Monitoring the Spatial Variation of the ACIS Contaminant with Abell 1795

Physics

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Chandra Proposal Id #05808195

Scientific paper

The spatial distribution of the contaminant on ACIS must be monitored. The calibration team has developed a scheme that will measure the depth of the contaminant with an uncertainty of 3% on scales of 1 arcminute with a raster scan of the rich cluster A1795. This plan consists of 2 observations on ACIS-I and 3 observations on ACIS-S at different chipy locations.

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