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    Herschel-ATLAS: first data release of the Science Demonstration Phase source catalogues

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    Herschel-ATLASFirstD ... (4.775Mb)
    Identificadores
    URI: https://hdl.handle.net/10902/28441
    DOI: 10.1111/j.1365-2966.2011.18864.x
    ISSN: 0035-8711
    ISSN: 1365-2966
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    Autoría
    Rigby, E. E.; Maddox, S. J.; Dunne, L.; Negrello, M.; Smith, D. J. B.; Gonzalez-Nuevo, J.; Herranz Muñoz, DiegoAutoridad Unican; López-Caniego Alcarria, Marcos; Auld, R.; Buttiglione, S.; Baes, M.; Cava, A.; Cooray, A.; Clements, D. L.; Dariush, A.; De Zotti, G.; Dye, S.; Eales, S.; Frayer, D.; [et al.]
    Fecha
    2011-08
    Derechos
    This article has been accepted for publication in Monthly notices of the Royal Astronomical Society © 2011 The authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
    Publicado en
    Monthly Notices of the Royal Astronomical Society, 2011, 415(3), 2336-2348
    Editorial
    Oxford University Press
    Enlace a la publicación
    https://doi.org/10.1111/j.1365-2966.2011.18864.x
    Palabras clave
    Methods: data analysis
    Catalogues
    Surveys
    Galaxies: general
    Submillimetre: galaxies
    Resumen/Abstract
    The Herschel Astrophysical Terahertz Large Area Survey (Herschel-ATLAS) is a survey of 550 deg2 with the Herschel Space Observatory in five far-infrared and submillimetre bands. The first data for the survey, observations of a field 4 × 4 deg2 in size, were taken during the Science Demonstration Phase (SDP), and reach a 5? noise level of 33.5 mJy beam?1 at 250 µm. This paper describes the source extraction methods used to create the corresponding SDP catalogue, which contains 6876 sources, selected at 250 µm, within ?14 deg2. Spectral and Photometric Imaging REciever (SPIRE) sources are extracted using a new method specifically developed for Herschel data and Photodetector Array Camera and Spectrometer (PACS) counterparts of these sources are identified using circular apertures placed at the SPIRE positions. Aperture flux densities are measured for sources identified as extended after matching to optical wavelengths. The reliability of this catalogue is also discussed, using full simulated maps at the three SPIRE bands. These show that a significant number of sources at 350 and 500 µm have undergone flux density enhancements of up to a factor of ?2, due mainly to source confusion. Correction factors are determined for these effects. The SDP data set and corresponding catalogue will be available from www.h-atlas.org.
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    UNIVERSIDAD DE CANTABRIA

    Repositorio realizado por la Biblioteca Universitaria utilizando DSpace software
    Contacto | Sugerencias
    Metadatos sujetos a:licencia de Creative Commons Reconocimiento 4.0 España