66B0331A.html |
RA Range: 4:45-6:30
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance):
| 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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Spectroscopy of several stars in LMC clusters. Targets never very high, hence the relaxed airmass constraint. Seeing constraint as defined by user actually refers to DIMM measurements; worse quality is admissible, especially in view of the high airmass at which the observations need to be done. The two targets not in phase 1 proposal are actually comparison stars. No special calibrations needed.
README of this run: