The Herschel Virgo Cluster Survey: I. Luminosity functions

A. Boselli; A. Dariush; A. P. Jones; Baes; Bicay; Binggeli; Binggeli; Binggeli; Boehringer; Boselli; Boselli; C. Giovanardi; C. Vlahakis; Clemens; Cortese; D. A. Garcia-Appadoo; D. Fadda; D. J. Bomans; D. Pierini; Davies; De Looze; Doyon; Draine; Dye; E. Corbelli; E. M. Xilouris; Eales; Eales; G. Gavazzi; G. J. Bendo; Gavazzi; Gavazzi; Girardi; Gomez; Griffin; Grossi; Haynes; I. De Looze; J. Fritz; J. I. Davies; J. Verstappen; L. Cortese; L. K. Hunt; Lewis; M. Baes; M. Clemens; M. Grossi; M. Pohlen; M. W. L. Smith; Pilbratt; Poglitsch; Pohlen; Rines; Rowan-Robinson; S. Bianchi; S. di Serego Alighieri; S. Madden; S. Sabatini; S. Zibetti; Smith; Swinyard; T. M. Hughes

research

The Herschel Virgo Cluster Survey: I. Luminosity functions

Abstract

We describe the Herschel Virgo Cluster Survey (HeViCS) and the first data obtained as part of the Science Demonstration Phase (SDP). The data cover a central 4x4 sq deg region of the cluster. We use SPIRE and PACS photometry data to produce 100, 160, 250, 350 and 500 micron luminosity functions (LFs) for optically bright galaxies that are selected at 500 micron and detected in all bands. We compare these LFs with those previously derived using IRAS, BLAST and Herschel-ATLAS data. The Virgo Cluster LFs do not have the large numbers of faint galaxies or examples of very luminous galaxies seen previously in surveys covering less dense environments.Comment: Letter accepted for publication in A&A (Herschel special issue