66B0323A.html |
RA Range:2-3hrs
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 0.6 1PHO 1.8 0.1 90
| 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 "pre-imaging" required in good seeing in order to determine whether or not the 2 targets in question are useful for part C of this program. Note the desire to check these two targets was only described in the text of proposal and not requested as a pre-imaging program in its own right and the good seeing requirement was also only briefly mentioned in the text proposal. The proposers state that they will supply new targets if one or both of the galaxies to be imaged here in part A turn out to have undesired warped disks..great. Just to be clear, the names of the two targets to be checked for warping are: UGCA023 abd ESO0299. In part C, a third galaxy is included for which they would like deep imaging in relatively poor seeing since it is already known to be suitable for their program and this object is called ESO0342-G017, and this object can be observed right away (although is at 21hrs so not likely to get observed now) but the two other galaxies also included in part C for deep poor-seeing observations are the two listed above in Part A of this program and should not be observed in part C until they are approved by the PI on the basis of the good seeing images requested here in part A. Note that this third galaxy ESO0342-G017 is also to be observed in good seeing and has been placed in part B of this program whos aim is to obtain good seeing images of this object for some reason alluded to in the text of the phase I proposal. Backup galaxies exist approved in phase I should they be required to replace warped disk objects. This program was split into 3 parts by Dave to help in tracking, and finally agreed to by De Marchi who prepared the OB's.
README of this run: