publication . Article . Preprint . 2017

The evolution of active galactic nuclei in clusters of galaxies from the Dark Energy Survey

Bufanda, E.; Hollowood, D.; Jeltema, T. E.; Rykoff, E. S.; Rozo, E.; Martini, P.; Abbott, T. M. C.; Abdalla, F. B.; Allam, S.; Banerji, M.; ...
Open Access English
  • Published: 01 Mar 2017
  • Publisher: Oxford Univ Press
The correlation between active galactic nuclei (AGN) and environment provides important clues to AGN fueling and the relationship of black hole growth to galaxy evolution. In this paper, we analyze the fraction of galaxies in clusters hosting AGN as a function of redshift and cluster richness for X-ray detected AGN associated with clusters of galaxies in Dark Energy Survey (DES) Science Verification data. The present sample includes 33 AGN with L_X > 10^43 ergs s^-1 in non-central, host galaxies with luminosity greater than 0.5 L* from a total sample of 432 clusters in the redshift range of 0.10.7. This result is in good agreement with previous work and parallel...
Persistent Identifiers
arXiv: Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics::High Energy Astrophysical Phenomena
free text keywords: active [galaxies], galaxies [X-rays], galaxies: clusters. [X-rays], X-rays: galaxies, X-rays: galaxies: clusters, galaxies: active, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Galáxias ativas, Nucleo galatico, Aglomerados de galaxias, Deslocamento para o vermelho, Galaxies active, X-rays galaxies, X-rays galaxies clusters, Space and Planetary Science, Astronomy and Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies, QB, astro-ph.HE, astro-ph.GA, galaxies: clusters [X-rays], RCUK, STFC, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Luminous infrared galaxy, Elliptical galaxy, Physics, Brightest cluster galaxy, Galaxy cluster, Astronomy, Galaxy, Active galactic nucleus, Astrophysics, Quasar, Disc galaxy
Funded by
Testing the Dark Energy Paradigm and Measuring Neutrino Mass with the Dark Energy Survey
  • Funder: European Commission (EC)
  • Project Code: 291329
  • Funding stream: FP7 | SP2 | ERC
NSF| Collaborative Research: The Dark Energy Survey Data Management Operations
  • Funder: National Science Foundation (NSF)
  • Project Code: 1138766
  • Funding stream: Directorate for Mathematical & Physical Sciences | Division of Astronomical Sciences
Understanding the Origin of Cosmic Structure
  • Funder: European Commission (EC)
  • Project Code: 306478
  • Funding stream: FP7 | SP2 | ERC
Capitalizing on Gravitational Shear
  • Funder: European Commission (EC)
  • Project Code: 240672
  • Funding stream: FP7 | SP2 | ERC
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