073A0340A.html |
RA Range: 11.8 - 16
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance):
0.8 2CLR 1.5 1.0 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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J, H, K MR spectroscopy of 4 Lyman break galaxies. Moderate constraints, part B of this program requires PHO for the same observations. The acquisition strategy is somewhat unconventional: If the targets are visible, acquire directly (and, if applicable, include the "pivot star" in the slit by adjusting PA). However, if the target is NOT visible, just shift the slit to go through the pivot star. However, do not center the star in the slit, but keep approximately the original distance to the slit centre. That way, the target stays ~ in the centre. This is different from the usual "blind target acquisition" strategy, because there is substantial hope that the target can be acquired directly.
README of this run:
Check if ftp directory/ies exist/s for this run:
P72 Directory does not exist for 073.A-0340A
P73 Directory exists for 073.A-0340A
P74 Directory does not exist for 073.A-0340A
P73 run ...search for JPEG finding charts in database:
Finding charts, click on them to display:
| OB_ID | OB_name | Finding chart |
| OB:161828 | SDSS1432-0001-H-P2 | s1432aP2.jpg |
| OB:161830 | SDSS1553+0056-H-P2 | s1553aP2.jpg |
| OB:156516 | SDSS1147-0250-J | s1147aP1.jpg |
| OB:161832 | SDSS1147-0250-H-P2 | s1147aP2.jpg |
| OB:156501 | SDSS1553+0056-K | s1553aP1.jpg |
| OB:156503 | SDSS1553+0056-H | s1553aP1.jpg |
| OB:156507 | SDSS1432-0001-K | s1432aP1.jpg |
| OB:156510 | SDSS1432-0001-J | s1432aP1.jpg |
| OB:156512 | SDSS1553+0056-J | s1553aP1.jpg |
| OB:156513 | SDSS1147-0250-K | s1147aP1.jpg |
| OB:156515 | SDSS1147-0250-H | s1147aP1.jpg |