Skip to content Skip to navigation
University of Warwick
  • Study
  • |
  • Research
  • |
  • Business
  • |
  • Alumni
  • |
  • News
  • |
  • About

University of Warwick
Publications service & WRAP

Highlight your research

  • WRAP
    • Home
    • Search WRAP
    • Browse by Warwick Author
    • Browse WRAP by Year
    • Browse WRAP by Subject
    • Browse WRAP by Department
    • Browse WRAP by Funder
    • Browse Theses by Department
  • Publications Service
    • Home
    • Search Publications Service
    • Browse by Warwick Author
    • Browse Publications service by Year
    • Browse Publications service by Subject
    • Browse Publications service by Department
    • Browse Publications service by Funder
  • Statistics
  • Help & Advice
University of Warwick

The Library

  • Login

HerMES : SPIRE galaxy number counts at 250, 350, and 500 μm

Tools
- Tools
+ Tools

Oliver, S. J., Wang, L., Smith, A. J., Altieri, B., Amblard, A., Arumugam, V., Auld, R., Aussel, H., Babbedge, T., Blain, A. W. (Andrew W.) et al.
. (2010) HerMES : SPIRE galaxy number counts at 250, 350, and 500 μm. Astronomy & Astrophysics, Vol.518 (No.L21). ISSN 0004-6361

[img] PDF
WRAP_Savage_7_Hermes_aa14697-10[1].pdf - Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader

