70D0046A.html |
RA Range: ToO
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 1.8 4THK 3.0 1.0 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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This is a ToO programme to detect narrow absorption/emission features in early stage supernovae. Finding charts and additional information will be supplied by the PI when the observations will be triggered. Note that the execution strategy changes according to the SN type: Ia) two epochs (1st + 2 days later) II) 4 epochs (1st + 3,7,14 days later) First epochs are equal for the two types, i.e. 4800s+DIC1 and 4800s+DIC2. Following epochs are different: Ia) 3x3600s+DIC1 and 3x3600s+DIC2; II) 2400s+DIC1 and 2400s+DIC2.
README of this run: