CCD Daily Monitor {Part 1}

Computer Science

Scientific paper

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Scientific paper

This program comprises basic tests for measuring the read noise and dark current of the ACS WFC and for tracking the growth of hot pixels. The recorded frames are used to create bias and dark reference images for science data reduction and calibration. This program will be executed four days per week {Sun, Mon, Wed, Fri} for the duration of Cycle 17 {1 August 2009 - 1 November 2010}. To facilitate scheduling, this program is split into three proposals. This proposal covers 352 orbits {22 weeks} from 1 August 2009 to 1 January 2010.;

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