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? | |
|---|---|---|---|---|---|
|
Special Remarks:
NO REMARKS
Abstract for MTS:
This is a UVES/RED(600) programme on very bright stars (5th to 9th mag).
Note that the PI has specified a priority list (see README). Also, just before or just after, a telluric standard should be observed. The PI has provided a one-to-one science/telluric OB series.
Besides this, OBs can be executed any time.
The PI is asking for very high signal to noise (2000-3000) flats. I am not sure this can be achieved, since at that level the CCD features (electronic pikup noise, fixed structure) might prevent the achievement of such high levels.
In general, such high SNR requires some 50 flats, which are clarly not obtainable
in Service Mode. The user was made aware of this.
README of this run:
Web version of approved README readme_83050300.html