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The Herschel Virgo Cluster survey, I : luminosity function

JI Davies, Maarten Baes UGent, GJ Bendo, S Bianchi, DJ Bomans, A Boselli, M Clemens, E Corbelli, L Cortese, A Dariush, et al. (2010) ASTRONOMY & ASTROPHYSICS. 518.
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 x 4 sq deg region of the cluster. We use SPIRE and PACS photometry data to produce 100, 160, 250, 350 and 500 mu m luminosity functions (LFs) for optically bright galaxies that are selected at 500 mu 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.
Please use this url to cite or link to this publication:
author
organization
year
type
journalArticle (original)
publication status
published
subject
keyword
extinction, REDSHIFT SURVEY, dust, galaxies: clusters: individual: Virgo, galaxies: evolution, DIGITAL SKY SURVEY, GALAXY STAR-FORMATION
journal title
ASTRONOMY & ASTROPHYSICS
Astron. Astrophys.
volume
518
article number
L48
pages
4 pages
Web of Science type
Article
Web of Science id
000281527200049
JCR category
ASTRONOMY & ASTROPHYSICS
JCR impact factor
4.41 (2010)
JCR rank
10/54 (2010)
JCR quartile
1 (2010)
ISSN
0004-6361
DOI
10.1051/0004-6361/201014571
language
English
UGent publication?
yes
classification
A1
copyright statement
I have transferred the copyright for this publication to the publisher
id
1236583
handle
http://hdl.handle.net/1854/LU-1236583
date created
2011-05-25 11:24:22
date last changed
2018-06-22 08:27:26
@article{1236583,
  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 x 4 sq deg region of the cluster. We use SPIRE and PACS photometry data to produce 100, 160, 250, 350 and 500 mu m luminosity functions (LFs) for optically bright galaxies that are selected at 500 mu 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.},
  articleno    = {L48},
  author       = {Davies, JI and Baes, Maarten and Bendo, GJ and Bianchi, S and Bomans, DJ and Boselli, A and Clemens, M and Corbelli, E and Cortese, L and Dariush, A and De Looze, Ilse and Alighieri, SD and Fadda, D and Fritz, Jacopo and Garcia-Appadoo, DA and Gavazzi, G and Giovanardi, C and Grossi, M and Hughes, TM and Hunt, LK and Jones, AP and Madden, S and Pierini, D and Pohlen, M and Sabatini, S and Smith, MWL and Verstappen, Joris and Vlahakis, C and Xilouris, EM and Zibetti, S},
  issn         = {0004-6361},
  journal      = {ASTRONOMY \& ASTROPHYSICS},
  keyword      = {extinction,REDSHIFT SURVEY,dust,galaxies: clusters: individual: Virgo,galaxies: evolution,DIGITAL SKY SURVEY,GALAXY STAR-FORMATION},
  language     = {eng},
  pages        = {4},
  title        = {The Herschel Virgo Cluster survey, I : luminosity function},
  url          = {http://dx.doi.org/10.1051/0004-6361/201014571},
  volume       = {518},
  year         = {2010},
}

Chicago
Davies, JI, Maarten Baes, GJ Bendo, S Bianchi, DJ Bomans, A Boselli, M Clemens, et al. 2010. “The Herschel Virgo Cluster Survey, I : Luminosity Function.” Astronomy & Astrophysics 518.
APA
Davies, JI, Baes, M., Bendo, G., Bianchi, S., Bomans, D., Boselli, A., Clemens, M., et al. (2010). The Herschel Virgo Cluster survey, I : luminosity function. ASTRONOMY & ASTROPHYSICS, 518.
Vancouver
1.
Davies J, Baes M, Bendo G, Bianchi S, Bomans D, Boselli A, et al. The Herschel Virgo Cluster survey, I : luminosity function. ASTRONOMY & ASTROPHYSICS. 2010;518.
MLA
Davies, JI, Maarten Baes, GJ Bendo, et al. “The Herschel Virgo Cluster Survey, I : Luminosity Function.” ASTRONOMY & ASTROPHYSICS 518 (2010): n. pag. Print.