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Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 2(420), p. 1481-1494

DOI: 10.1111/j.1365-2966.2011.20135.x

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The importance of the local density in shaping the galaxy stellar mass functions★: Mass functions at different local densities

Journal article published in 2011 by Benedetta Vulcani ORCID, Bianca M. Poggianti, Giovanni Fasano, Vandana Desai, Alan Dressler, August Oemler, Rosa Calvi, Mauro D’Onofrio, Alessia Moretti ORCID
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Abstract

Exploiting the capabilities of four different surveys - the Padova-Millennium Galaxy and Group Catalogue (PM2GC), the WIde-field Nearby Galaxy-cluster Survey (WINGS), the IMACS (Inamori-Magellan Areal Camera and Spectrograph) Cluster Building Survey (ICBS) and the ESO (European Southern Observatory) Distant Cluster Survey (EDisCS) - we analyse the galaxy stellar mass distribution as a function of local density in mass-limited samples, in the field and in clusters from low (z>0.04) to high (z