Discovery of a z=4.93, X-ray selected quasar by the Chandra Multiwavelength Project (ChamP).pdfVIP
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Discovery of a z=4.93, X-ray selected quasar by the Chandra Multiwavelength Project (ChamP)
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Discovery of a z=4.93, X-ray selected quasar by the Chandra
Multiwavelength Project (ChamP)
John D. Silverman1,2,3, Paul J. Green, Dong-Woo Kim, Belinda J. Wilkes, Robert A.
Cameron, David Morris, Anil Dosaj2
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138
Chris Smith
Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory,
Casilla 603, La Serena, Chile
Leopoldo Infante4
Departamento de Astronom??a y Astrof??sica, P. Universidad Cato?lica, Casilla 306, Santiago,
Chile
Paul S. Smith
Steward Observatory, The University of Arizona, Tucson, AZ 85721
Buell T. Jannuzi
National Optical Astronomy Observatory, P.O. Box 26732, Tucson, AZ, 85726-6732
Smita Mathur
Astronomy Department, Ohio State University, 140 West 18th Avenue, Columbus, OH
43210
ABSTRACT
1Astronomy Department, University of Virginia, P.O. Box 3818, Charlottesville, VA, 22903-0818
2Visiting Astronomer, Cerro Tololo Inter-American Observatory, National Optical Astronomy Observa-
tory, which is operated by the Association of Universities for Research in Astronomy, Inc. (AURA) under
cooperative agreement with the National Science Foundation.
3email: jds@
4Visiting astronomer, ESO New Technology Telescope
– 2 –
We present X-ray and optical observations of CXOMPJ213945.0-234655, a
high redshift (z = 4.93) quasar discovered through the Chandra Multiwavelength
Project (ChaMP). This object is the most distant X-ray selected quasar pub-
lished, with a rest-frame X-ray luminosity of LX = 5.9×10
44 erg s?1 (measured in
the 0.3–2.5 keV band and corrected for Galactic absorption). CXOMPJ213945.0-
234655 is a g′ dropout object ( 26.2), with r′ = 22.87 and i′ = 21.36. The
rest-frame X-ray to optical flux ratio is similar to quasars at lower redshifts and
slightly X-ray bright relative to z 4 optically-selected quasars observed with
Chandra. The ChaMP is beginning to acquire significant numbers of
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