271D5006A.html |
RA Range:10:33
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 1.8 3THN 1.8 0.0 30.0
| Pre-imaging run? |
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Chilean run? |
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Special calibrations? |
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| Time critical? |
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ToO? |
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Carry-over run? |
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This is a FORS2 LSS (+IMG) programme on SN2003dh, which was associated with a GRB. Due to the RA of the target, the OBs must be executed before the end of May. Useful nights are from 23/05 to 27/05. Observations must be executed at the beginning of the night. Additionally, there are two OBs (labelled with "_June18") which must be executed on June 18 or 19, at the very beginning of the night. Included are also two identical Imaging OBs, one for the May slot ond the other for June. They should be executed just after one of the LSS OBs. The PI asks for the observation of a specific spectrophotometric STD star (either Feige66 or Feige67), which is included in the FORS calibration plan. Note that, even if they have specified a PA angle in order to include a field star in the slit, this is probably not accurate enough. The PI states in the README that this is not really important and that the acquisition should be done focussing on the SN only.
README of this run: