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:
Execute OBs in blocks of 4 (PA=0,90,180,270)!
Abstract for MTS:
This is a UVES/RED programme on spectro-astrometry of Be stars.
For each target the PI has submitted 4 OBs, which differ for the slit position angle:
0, 90, 180, 270. OBs should be executed in blocks of 4, with the four PAs one after the other.
Even though the acquisition cannot be skipped (since it sets the adapter position angle), the telescope preset can be skipped after the first OB in each block. The effective execution time of each blouck should be always less than one hour.
Note that the OBs make use of the _expfree_ template, coupled to a Halpha interference filter. Also, attached wavelength calibrations are used. The PI is aware that he will not received pipeline processed data.
Since the PI wants to reach the maximum exposure level and the Halpha line is variable, there is some risk of saturation. For this reason the PI asks the NA to check the exposure level on the first of the sub-integrations and, in case of saturation, to reduce the exposure time of the remaining integration.
The PI is aware that this will be done on a best effort basis.
Targets are bright. No finding charts are supplied.
README of this run:
Web version of approved README readme_82014000.html