69C0034A.html |
RA Range: 12.7h - 17.75h
Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 2.0 1PHO,3THN 2.0 0.5 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 program is a time series imaging observation of a single field in the open cluster IC4665. It has short OBs for photometric weather and very long OBs for the rest. The program requests for standard calibrations for R and I filters and submitted OBs for calibrations with narrow-band filters. Program needs a high signal-to-noise twilight flat in the I-filter and included the OB SkyflatI to obtain such a flat. Important!!!: 1. Please, note that this program is a time series, which is time-critical once it has been startet. It cannot be interrupted by other observations for other programs should the weather conditions change (i.e. once it has been started, it is very similar to a visitor mode program). 2. They use Move_to_gap template and have FCs for that. Aim: center the marked star on pixel (1443,2537) on chip.7 This corresponds to pixel (3585,2539) in the mosaic. Read README file for all details.
README of this run: