Last update of this page: Thu Mar 31 17:45:24 2005
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0 done (of 11 OBs)
0.00 hrs done (of 6.63 hrs) |
| PHOT | CLR | THN | THK | Seeing & Airmass Constraints: |
| -- | 11 OB(s) |
-- | -- |
Seeing < 0.80 Airmass < 2.00 |
Last update of the USG file: Oct 25 19:25:05 2004
Major Instrument Modes: ISAAC Hawaii Imaging Nb1.64
RA Range: 03:32
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance):
0.8 2CLR 2.0 0.4 60.
| Pre-imaging run? |
|
Chilean run? |
|
Special calibrations? |
|
|
| Time critical? |
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ToO? |
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Carry-over run? |
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Narrow band imaging (1.64) of the UDF to look for Halpha emitters for determination of SFR. The OBs are all identical and should all have the same pointing. They impose the lunar constraint to achieve their limiting magnitudes. I'm not sure how valid this reason is at H-band. There is an accompanying B-run with the broadband imaging. Even though I requested it, larger finding charts or finding charts where the orientation arrows actually print were not provided (yet). If you cannot identify the field, don't repeat the OB, but please inform USD.
Approved README of this run:
Finding charts are attached to the following OBs of this run:
| OB_ID | OB_name | Finding chart |
| OB:172923 | Halpha Sci Nb1.64-11 | udf_1.6micron.jpg |
| OB:172928 | Halpha Sci Nb1.64-7 | udf_1.6micron.jpg |
| OB:172925 | Halpha Sci Nb1.64-10 | udf_1.6micron.jpg |
| OB:172926 | Halpha Sci Nb1.64-9 | udf_1.6micron.jpg |
| OB:172927 | Halpha Sci Nb1.64-8 | udf_1.6micron.jpg |
| OB:172929 | Halpha Sci Nb1.64-6 | udf_1.6micron.jpg |
| OB:172930 | Halpha Sci Nb1.64-5 | udf_1.6micron.jpg |
| OB:172931 | Halpha Sci Nb1.64-4 | udf_1.6micron.jpg |
| OB:172932 | Halpha Sci Nb1.64-3 | udf_1.6micron.jpg |
| OB:172933 | Halpha Sci Nb1.64-2 | udf_1.6micron.jpg |
| OB:172934 | Halpha Sci Nb1.64-1 | udf_1.6micron.jpg |
| OB_ID | OB_name | Ephemeris file |