Chandra Source Catalog: Background Determination and Source Detection

Details Chandra Source Catalog: Background Determination and Source Detection Chandra Source Catalog: Background Determination and Source Detection

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21347210m&link_type=abstract

American Astronomical Society, AAS Meeting #213, #472.10; Bulletin of the American Astronomical Society, Vol. 41, p.426

Astronomy and Astrophysics

Astronomy

Scientific paper

The Chandra Source Catalog (CSC) is a major project in which all of the pointed imaging observations taken by the Chandra X-Ray Observatory will used to generate the most extensive X-ray source catalog produced to date. Early in the development of the CSC it was recognized that the ability to estimate local background levels in an automated fashion would be critical for essential CSC tasks such as source detection, photometry, sensitivity estimates, and source characterization. We present a discussion of how such background maps are created directly from the Chandra data and how they are used in source detection.
The general background for Chandra observations is rather smoothly varying, containing only low spatial frequency components. However, in the case of ACIS data, a high spatial frequency component is added that is due to the readout streaks of the CCD chips. We discuss how these components can be estimated reliably using the Chandra data and what limitations and caveats should be considered in their use.
We will discuss the source detection algorithm used for the CSC and the effects of the background images on the detection results. We will also touch on some the Catalog Inclusion and Quality Assurance criteria applied to the source detection results.
This work is supported by NASA contract NAS8-03060 (CXC).

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