activity
19972011
most citedThe Chandra COSMOS Survey, I: Overview and Point Source Catalog

445 citations · 1.9k across the 43 of their papers we have counts for

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Showing 2004 · astro-phShow all

8 papers · 2 filters

astro-ph2004

X-rays from the First Massive Black Holes

W. N. Brandt, C. Vignali, B. D. Lehmer +3

We briefly review some recent results from Chandra and XMM-Newton studies of the highest redshift (z > 4) active galactic nuclei (AGNs). Specific topics covered include radio-quiet…

astro-ph2004

A Chandra observation of the z=2.285 galaxy FSC10214+4724: Evidence for a Compton-thick quasar?

D. M. Alexander, G. Chartas, F. E. Bauer +3

We present a ~20 ks Chandra ACIS-S observation of the strongly lensed z=2.285 ultra-luminous infrared galaxy FSC10214+4724. Although this observation achieves the equivalent sensit…

astro-ph2004

Obscured accreting black holes at high redshift

A. Comastri, F. Fiore, C. Vignali +2

A significant fraction of the accreting black holes powering high redshift AGN are obscured by large columns of dust and gas. For this reason, luminous type 2 quasars can be effici…

astro-ph2004

Type II quasar candidates in the Sloan Digital Sky Survey: evidence for X-ray obscuration

C. Vignali, D. M. Alexander, A. Comastri

Recent X-ray surveys with Chandra and XMM-Newton have found several genuine Type II quasars, the long sought-after population of high-luminosity (high-redshift) Seyfert 2 galaxies,…

astro-ph2004

XMM-Newton observations of Extremely Red Objects and the link with luminous, X-ray obscured Quasars

M. Brusa, A. Comastri, E. Daddi +8

We present the results of a deep (about 80 ks) XMM-Newton survey of the largest sample of near-infrared selected Extremely Red Objects (R-K>5) available to date to K_S< 19.2. At th…

astro-ph2004

Evidence for X-ray Obscuration in Type II Quasar Candidates from the Sloan Digital Sky Survey

C. Vignali, D. M. Alexander, A. Comastri

Recently, Zakamska et al. (2003) selected 291 high-ionization narrow emission-line AGN in the redshift range 0.3-0.83 from the Sloan Digital Sky Survey spectroscopic data. The samp…