Download (268Kb)
Official URL: http://dx.doi.org/10.1051/0004-6361/201014697

Abstract

Emission at far-infrared wavelengths makes up a significant fraction of the total light detected from galaxies over the age of Universe. Herschel provides an opportunity for studying galaxies at the peak wavelength of their emission. Our aim is to provide a benchmark for models of galaxy population evolution and to test pre-existing models of galaxies.With the Herschel Multi-tiered Extra-galactic survey, HerMES, we have observed a number of fields of different areas and sensitivity using the SPIRE instrument on Herschel. We have determined the number counts of galaxies down to ∼20 mJy. Our constraints from directly counting galaxies are consistent with, though more precise than, estimates from the BLAST fluctuation analysis. We have found a steep rise in the Euclidean normalised counts <100 mJy. We have directly resolved ∼15% of the infrared extra-galactic background at the wavelength near where it peaks.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science > Centre for Systems Biology
Library of Congress Subject Headings (LCSH): Galaxies -- Evolution, Galaxies -- Statistics, Infrared astronomy
Journal or Publication Title: Astronomy & Astrophysics
Publisher: EDP Sciences
ISSN: 0004-6361
Date: July 2010
Volume: Vol.518
Number: No.L21
Identification Number: 10.1051/0004-6361/201014697
Status: Peer Reviewed
Access rights to Published version: Open Access
Funder: Science and Technology Facilities Council (Great Britain) (STFC), Canadian Space Agency (CSA), National Astronomical Observatory of China (NAOC), France. Commissariat à l'énergie atomique (CEA), Centre national d'études spatiales (France) (CNES), Centre national de la recherche scientifique (France) (CNRS), Agenzia spaziale italiana [Italian Space Agency] (ASI), Spain. Ministerio de Ciencia e Innovación (MICINN), Rymdstyrelsen [Swedish National Space Board] (SNSB), United States. National Aeronautics and Space Administration (NASA)
Grant number: ST/F002858/1 (STFC)
References: Baugh, C. M., Lacey, C. G., Frenk, C. S., et al. 2005, MNRAS, 356, 1191 Béthermin, M., Dole, H., Cousin, M., & Bavouzet, N. 2010, A&A, 516, A43 Coppin, K., Chapin, E. L., Mortier, A. M. J., et al. 2006, MNRAS, 372, 1621 Crawford, T. M., Switzer, E. R., Holzapfel, W. L., et al. 2009, ApJ, submitted, [arXiv:0912.2341] Fixsen, D. J., Dwek, E.,Mather, J. C., Bennett, C. L., & Shafer, R. A. 1998, ApJ, 508, 123 Franceschini, A., Rodighiero, G., Vaccari, M., Marchetti, L., & Mainetti, G. 2009, A&A, accepted [arXiv:0906.4264] Frayer, D. T., Sanders, D. B., Surace, J. A., et al. 2009, AJ, 138, 1261 Granato, G. L., De Zotti, G., Silva, L., Bressan, A., & Danese, L. 2004, ApJ, 600, 580 Greve, T. R., Pope, A., Scott, D., et al. 2008, MNRAS, 389, 1489 Griffin, M. J., et al. 2010, A&A, 518, L3 Héraudeau, P., Oliver, S., del Burgo, C., et al. 2004, MNRAS, 354, 924 Khan, S. A., Shafer, R. A., Serjeant, S., et al. 2007, ApJ, 665, 973 Lacey, C. G., Baugh, C. M., Frenk, C. S., & Benson, A. J. 2010, MNRAS, submitted Lagache, G., Puget, J., & Gispert, R. 1999, Ap&SS, 269, 263 Lagache, G., Dole, H., Puget, J., et al. 2004, ApJS, 154, 112 Le Borgne, D., Elbaz, D., Ocvirk, P., & Pichon, C. 2009, A&A, 504, 727 Longair, M. S. 1966, MNRAS, 133, 421 Maloney, P. R., Glenn, J., Aguirre, J. E., et al. 2005, ApJ, 635, 1044 Negrello, M., Perrotta, F., González-Nuevo, J., et al. 2007, MNRAS, 377, 1557 Nguyen, H., et al. 2010, A&A, 518, L5 Oliver, S., Mann, R. G., Carballo, R., et al. 2002, MNRAS, 332, 536 Oliver, S. J., Rowan-Robinson, M., & Saunders, W. 1992, MNRAS, 256, 15P Ott, S. 2010, in Astronomical Data Analysis Software and Systems XIX, ed. Y. Mizumoto, K.-I. Morita, & M. Ohishi, ASP Conf. Ser. Patanchon, G., Ade, P. A. R., Bock, J. J., et al. 2009, ApJ, 707, 1750 Pearson, C., & Khan, S. A. 2009, MNRAS, 399, L11 Pilbratt, G. L., et al. 2010, A&A, 518, L1 Puget, J., Abergel, A., Bernard, J., et al. 1996, A&A, 308, L5 Rowan-Robinson, M. 2009, MNRAS, 394, 117 Savage, R. S., & Oliver, S. 2007, ApJ, 661, 1339 Scott, K. S., Yun, M. S., Wilson, G. W., et al. 2010, MNRAS, in press [arXiv:1003.1768] Serjeant, S., & Harrison, D. 2005, MNRAS, 356, 192 Shupe, D. L., Rowan-Robinson, M., Lonsdale, C. J., et al. 2008, AJ, 135, 1050 Sibthorpe, B., Chanial, P., & Griffin, M. J. 2009, A&A, 503, 625 Swinyard, B. M., et al. 2010, A&A, 518, L4 Valiante, E., Lutz, D., Sturm, E., Genzel, R., & Chapin, E. L. 2009, ApJ, 701, 1814 Weiß, A., Kovács, A., Coppin, K., et al. 2009, ApJ, 707, 1201 Wilman, R. J., Jarvis, M. J., Mauch, T., Rawlings, S., & Hickey, S. 2010, MNRAS, accepted [arXiv:1002.1112] Xu, C. K., Lonsdale, C. J., Shupe, D. L., et al. 2003, ApJ, 587, 90
URI: http://wrap.warwick.ac.uk/id/eprint/3416

Request changes to a record

Actions (login required)

View Item View Item

Document Downloads

More statistics for this item...
twitter

Email us: publications@warwick.ac.uk
Contact Details
About Us