Astro-2 and the UIT Experiment

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Дата изменения: Mon Oct 7 06:14:34 1996
Дата индексирования: Mon Oct 1 20:03:20 2012
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UIT Targets Sucessfully Acquired (Whew!):

Days 11--12:

We report here on those proposed UIT targets that, in fact, were successfully acquired. Where possible we provide an optical CCD image of the target or the field.

Note on Filters:

A1 centered at 2500 angstroms with a width of 1200 angstroms
B5 centered at 1615 angstroms with a width of 150 angstroms

Observed at MET: 11/01:06

NGC 4214 is a star forming irregular galaxy with a pronounced underlying old population as well. This observation was for 531 seconds through A1 and 1063 seconds through B1.

Observed at MET: 11/02:02

A western field in M31

1052

Observed at MET: 11/02:41

UGC 5675 is another Low Surface Brightness galaxy which is the center of the fourth deep A1 field. This exposure was for 1641 seconds through the A1 filter in orbital darkness.

Observed at MET: 11/12:43

M32 a very high surface brightness dwarf elliptical companion was observed for 1561 seconds through the B5 filter. This exposure is sufficiently deep that any hot stars associated with a recent star formation event should be visible. It is unknown, at present, if such a star formation event has occurred.

Observed at MET: 11/13:31

The Hercules Cluster was exposed again for 1310 seconds through the A1 filter.

Observed at MET: 11/14:11

NGC 6752

781