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 4 × 4 sq deg region of the cluster. We use SPIRE and PACS photometry data to produce 100, 160, 250, 350 and 500 μ m luminosity functions (LFs) for optically bright galaxies that are selected at 500 μ m 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. © 2010 ESO.
Original language | English |
---|---|
Pages (from-to) | 4 |
Journal | Astronomy and Astrophysics |
Volume | 518 |
Issue number | 8 |
DOIs | |
Publication status | Published - 2010 |