68D0112B.html |
RA Range: 04:41
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 1.0 2CLR 1.6 0.2 40.
| Pre-imaging run? |
|
Chilean run? |
|
Special calibrations? |
|
|
| Time critical? |
|
ToO? |
|
Carry-over run? |
|
FIMS-based LSS and IMG of SN1999em. Time critical: the aim of the program is to follow the evolution of the supernova. This run is the second epoch, 68.D-0112(A) was the first, and it should be executed as late as possible in the period (preferably close to new moon on Feb 11, but new moon in January is also acceptable). All OBs for run (B) should be executed at the same time, i.e. within one week. If the spectroscopic OBs are executed in a sequence re-acquisition can be skipped.
README of this run: