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astro-ph2004

The Power of Exploratory Chandra Observations

S. C. Gallagher, G. T. Richards, W. N. Brandt +1

With its excellent spatial resolution, low background, and hard-band response, the Chandra X-ray Observatory is ideal for performing exploratory surveys. These efficient, sensitive…

astro-ph2003

SDSS Quasars and Dust Reddening

Patrick B. Hall, Philip Hopkins, Michael Strauss +2

The Sloan Digital Sky Survey can be used to detect and characterize red and reddened quasars. In Richards et al. (2003), we showed that 6% of SDSS quasars have red colors consisten…

astro-ph2003

Constraints on Quasar Continuum, BELR, and BALR Physics from SDSS Composite Spectra

Gordon T. Richards, Patrick B. Hall, Timothy A. Reichard +3

We review recent results on quasars from the SDSS as they relate to our understanding of the UV/optical continuum, the broad emission line region, and the broad absorption line reg…

astro-ph2003

Quasar Radio Dichotomy: Two Peaks, or not Two Peaks, that is the Question

Z. Ivezic, G. T. Richards, P. B. Hall +8

Recent claims by Ivezic et al. (2002) that the distribution of the radio-to-optical flux ratio, R, for quasars is bimodal (the so-called quasar radio dichotomy) were questioned on…

astro-ph2003

Counts of Low-redshift SDSS Quasar Candidates

Z. Ivezic, R. H. Lupton, D. E. Johnston +10

We analyze the counts of low-redshift quasar candidates selected using nine-epoch SDSS imaging data. The co-added catalogs are more than 1 mag deeper than single-epoch SDSS data, a…

astro-ph2002

X-rays from the First Massive Black Holes

W. N. Brandt, C. Vignali, D. P. Schneider +7

X-ray studies of high-redshift (z > 4) active galaxies have advanced substantially over the past few years, largely due to results from the new generation of X-ray observatories. A…