072C0071A.html |
RA Range: 03:47
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance):
2.0 2CLR 2.5 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 UVES-RED programme aimed at determining the radial velocity curve of an eclipsing brown dwarf. OBs are all identical and MUST be executed in different nights. The users suggests to execute one OB each clear night, once the sequence is started. A two-week time span would be optimal. Note that the PI has included one OB for HR948, a telluric standard. No time contraint for this OB is given.
README of this run: