Last update of this page: Wed Oct 7 15:41:04 2009
Run State: COMPLETED
USD review status:
O.K.!
| Pre-Imaging? | Special-Calibration? | Time-Critical? | ToO/GTO/Large program? | Carry-Over? |
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Special Remarks:
NO REMARKS
Abstract for MTS:
ISAAC SWS-LR 2.2 microns to observe the CO absorption feature in ultra-compact
dwarf galaxies compared to a comparsion source.
There are 12 identical OBs on the primary source called UCD*, where the slit
includes two UCDs in the Virgo cluster.
There are 4 OBs on the comparison source called GC*, and two further
reference sources (Gliese 880 and M87). The latter are bright, and the
seeing for Gliese 880 should be worse than 1.2 arcsec to avoid saturation.
Note added 30 June: The GC* OBs are completed. So, from now on there are
only UCD* OBs left to complete.
README of this run:
Web version of approved README readme_81028200.html