Classifying Serendipitous Sources for the ChaMP

Details Classifying Serendipitous Sources for the ChaMP Classifying Serendipitous Sources for the ChaMP

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.1116w&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #11.16; Bulletin of the American Astronomical Society, Vol. 34, p.1111

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ChaMP, the Chandra Multiwavelength Project, is producing a large database of optical, radio, and other wavelength data to complement the archived observations made by the Chandra X-ray observatory. A key component of the project is the classification of X-ray objects using optical spectroscopy. We develop and test a semi-automated cross-correlation routine on a bright (r'<17) and on a fainter (1780% of the identified AGN and for 60% of identified galaxies. The overall X-ray and optical properties of the extragalactic faint sample are also presented and briefly discussed. The ChaMP project can be found on the web at http://hea-www.harvard.edu/CHAMP/. This work was funded in part by NSF grant AST-9731923 through the SAO Summer Intern Program.

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