HerMES: point source catalogues from deep Herschel-SPIRE observations★

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.

[1]  D. Elbaz,et al.  The Herschel Multi-Tiered Extragalactic Survey: source extraction and cross-identifications in confusion-dominated SPIRE images , 2010, 1009.1658.

[2]  S. Ott,et al.  Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy , 2010, 1005.5331.

[3]  S. J. Liu,et al.  Herschel : the first science highlights Special feature L etter to the E ditor The Herschel-SPIRE instrument and its in-flight performance , 2010 .

[4]  H. Roussel,et al.  In-flight calibration of the Herschel-SPIRE instrument , 2010, 1005.5073.

[5]  D. Elbaz,et al.  HerMES: The submillimeter spectral energy distributions of Herschel/SPIRE-detected galaxies , 2010, 1005.2396.

[6]  D. Elbaz,et al.  HerMES: The SPIRE confusion limit , 2010, 1005.2207.

[7]  D. Elbaz,et al.  HerMES: SPIRE galaxy number counts at 250, 350, and 500 μm , 2010, 1005.2184.

[8]  J. Dunlop,et al.  A joint analysis of BLAST 250–500 μm and LABOCA 870 μm observations in the Extended Chandra Deep Field-South , 2010, 1003.2647.

[9]  Robert Mann,et al.  Astronomical Data Analysis Software and Systems XXI , 2012 .

[10]  James J. Bock,et al.  SUBMILLIMETER NUMBER COUNTS FROM STATISTICAL ANALYSIS OF BLAST MAPS , 2009, 0906.0981.

[11]  S. Oliver,et al.  Bayesian Methods of Astronomical Source Extraction , 2005, astro-ph/0512597.

[12]  Jasper V. Wall,et al.  Practical Statistics for Astronomers , 2003 .

[13]  C. Bennett,et al.  The Spectrum of the Extragalactic Far-Infrared Background from the COBE FIRAS Observations , 1998, astro-ph/9803021.

[14]  E. L. Wright,et al.  The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background. IV. Cosmological Implications , 1997, astro-ph/9806129.

[15]  N. Wiener Resume of Fundamental Mathematical Notions , 1949 .