activity
20042017
most citedThe Chandra COSMOS Legacy survey: overview and point source catalog

511 citations · 3.4k across the 22 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

13 papers · 1 filter

astro-ph.CO2013★ 1 cited

The Distribution of AGN Covering Factors

Andy Lawrence, Isaac Roseboom, Jack Mayo +4

We review our knowledge of the most basic properties of the AGN obscuring region - its location, scale, symmetry, and mean covering factor - and discuss new evidence on the distrib…

astro-ph.CO2012★ 84 cited

Spectral Energy Distributions of Type 1 AGN in the COSMOS Survey I - The XMM-COSMOS Sample

M. Elvis, H. Hao, F. Civano +39

The "Cosmic Evolution Survey" (COSMOS) enables the study of the Spectral Energy Distributions (SEDs) of Active Galactic Nuclei (AGN) because of the deep coverage and rich sampling…

astro-ph.CO2012★ 255 cited

Accreting SMBHs in the COSMOS field and the connection to their host galaxies

A. Bongiorno, A. Merloni, M. Brusa +22

Using the wide multi-band photometry available in the COSMOS field we explore the host galaxy properties of a large sample of Active Galactic Nuclei (AGN) obtained by combining X-r…

astro-ph.CO2012★ 247 cited

The Chandra COSMOS Survey: III. Optical and Infrared Identification of X-ray Point Sources

F. Civano, M. Elvis, M. Brusa +29

The Chandra COSMOS Survey (C-COSMOS) is a large, 1.8 Ms, Chandra program that has imaged the central 0.9 deg^2 of the COSMOS field down to limiting depths of 1.9 10^-16 erg cm^-2 s…

astro-ph.CO2012★ 70 cited

IR-derived covering factors for a large sample of quasars from WISE-UKIDSS-SDSS

I. G. Roseboom, A. Lawrence, M. Elvis +3

We investigate the range of covering factors (determined from the ratio of IR to UV/optical luminosity) seen in luminous type 1 quasars using a combination of data from the WISE, U…

astro-ph.CO2011★ 183 cited

The impact of galaxy interactions on AGN activity in zCOSMOS

J. D. Silverman, P. Kampczyk, K. Jahnke +52

Close encounters between galaxies are expected to be a viable mechanism, as predicted by numerical simulations, by which accretion onto supermassive black holes can be initiated. T…