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Time Critical |
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Last update of this page: Wed Oct 7 15:41:04 2009
Run State: TERMINATED/EP
USD review status:
O.K.!
| Pre-Imaging? | Special-Calibration? | Time-Critical? | ToO/GTO/Large program? | Carry-Over? | ||
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Special Remarks:
NO REMARKS
Abstract for MTS:
FORS2 Long slit spectroscopy of 10 asteroids. Observations of a standard star is required after each LS spectrum is observed : the PI has supplied 12 calibration OBs, and only 9 of those should be executed.
PI asks that the standard star is observed during the same night as the asteroid and just after the object with similar atmospheric conditions and airmass.
No finding charts are attached to the OBs but they are available at the following website:
http://asteroid.lowell.edu/cgi-bin/koehn/astfinder
Time-Critical Aspects
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The targets need to be observed close to oppostion because they are brighter there and with an airmass under 1.7. The only exception is for the asteroid 14627 which can not be observed at optimal airmass. Anyway, we ask that the asteroid is observed with an airmass under 1.9.
For each object, we list the OB name, the starting date and ending date (i.e. time intervals).
OB Starting date Ending date
MOV_1270 2007-11-28T07:20 2008-03-08T03:00
MOV_60151 2008-03-09T05:20 2008-03-31T10:40
MOV_89309 2007-10-01T23:00 2007-11-05T01:00
MOV_2003SQ168 2008-01-06T05:00 2008-02-12T05:00
MOV_14627 2008-01-06T08:00 2008-03-31T03:40
MOV_1992YC2 2008-03-01T09:00 2008-03-31T10:40
MOV_21509 2008-03-01T04:40 2008-03-31T09:00
MOV_2003VM9 2008-02-13T04:20 2008-03-25T05:40
MOV_2004XL40 2007-10-01T00:20 2007-10-22T05:40
README of this run:
Web version of approved README readme_80024100.html