Last update of this page: Tue Oct 7 15:41:33 2008
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:
This is runB of a programme using both FEROS (runA) and UVES. The aim is to measure the metallicity of a sample of M dwarfs, by observing all primary components with FEROS and all secondary ones with UVES.
Notes: for 2 targets (GJ9390B and GJ1126B) there might be some light contamination from the primary, but PI said that he has already successfully observed them in the past (though under very good seeing conditions) and that target coordinates should have a 1" accuracy.
NEW NOTE (17.11.06): if you experience problems in identifying the right target (because on FC primary is too bright), please dump SV image and let us know . Unfortunately, user is able to correctly identify target only from SV image.
Since this has happened already for GJ1126B (cf USD-17936 and newly attached FC)
it may happen again also for GJ9390B (and maybe other stars).
README of this run:
Web version of approved README readme_78076001.html