C H A N D R A
S C I E N C E
C E N T E R O B S E R V A T I O N C A T A L O G |
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Abstract: Understanding the rapid growth of supermassive black holes and the assembly of their host galaxies is severely limited by the lack of reliable estimates of black-hole mass and accretion rate in distant quasars. We propose Chandra observations of 54 luminous, high-redshift quasars to boost our ability to identify the most reliable and practical Eddington-ratio indicator. In conjunction with archival data, we will investigate diagnostics of quasar accretion power in the X-ray and UV-optical spectral bands of a carefully selected sample of ~80 sources. We will ``stress test'' these diagnostics, relying critically on the X-ray observable properties, and deliver a prescription for the most robust Eddington-ratio estimate that can be utilized economically at the highest accessible redshifts. |
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