072C0287C.html |
RA Range: 02:10
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance):
0.8 2CLR 5.0 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 UVES-RED programme aimed at high-res spectroscopy of the faint companion of the exoplanet-system G186. Total execution time is only 2 hours and the programme includes 3 OBs only. Two of them are actually devoted to the companion, while one obtains spectroscopy of the main star. For the companion, the pointing is done through a blind offset from the bright star. Most likely, the companion will not be visible in the UVES slit viewer image. OB G186_star_1 should be executed just before or just after G186_companion_1. This should not cause any problem, since the duration of G186_star_1 is less than 10 minutes. OB G186_companion_2 should be executed a few months after. However, the PI says this is not a strong constraint, and smaller time separations would also be acceptable.
README of this run: