69D0178A.html |
RA Range: 17:52, 19:18
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 1.0 2CLR 5.0 0.3 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 simple LSS/IMAGING programme, aimed to obtain low resolution spectroscopy and broad band imaging for two helium flash objects, i.e. V4334 (Sakurai's Object) and V605 Aql. The idea is to derive physical parameters of the stellar remnants trhough atmosphere modelling and optical properties of dust shells. The high priority target is V4334, which should be around I=21.5. V605 is fainter, V=23, and surrounded by a central nebula, which will be possibly resolved in the FORS2 images. Notice that the user writes in the finding charts that the position angle should be chosen by the observer. Please, ignore this statement. Position angle is set to 0.
README of this run: