activity
20072023
most citedGOODS-Herschel: an infrared main sequence for star-forming galaxies

1.1k citations · 9.5k across the 105 of their papers we have counts for

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Showing 2013Show all

8 papers · 1 filter

astro-ph.CO2013★ 58 cited

A wide search for obscured Active Galactic Nuclei using XMM-Newton and WISE

E. Rovilos, I. Georgantopoulos, A. Akylas +8

We use a combination of the XMM-Newton serendipitous X-ray survey with the optical SDSS, and the infrared WISE all-sky survey in order to check the efficiency of the low X-ray to i…

astro-ph.HE2013★ 93 cited

The NuSTAR Extragalactic Survey: A First Sensitive Look at the High-Energy Cosmic X-ray Background Population

D. M. Alexander, D. Stern, A. Del Moro +31

We report on the first ten identifications of sources serendipitously detected by the NuSTAR to provide the first sensitive census of the cosmic X-ray background (CXB) source popul…

astro-ph.CO2013★ 195 cited

A correlation between star formation rate and average black hole accretion in star forming galaxies

Chien-Ting J. Chen, Ryan C. Hickox, Stacey Alberts +14

We present a measurement of the average supermassive black hole accretion rate (BHAR) as a function of star formation rate (SFR) for galaxies in the redshift range 0.25<z<0.8. We s…

astro-ph.CO2013★ 358 cited

Black hole variability and the star formation-AGN connection: Do all star-forming galaxies host an AGN?

Ryan C. Hickox, James R. Mullaney, David M. Alexander +4

We investigate the effect of active galactic nucleus (AGN) variability on the observed connection between star formation and black hole accretion in extragalactic surveys. Recent s…

astro-ph.CO2013★ 1 cited

New insights on the distant AGN population

A. Del Moro, D. M. Alexander, J. R. Mullaney +3

Current X-ray surveys have proved to be essential tools in order to identify and study AGNs across cosmic time. However, there is evidence that the most heavily obscured AGNs are l…

astro-ph.CO2013★ 303 cited

Narrow-line region gas kinematics of 24,264 optically-selected AGN: the radio connection

J. R. Mullaney, D. M. Alexander, S. Fine +3

Using a sample of 24264 optically selected AGNs from the SDSS DR7 database, we characterise how the profile of the [OIII] emission line relates to bolometric luminosity (L_Bol), Ed…