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The unprecedented spatial resolution and sensitivity of the Chandra
X-ray Observatory provides a rich archive of serendipitous sources.
The ChaMP seeks to understand the nature and evolution of
quasars, galaxies, and clusters of galaxies in a large, carefully
constructed multi-wavelength survey. A team of scientists, led
by staff members at the Chandra X-ray Center (CXC) with collaborators
from NOAO, MIT, MMTO, SDSS, UofA, MSU, OSU, Ohio, UT, Rome, Italy and
Bristol, UK, is carrying out a multi-wavelength identification program
for these X-ray sources. In addition to our extragalactic study, a Chandra Galactic Plane survey, ChaMPlane, is being led by Josh Grindlay
Recent ChaMP Papers The Luminosity Function of X-ray Selected Active Galactic Nuclei: Evolution of Supermassive Black Holes at High Redshift(PDF) Silverman, J. D. et al. 2007, arXiv0710.2461 (ApJ, in press) Chandra Multiwavelength Project X-ray Point Source catalog(PDF) M. Kim et al., 2007, ApJS, 169, 401 Chandra Multiwavelength Project X-ray Point Source Number Counts and the Cosmic X-ray Background(PDF) M. Kim et al., 2007, ApJS, 659, 29 ChaMP Serendipitous Galaxy Cluster Survey(PDF), Barkhouse et al., 2006, ApJ, 645, 955 Chandra Multiwavelength Project: Normal Galaxies at Intermediate Redshift, Kim, D.-W. et al. 2006 ApJ, 644, 829
Co-moving space density of X-ray-selected Active Galactic Nuclei,
Silverman et al. Hard X-ray emitting Active Galactic Nuclei selected by the Chandra Multi-wavelength Project, Silverman et al., 2005 ApJ, 618, 123
Discovery of a Jetlike Structure at the High-Redshift QSO CXOMP J084128.3+13110
Schwartz et al. 2004, ApJ Letters, 605, 105 ChaMP Contact Information:
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Date Last Modified: 29 November 2006
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