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:
The OBs for one particular target should be spread out over several months. PI woud like to have a given epoch finished for ALL targets before moving to the next epoch. For this reason, he has made use of the UsrP (User Priority) field.
Abstract for MTS:
UVES part of the program to monitor accreation rate of a few young stars.
Time gap note: Ideally the OBs for this run should be
spread out over several months. Minimum time gap
between OBs for a given target is one night.
PI woud like to have a given epoch finished for ALL
targets before moving to the next one. For this reason,
he has made use of the UsrP (User Priority) field.
For the SCrA_* OBs, the PI used a PA=157 in order to put both stars on the slit (second star not visible in the FC).
README of this run:
Web version of approved README readme_82000501.html