activity
20022020
most citedThe 2-10 keV luminosity as a Star Formation Rate indicator

589 citations · 6.1k across the 72 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

14 papers · 1 filter

astro-ph.HE2020★ 10 cited

The hot interstellar medium towards 4U 1820-30: a Bayesian analysis

Daniele Rogantini, Elisa Costantini, Missagh Mehdipour +3

High ionisation lines in the soft X-ray band are generally associated to either interstellar hot gas along the line of sight or to photoionised gas intrinsic to the source. In the…

astro-ph.HE2019★ 8 cited

Compton-thick active galactic nuclei from the 7 Ms observation in the Chandra Deep Field South

A. Corral, I. Georgantopoulos, A. Akylas +1

We present the X-ray spectroscopic study of the Compton-thick (CT) active galactic nuclei (AGN) population within the Deep Field South (CDF-S) by using the deepe…

astro-ph.HE2017★ 7 cited

The XMM deep survey in the CDF-S. X. X-ray variability of bright sources

S. Falocco, M. Paolillo, A. Comastri +6

We aim to study the variability properties of bright hard X-ray selected Active Galactic Nuclei (AGN) with redshift between 0.3 and 1.6 detected in the Chandra Deep Field South (XM…

astro-ph.HE2017★ 91 cited

A New, Faint Population of X-ray Transients

F. E. Bauer, E. Treister, K. Schawinski +22

We report on the detection of a remarkable new fast high-energy transient found in the Chandra Deep Field-South, robustly associated with a faint ( mag, $z_{\rm ph}…

astro-ph.HE2015★ 25 cited

The 2-10 keV unabsorbed luminosity function of AGN from the XMM-Newton LSS, CDFS and COSMOS surveys

P. Ranalli, E. Koulouridis, I. Georgantopoulos +15

The XMM-LSS, XMM-COSMOS, and XMM-CDFS surveys are complementary in terms of sky coverage and depth. Together, they form a clean sample with the least possible variance in instrumen…

astro-ph.HE2014★ 18 cited

Searching for highly obscured AGN in the XMM-Newton serendipitous source catalog

A. Corral, I. Georgantopoulos, M. G. Watson +9

The majority of active galactic nuclei (AGN) are obscured by large amounts of absorbing material that makes them invisible at many wavelengths. X-rays, given their penetrating powe…