1 citations · 1 across the 2 of their papers we have counts for
6 papers
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…
Understanding the Elusive Dwarf Carbon Star
Paul J. Green
Most stars in our Galaxy with photospheric C/O>1 (carbon stars) are not giants but dwarfs. The newly-recognized class of dwarf carbon (dC) stars joins the growing family of stars w…