267B5133B.html |
RA Range: 10
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 2 CLR 1.5 1 30
| 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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SW LR in J spectroscopy of a candidate supernova in NGC 3256. FORS observations of the source are done under 267.B-5133(A): not simultaneous observations with FORS are needed. User says: "The observations are not extremely time critical, however the SN was K=16.5 in January, K=18 in March. A delay of few days is not a disaster but a month could be too much" A telluric standard is provided.
README of this run: