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19972025
most citedThe Chandra Deep Field-South Survey: 7 Ms Source Catalogs

534 citations · 5.5k across the 161 of their papers we have counts for

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Showing 2009 · astro-ph.COShow all

6 papers · 2 filters

astro-ph.CO2009

AGN unified scheme and evolution: a Suzaku view

A. Comastri, K. Iwasawa, R. Gilli +2

We present broad band Suzaku}observations of a small sample of hard X-ray selected (> 10 keV), nearby Seyfert 2 galaxies and discuss the results in the context of AGN unified model…

astro-ph.CO2009★ 2 cited

The gravitationally lensed, luminous infrared galaxy IRAS F10214+4724 observed with XMM-Newton

K. Iwasawa, C. Vignali, A. S. Evans +2

We report on a short XMM-Newton observation of the gravitationally-lensed, luminous infrared galaxy IRAS F10214+4724 at z=2.3. A faint X-ray source is detected at 4 sigma. The obse…

astro-ph.CO2009★ 445 cited

The Chandra COSMOS Survey, I: Overview and Point Source Catalog

Martin Elvis, Francesca Civano, Cristian Vignali +40

The Chandra COSMOS Survey (C-COSMOS) is a large, 1.8 Ms, Chandra} program that has imaged the central 0.5 sq.deg of the COSMOS field (centered at 10h, +02deg) with an effective exp…

astro-ph.CO2009★ 6 cited

The Growth of Supermassive Black Holes Across Cosmic Time

K. Nandra, J. A. Aird, D. M. Alexander +54

One of the main themes in extragalactic astronomy for the next decade will be the evolution of galaxies over cosmic time. Many future observatories, including JWST, ALMA, GMT, TMT…

astro-ph.CO2009★ 1 cited

Multi-wavelength data handling in current and future surveys: the possible role of Virtual Observatory

C. Vignali, F. Fiore, A. Comastri +5

Here we review some of the main issues related to multi-wavelength source identification and characterization, with particular emphasis on the field of X-ray surveys carried out ov…

astro-ph.CO2009★ 75 cited

Revealing X-ray obscured quasars in SWIRE sources with extreme mid-IR/optical flux ratios

G. Lanzuisi, E. Piconcelli, F. Fiore +4

Recent works have suggested that selection criteria based on MIR colors can be used to reveal a population of dust-enshrouded, extremely luminous quasars at z>1. However the X-ray…