SCIENTIFIC ABSTRACT
Observations of low mass stars, such as M dwarfs, are vital for models of our
galaxy. Waters et al. (1987) showed that M stars were under-represented at IRAS
wavelengths. Photometry will be performed to establish whether the infrared
energy distribution of M dwarfs is of the thermal black-body type, or whether
it is dominated by features, either from molecular absorption bands or dust
emission. Photometry will be performed on a set of M dwarfs, which are not known
to have significant mass loss or optical emission features.
OBSERVATION SUMMARY
PHT-P broad band photometry will be performed for all the stars proposed,
using P03 with 7 filters and a 99" aperture. The filters selected are;
7.7, 10, 12.8, 16, 25, 60, 100 um. The observations will use the chopper
in rectangular mode, with a 120" chop. For GL726, the 100um band is not
selected. The integration time selected is 32sec in all cases.
The times are estimated using the cookbook.
<=== scientific_justification ===>
Time distribution for autumn lauch targets:
Team top 40% second 30% last 30%
PHT : 0 0 14191
Time distribution for spring launch targets:
Team top 40% second 30% last 30%
PHT : 0 0 15216
<=== autumn_launch_targets ===>
1, "PHT03", 3.0, "N", "GL887 ", 23.04417, -36.14167, 1950, 6.776, 1.310, 951,0
2, "PHT03", 3.0, "N", "GL411 ", 11.01028, 36.30500, 1950,-0.566,-4.743, 951,0
3, "PHT03", 3.0, "N", "GL1 ", 0.04111, -37.60333, 1950, 5.648,-2.329, 951,0
4, "PHT03", 3.0, "N", "GL832 ", 21.50389, -49.22000, 1950,-0.060,-0.810, 951,0
5, "PHT03", 3.0, "N", "GL338 ", 9.18306, 52.90167, 1950,-1.572,-0.587, 951,0
6, "PHT03", 3.0, "N", "GL619 ", 16.32000, 41.07666, 1950,-0.031, 0.126, 951,0
7, "PHT03", 3.0, "N", "GL726 ", 18.74722, -3.69167, 1950,-0.123,-0.247, 877,0
8, "PHT03", 3.0, "N", "GL699 ", 17.92306, 4.55500, 1950,-0.750,10.310, 951,0
9, "PHT03", 3.0, "N", "GL752 ", 19.24139, 5.09667, 1950,-0.590,-1.350, 951,0
10, "PHT03", 3.0, "N", "GL866 ", 22.59583, -15.59333, 1950, 2.340, 2.270, 951,0
11, "PHT03", 3.0, "N", "GL447 ", 11.75250, 1.10000, 1950, 0.650,-1.220, 951,0
12, "PHT03", 3.0, "N", "GL727 ", 18.76861, 10.69500, 1950, 0.141,-0.439, 951,0
13, "PHT03", 3.0, "N", "GL406 ", 10.90167, 7.32000, 1950,-3.850,-2.700, 951,0
14, "PHT03", 3.0, "N", "GL821 ", 20.10833, -13.47833, 1950, 0.710,-1.960, 951,0
15, "PHT03", 3.0, "N", "GL829 ", 21.45333, 17.41833, 1950, 1.000, 0.380, 951,0
<=== spring_launch_targets ===>
1, "PHT03", 3.0, "N", "GL887 ", 23.04417, -36.14167, 1950, 6.776, 1.310, 951,0
2, "PHT03", 3.0, "N", "GL411 ", 11.01028, 36.30500, 1950,-0.566,-4.743, 951,0
3, "PHT03", 3.0, "N", "GL1 ", 0.04361, -37.60333, 1950, 5.648,-2.329, 951,0
4, "PHT03", 3.0, "N", "GL832 ", 21.50389, -49.22000, 1950,-0.060,-0.810, 951,0
5, "PHT03", 3.0, "N", "GL338 ", 9.18306, 52.90167, 1950,-1.572,-0.587, 951,0
6, "PHT03", 3.0, "N", "GL191 ", 5.16139, -44.99833, 1950, 6.595,-5.702, 951,0
7, "PHT03", 3.0, "N", "GL310 ", 8.53194, 67.46833, 1950,-0.130,-0.146, 951,0
8, "PHT03", 3.0, "N", "GL273 ", 7.41194, 5.37833, 1950, 0.590,-3.720, 951,0
9, "PHT03", 3.0, "N", "GL866 ", 22.59583, -15.59333, 1950, 2.340, 2.270, 951,0
10, "PHT03", 3.0, "N", "GL447 ", 11.75250, 1.10000, 1950, 0.650,-1.220, 951,0
11, "PHT03", 3.0, "N", "GL123 ", 3.06389, -17.85167, 1950, 0.387,-0.884, 951,0
12, "PHT03", 3.0, "N", "GL84 ", 2.04361, -17.85167, 1950, 1.280,-0.160, 951,0
13, "PHT03", 3.0, "N", "GL234 ", 6.44750, -2.77000, 1950, 0.730,-0.690, 951,0
14, "PHT03", 3.0, "N", "GL406 ", 10.90167, 7.32000, 1950,-3.850,-2.700, 951,0
15, "PHT03", 3.0, "N", "GL821 ", 20.10833, -13.47833, 1950, 0.710,-1.960, 951,0
16, "PHT03", 3.0, "N", "GL829 ", 21.45333, 17.41833, 1950, 1.000, 0.380, 951,0