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Time Critical |
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:
FORS2 LS spectroscopy of binary stars. 30 faint WDMS have been selected to be observed with FORS equipped with the GRS_1028z+29 grating. The PI needs two ~15min exposures of each system to measure radial velocity variations. The two spectra of an individual system should not be taken in the same night (see time-critical aspects).
Time-Critical Aspects
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WeThe scientific requirements need two spectra of each targets. There are two OBs for each target, which are labeled object-name and object-name-0. The two OBs of an individual object must be executed in two different (ideally consecutive) nights.
README of this run:
Web version of approved README readme_80040700.html