Antonis Georgakakis

Affiliations: 
1998 Imperial College, London, London, England, United Kingdom 
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"Antonis Georgakakis"
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Publications

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Georgakakis A, Ruiz A, LaMassa SM. (2020) Forward modeling the multiwavelength properties of Active Galactic Nuclei: application to X-ray and WISE mid-infrared samples Monthly Notices of the Royal Astronomical Society
Comparat J, Merloni A, Dwelly T, et al. (2020) The final SDSS-IV/SPIDERS X-ray point source spectroscopic catalogue Astronomy and Astrophysics. 636
LaMassa SM, Georgakakis A, Vivek M, et al. (2019) SDSS-IV eBOSS Spectroscopy of X-Ray and WISE AGNs in Stripe 82X: Overview of the Demographics of X-Ray- and Mid-infrared-selected Active Galactic Nuclei The Astrophysical Journal. 876: 50
Aird J, Coil AL, Georgakakis A. (2019) X-rays across the galaxy population – III. The incidence of AGN as a function of star formation rate Monthly Notices of the Royal Astronomical Society. 484: 4360-4378
Georgakakis A, Comparat J, Merloni A, et al. (2019) Exploring the halo occupation of AGN using dark-matter cosmological simulations Monthly Notices of the Royal Astronomical Society. 487: 275-295
Kocevski DD, Hasinger G, Brightman M, et al. (2018) X-UDS: The Chandra Legacy Survey of the UKIDSS Ultra Deep Survey Field Astrophysical Journal Supplement Series. 236: 48
Koutoulidis L, Georgantopoulos I, Mountrichas G, et al. (2018) Dependence of clustering of X-ray AGN on obscuration Monthly Notices of the Royal Astronomical Society. 481: 3063-3069
McLure RJ, Pentericci L, Cimatti A, et al. (2018) The VANDELS ESO public spectroscopic survey Monthly Notices of the Royal Astronomical Society. 479: 25-42
Aird J, Coil AL, Georgakakis A. (2018) X-rays across the galaxy population - II. The distribution of AGN accretion rates as a function of stellar mass and redshift Monthly Notices of the Royal Astronomical Society. 474: 1225-1249
Kocevski DD, Barro G, Faber SM, et al. (2017) CANDELS: Elevated Black Hole Growth in the Progenitors of Compact Quiescent Galaxies atz∼ 2 The Astrophysical Journal. 846: 112
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