Last update of this page: Wed Apr 1 15:42:30 2009
Run State: TERMINATED/EP
USD review status:
O.K.!
| Pre-Imaging? | Special-Calibration? | Time-Critical? | ToO/GTO/Large program? | Carry-Over? | ||
|---|---|---|---|---|---|---|
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Special Remarks:
OBs must be executed in specific time windows (May to August)
Abstract for MTS:
This is a FORS2/LSS programme on old Supernovae.
OBs are grouped into 9 sets, with different priorities (see also the UsrP field
in OT). Each set has also a specific time window. Please, refer to the README file
for a detailed time schedule).
OBs belonging to the same set should be executed as close as possible in time,
ideally, within the same night.
In the case one or more sets are not completed, the night astronomer should still try to proceed with the remaining sets. According to the way things evolve, the PI might change the strategy during the last months of the period.
Note that for some of the sets, the PI has submitted a calibration OB, which
should be executed after one of the science OBs.
IMPORTANT NOTE: run (B) contains the imaging part of this program. See the README
about the coordinations between LSS and IMG. As a rule of thumb, for each LSS set there is one IMG OB.
Finally, note that the parallactic angle is used, and hence the slits are not
drawn in the finding charts.
README of this run:
Web version of approved README readme_79071600.html