273D5019A.html |
RA Range: 10:56
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance):
2.0 4THK 5.0 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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This is UVES-DIC1 programme on CN Leo. The programme is in principle simple, but it MUST be excuted simultaneosly with XMM-Newton. Due to the target's position, the observations MUST START AS SOON AS POSSIBLE AFTER SUNSET ON MAY 19 and continue until possible. Most probably not all OBs will be completed, but the user is aware of this. This means that on May 19, observations should start right with this programme and possible twilight calibrations should be postponed. The PI has put together 5 (identical) observing sequences to carry out the observations (with indicative start times): Sequence A must be executed during May 19 23:00 - 24:00. Sequence B must be executed during May 20 00:00 - 01:00. Sequence C must be executed during May 20 01:00 - 02:00. Sequence D must be executed during May 20 02:00 - 03:00. Sequence E must be executed during May 20 03:00 - 04:00. NOTE: the target has a rather high proper motion. The f. chart has the 2002 position marked. The current target's position should be a few arcsec away from it. NOTE also that the PI asks to get, if possible, the exp. meter data, which proved to be very useful in previous observations.
README of this run:
Check if ftp directory/ies exist/s for this run:
P72 Directory does not exist for 273.D-5019A
P73 Directory exists for 273.D-5019A
P74 Directory does not exist for 273.D-5019A
P73 run ...search for JPEG finding charts in database:
Finding charts, click on them to display:
| OB_ID | OB_name | Finding chart |
| OB:163810 | CN Leo 5 | CN_Leo_new.jpg |
| OB:163811 | CN Leo 4 | CN_Leo_new.jpg |
| OB:163812 | CN Leo 3 | CN_Leo_new.jpg |
| OB:163813 | CN Leo 2 | CN_Leo_new.jpg |
| OB:163808 | CN Leo 1 | CN_Leo_new.jpg |