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The evolution of the luminosity function faint end of cluster galaxies in the Cluster-EAGLE simulation

Published online by Cambridge University Press:  30 October 2019

Andrea Negri Open the ORCID record for Andrea Negri [Opens in a new window] ,
Claudio Dalla Vecchia ,
Alfonso Aguerri ,
Yannick Bahé ,
David Barnes  and
Scott Kay
Andrea Negri
Affiliation:
Instituto de Astrofsica de Canarias, C/Va Lactea s/n, E-38205 La Laguna, Tenerife, Spain email: [email protected] Departamento de Astrofsica, Universidad de La Laguna, Av. del Astrofsico Francisco Sanchez s/n, E-38205 La Laguna, Tenerife, Spain
Claudio Dalla Vecchia
Affiliation:
Instituto de Astrofsica de Canarias, C/Va Lactea s/n, E-38205 La Laguna, Tenerife, Spain email: [email protected] Departamento de Astrofsica, Universidad de La Laguna, Av. del Astrofsico Francisco Sanchez s/n, E-38205 La Laguna, Tenerife, Spain
Alfonso Aguerri
Affiliation:
Instituto de Astrofsica de Canarias, C/Va Lactea s/n, E-38205 La Laguna, Tenerife, Spain email: [email protected] Departamento de Astrofsica, Universidad de La Laguna, Av. del Astrofsico Francisco Sanchez s/n, E-38205 La Laguna, Tenerife, Spain
Yannick Bahé
Affiliation:
Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, the Netherlands Max-Planck-Institut fur Astrophysik, Karl-Schwarzschild Str. 1, D-85748 Garching, Germany
David Barnes
Affiliation:
Department of Physics, Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
Scott Kay
Affiliation:
Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
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Abstract

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In the last decade observations have been able to probe the evolution of the galaxy luminosity function, in particular showing a variation of its faint-end with redshift. We employ the data of the Cluster-EAGLE project, a set of cosmological, hydrodynamical zoom-in simulations of 30 galaxy clusters, to study the evolution of the galaxy luminostity functions in clusters with redshift. We compile a catalogue of simulated galaxies’ luminosities in the SDSS bands using the E-MILES spectra database, and taking into account dust attenuation. Stacked luminosity functions present little evolution with redshift of the faint-end slope from z=3.5 to z=0, regardless of the cluster mass.

Keywords

galaxies: evolutiongalaxies: formationgalaxies: dwarfgalaxies: high-redshifmethods: numerical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S344: Dwarf Galaxies: From the Deep Universe to the Present , August 2018 , pp. 495 - 497
Copyright
© International Astronomical Union 2019 

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