X-ray Properties of Optical Sources in the Lockman Hole - Northwest

Details X-ray Properties of Optical Sources in the Lockman Hole - Northwest X-ray Properties of Optical Sources in the Lockman Hole - Northwest

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.8502s&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #85.02; Bulletin of the American Astronomical Society, Vol. 34, p.1244

Astronomy and Astrophysics

Astronomy

Scientific paper

We present Chandra X-ray observations of optical sources in the Lockman Hole - Northwest. Our nine moderately deep ( 40 ks) Chandra pointings cover an area of 0.36 deg2 to a depth of 2 x 10-15 erg cm-2 s-1 in the soft band (0.5 - 2 keV) and 1.5 x 10-14 erg cm-2 s-1 in the hard band (2 - 8 keV). Using deep BVRIz observations from Subaru's Suprime-CAM we group the optical sources by their observed properties (i.e., magnitude, color, etc...). We use a stacking procedure to measure the X-ray properties of each group of optical sources.

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