168.A-0485(B) |
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PI:Cesarsky/ Bergeron/ Cristiani/ da Costa/ Dickinson/ Elbaz/ Fosbury/ Giavalisco/ Hook/ Renzini/ Rosati |
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| * Rank Class: A |
Last update of this page: Mon Apr 2 13:45:03 2007
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62 done (of 89 OBs)
51.12 hrs done (of 56.03 hrs) |
| PHOT | CLR | THN | THK | Seeing & Airmass Constraints: |
3 OB(s) |
-- | -- | -- |
Seeing < 1.00 Airmass < 1.20 |
Last update of the USG file: Oct 20 14:08:34 2004
Major Instrument Modes: WFI with BVR filters
RA Range: 3.5 (single field)
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance):
1.0 PHO 1.2 0.0/0.4 180
| 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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Long program, simple broadband imaging of a deep field divided into several areas. Program needs the standard photometric calibrations in BVR. No special calibrations needed, and no time constraints. Period 70: Observation of a spectrophotometric standard star in U#877, U#841, I#845, I#879. Magnitude of spectrophotometric standard SA95-42: V=15.61, A type star. The spectrophotometric standard star SA95-42 is observed in the old and new U and I filters. Standard calibration for U/50 and I#879. Non-standard calibration U and I twilight (FS-F* OBs) and dome flats (FD-F*-1, FD-F*-2, FD-F*-3 OBs) to be observed before and after the corresponding OBs for the spectrophotometric standard are carried out. Three different sets dome flat OBs for different exposure levels are provided. One of each should be carried out during each calibration.
Approved README of this run:
Finding charts are attached to the following OBs of this run:
| OB_ID | OB_name | Finding chart |
| OB_ID | OB_name | Ephemeris file |
| ProgId | USD-EntryId | SenderEmail | EntryTime | Last Ticket Update Time |
Short Problem Description |
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