HerMES: point source catalogues from deep Herschel-SPIRE observations

A. J. Smith*, L. Wang, S. J. Oliver, R. Auld, J. Bock, D. Brisbin, D. Burgarella, P. Chanial, E. Chapin, D. L. Clements, L. Conversi, A. Cooray, C. D. Dowell, S. Eales, D. Farrah, A. Franceschini, J. Glenn, M. Griffin, R. J. Ivison, A. M. J. MortierM. J. Page, A. Papageorgiou, C. P. Pearson, I. Perez-Fournon, M. Pohlen, J. I. Rawlings, G. Raymond, G. Rodighiero, I. G. Roseboom, M. Rowan-Robinson, R. Savage, Douglas Scott, N. Seymour, M. Symeonidis, K. E. Tugwell, M. Vaccari, I. Valtchanov, L. Vigroux, R. Ward, G. Wright, M. Zemcov

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

We describe the generation of single-band point source catalogues from submillimetre Herschel-SPIRE observations taken as part of the Science Demonstration Phase of the Herschel Multi-tiered Extragalactic Survey (HerMES). Flux densities are found by means of peak finding and the fitting of a Gaussian point-response function. With highly confused images, careful checks must be made on the completeness and flux-density accuracy of the detected sources. This is done by injecting artificial sources into the images and analysing the resulting catalogues. Measured flux densities at which 50 per cent of injected sources result in good detections at (250, 350 and 500) mu m range from (11.6, 13.2 and 13.1) to (25.7, 27.1 and 35.8) mJy, depending on the depth of the observation (where a good detection is taken to be one with positional offset less than one full-width half-maximum of the point-response function, and with the measured flux density within a factor of 2 of the flux density of the injected source). This paper acts as a reference for the 2010 July HerMES public data release.

Original languageEnglish
Pages (from-to)377-389
Number of pages13
JournalMonthly Notices of the Royal Astronomical Society
Volume419
Issue number1
DOIs
Publication statusPublished - Jan 2012

Keywords

  • methods: data analysis
  • catalogues
  • galaxies: photometry
  • submillimetre: galaxies
  • SOURCE EXTRACTION
  • NUMBER COUNTS
  • MU-M
  • INSTRUMENT

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