The Herschel Virgo Cluster Survey

J.I. Davies; M. Baes; G.J. Bendo; S. Bianchi; D.J. Bomans; A. Boselli; M. Clemens; E. Corbelli; Luca Cortese; A. Dariush; I. De Looze; S. Di Serego Alighieri; D. Fadda; J. Fritz; D.A. Garcia-Appadoo; G. Gavazzi; C. Giovanardi; M. Grossi; T.M. Hughes; L.K. Hunt; A.P. Jones; S. Madden; D. Pierini; M. Pohlen; S. Sabatini; M.W.L. Smith; J. Verstappen; C. Vlahakis; E.M. Xilouris; S. Zibetti

doi:10.1051/0004-6361/201014571

The Herschel Virgo Cluster Survey

J.I. Davies, M. Baes, G.J. Bendo, S. Bianchi, D.J. Bomans, A. Boselli, M. Clemens, E. Corbelli, Luca Cortese, A. Dariush, I. De Looze, S. Di Serego Alighieri, D. Fadda, J. Fritz, D.A. Garcia-Appadoo, G. Gavazzi, C. Giovanardi, M. Grossi, T.M. Hughes, L.K. HuntA.P. Jones, S. Madden, D. Pierini, M. Pohlen, S. Sabatini, M.W.L. Smith, J. Verstappen, C. Vlahakis, E.M. Xilouris, S. Zibetti

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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	https://doi.org/10.1051/0004-6361/201014571
Publication status	Published - 2010

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Davies, J. I., Baes, M., Bendo, G. J., Bianchi, S., Bomans, D. J., Boselli, A., Clemens, M., Corbelli, E., Cortese, L., Dariush, A., De Looze, I., Di Serego Alighieri, S., Fadda, D., Fritz, J., Garcia-Appadoo, D. A., Gavazzi, G., Giovanardi, C., Grossi, M., Hughes, T. M., ... Zibetti, S. (2010). The Herschel Virgo Cluster Survey. Astronomy and Astrophysics, 518(8), 4. https://doi.org/10.1051/0004-6361/201014571

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title = "The Herschel Virgo Cluster Survey",

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. {\textcopyright} 2010 ESO.",

author = "J.I. Davies and M. Baes and G.J. Bendo and S. Bianchi and D.J. Bomans and A. Boselli and M. Clemens and E. Corbelli and Luca Cortese and A. Dariush and {De Looze}, I. and {Di Serego Alighieri}, S. and D. Fadda and J. Fritz and D.A. Garcia-Appadoo and G. Gavazzi and C. Giovanardi and M. Grossi and T.M. Hughes and L.K. Hunt and A.P. Jones and S. Madden and D. Pierini and M. Pohlen and S. Sabatini and M.W.L. Smith and J. Verstappen and C. Vlahakis and E.M. Xilouris and S. Zibetti",

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doi = "10.1051/0004-6361/201014571",

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Davies, JI, Baes, M, Bendo, GJ, Bianchi, S, Bomans, DJ, Boselli, A, Clemens, M, Corbelli, E, Cortese, L, Dariush, A, De Looze, I, Di Serego Alighieri, S, Fadda, D, Fritz, J, Garcia-Appadoo, DA, Gavazzi, G, Giovanardi, C, Grossi, M, Hughes, TM, Hunt, LK, Jones, AP, Madden, S, Pierini, D, Pohlen, M, Sabatini, S, Smith, MWL, Verstappen, J, Vlahakis, C, Xilouris, EM & Zibetti, S 2010, 'The Herschel Virgo Cluster Survey', Astronomy and Astrophysics, vol. 518, no. 8, pp. 4. https://doi.org/10.1051/0004-6361/201014571

TY - JOUR

T1 - The Herschel Virgo Cluster Survey

AU - Davies, J.I.

AU - Baes, M.

AU - Bendo, G.J.

AU - Bianchi, S.

AU - Bomans, D.J.

AU - Boselli, A.

AU - Clemens, M.

AU - Corbelli, E.

AU - Cortese, Luca

AU - Dariush, A.

AU - De Looze, I.

AU - Di Serego Alighieri, S.

AU - Fadda, D.

AU - Fritz, J.

AU - Garcia-Appadoo, D.A.

AU - Gavazzi, G.

AU - Giovanardi, C.

AU - Grossi, M.

AU - Hughes, T.M.

AU - Hunt, L.K.

AU - Jones, A.P.

AU - Madden, S.

AU - Pierini, D.

AU - Pohlen, M.

AU - Sabatini, S.

AU - Smith, M.W.L.

AU - Verstappen, J.

AU - Vlahakis, C.

AU - Xilouris, E.M.

AU - Zibetti, S.

PY - 2010

Y1 - 2010

N2 - 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.

AB - 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.

U2 - 10.1051/0004-6361/201014571

DO - 10.1051/0004-6361/201014571

M3 - Article

VL - 518

SP - 4

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

IS - 8

ER -

The Herschel Virgo Cluster Survey

Abstract

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