270C5010A.html |
RA Range: 20:41, 21:47, 21:49
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 0.8 3THN 2.0 1.0 45
| 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 simple DDT imaging programme on Uranus and Neptune satellites. The OB execution is strongly inter-dependent. The optimal execution sequence should be as follows: 2002N4-1, 2002N6-1, c02u5-1, 2001U1-1, 2002N4-2, 2002N6-2 on one night, and c02u5-2, 2001U1-2 the night after. The following constraints have also to be met: 2002N4-2: at least 1 hour and at most 50 hours after 2002N4-1; 2002N6-2: at least 1 hour and at most 50 hours after 2002N6-1; c02u5-2 : at least 20 hours after c02u5-1 but before Nov 8; 2001U1-2: at least 20 hours after 2001U1-1 but before Nov 8; For more details see the README file. Note that the users supply the ephemeris directly in the README file, since only 4 nights are suitable for the observations.
README of this run: