115 citations · 116 across the 3 of their papers we have counts for
7 papers · 1 filter
Chandra Multiwavelength Project X-ray Point Source Number Counts and the Cosmic X-ray Background
Minsun Kim, Belinda J. Wilkes, Dong-Woo Kim +5
We present the Chandra Multiwavelength Project (ChaMP) X-ray point source number counts and the cosmic X-ray background (CXRB) flux densities in multiple energy bands. From the Cha…
X-ray emitting AGN unveiled by the Chandra Multiwavelength Project
John D. Silverman, Paul J. Green, Thomas L. Aldcroft +4
We present an X-ray and optical analysis of a 2-8 keV flux limited (fx > 10e-14 erg s^-1 cm^-2) sample of 126 AGN detected in 16 Chandra fields. This work represents a small though…
Emission Line Properties of AGN from a post-COSTAR FOS HST Spectral Atlas
J. K. Kuraszkiewicz, P. J. Green, D. M. Crenshaw +4
This paper joins a series compiling consistent emission line measurements of large AGN spectral databases, useful for reliable statistical studies of emission line properties. It i…
ChaMP and the High Redshift Quasars in X-rays
S. Mathur, H. Marshall, N. Evans +2
Chandra X-ray Observatory, (formerly known as AXAF), will observe down to the flux limit of 2\times 10^{-16} erg~s^{-1} cm^{-2}. In its first year of operation Chandra's CCD detect…
Evidence Against BALS in the X-ray Bright QSO PG1416-129
Paul J. Green, Thomas L. Aldcroft, Smita Mathur +1
Recent results from the ROSAT All Sky Survey, and from deep ROSAT pointings reveal that broad absorption line quasars (BALQSOs) are weak in the soft X-ray bandpass (with optical-to…
Emission Lines and the Spectral Energy Distributions of Quasars
B. J. Wilkes, P. J. Green, S. Mathur +1
Many years of study have failed to conclusively establish relations between a quasar's spectral energy distribution (SED) and the emission lines it is thought to produce. This is a…