activity
20062025
most citedThe X-ray luminosity function of Active Galactic Nuclei in the redshift interval z=3-5

98 citations · 209 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2025★ 9 cited

The eROSITA Final Equatorial Depth Survey (eFEDS): SDSS spectroscopic observations of X-ray sources

Catarina Aydar, Andrea Merloni, Tom Dwelly +45

We present one of the largest uniform optical spectroscopic surveys of X-ray selected sources to date that were observed as a pilot study for the Black Hole Mapper (BHM) survey. Th…

astro-ph.HE2015★ 98 cited

The X-ray luminosity function of Active Galactic Nuclei in the redshift interval z=3-5

A. Georgakakis, J. Aird, J. Buchner +13

We combine deep X-ray survey data from the Chandra observatory and the wide-area/shallow XMM-XXL field to estimate the AGN X-ray luminosity function in the redshift range z=3-5. Th…

astro-ph.HE2014★ 53 cited

On the Fe K absorption - accretion state connection in the Galactic center neutron star X-ray binary AX J1745.6-2901

G. Ponti, S. Bianchi, T. Munoz-Darias +17

AX J1745.6-2901 is a high-inclination (eclipsing) neutron star Low Mass X-ray Binary (LMXB) located less than ~1.5 arcmin from Sgr A*. Ongoing monitoring campaigns have targeted Sg…

astro-ph.GA2014★ 31 cited

Herschel observations of gamma-ray burst host galaxies: implications for the topology of the dusty interstellar medium

P. Schady, S. Savaglio, T. Mueller +11

Long-duration gamma-ray bursts (GRBs) are indisputably related to star formation, and their vast luminosity in gamma rays pin-points regions of star formation independent of galaxy…

astro-ph.CO2009★ 18 cited

The Comoving Infrared Luminosity Density: Domination of Cold Galaxies across 0<z<1

N. Seymour, M. Symeonidis, M. J. Page +4

In this paper we examine the contribution of galaxies with different infrared (IR) spectral energy distributions (SEDs) to the comoving infrared luminosity density, a proxy for the…

astro-ph2006

The Star-formation History of the Universe as Revealed from Deep Radio Observations of the 13H XMM-Newton/Chandra Deep Field

N. Seymour, T. Dwelly, D. Moss +4

Discerning the exact nature of the faint (sub-mJy) radio population has been historically difficult due to the low luminosity of these sources at most wavelengths. Using deep obser…