67A0361E.html |
RA Range: 9 -- 15
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 0.8 CLR 1.8 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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Js BB follow up imaging of distant Supernova just discovered past April. ! Time critical: observations should be done during the first two weeks of May. Currently, the program is on hold ==>Chris will directly inform PSO on which OBs should be observed. This is to cope with simultaneous space and ground-based observations. For some SNs, observations are split in several OBs to cope with long integrations. It is important to execute all the OBs of a single SN as close in time as schedule allows. Program is oversubscribed: yet some SNe will be observed by other observatories and will thus NOT be repeated with VLT. Chris will inform USG on which targets should be cancelled.
README of this run: