Last update of this page: Wed Jul 23 15:41:28 2008
Run State: TERMINATED/EP
USD review status:
O.K.!
| Pre-Imaging? | Special-Calibration? | Time-Critical? | ToO/GTO/Large program? | Carry-Over? | |
|---|---|---|---|---|---|
|
Special Remarks:
NO REMARKS
Abstract for MTS:
In this run PI is going to observe 4 galactic bulge fields and 2 galactic disk fields.
Program has one OB per field with short exposures in the UBVI filters. There are 6 OBs to observe during PHO conditions and 6 OBS for them to observe Landolt standard stars during the same nights to calibrate the data (program uses non-standard U, B and I filters).
PI assigned to each field a priority (determined by OB name):
-------------------------------------------------------------
1st priority: Bulge1, std-bulge1, Disk1 and std-disk1
2nd priority: Bulge2 and std-bulge2
3d priority: Bulge3, std-bulge3, Disk2 and std-disk2
4th priority: Bulge4 and std-bulge4
The U and I filters are non-standard and PI have prepared and submitted CalOBs to take skyflats and domeflats. Regard to the B filter, for 4 fields it is also non-standard filter and PI have prepared and submitted OBs for skyflats and domeflats. Only part of them should be done to support OBs, observed in the same/previous night.
Please, see README file for more details.
See User Priority for OBs.
README of this run:
Web version of approved README readme_75029100.html