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The SCUBA HAlf Degree Extragalactic Survey – VI. 350-μm mapping of submillimetre galaxies

Identifieur interne : 000152 ( Main/Exploration ); précédent : 000151; suivant : 000153

The SCUBA HAlf Degree Extragalactic Survey – VI. 350-μm mapping of submillimetre galaxies

Auteurs : Kristen Coppin [Canada, Royaume-Uni] ; Mark Halpern [Canada] ; Douglas Scott [Canada] ; Colin Borys [Canada] ; James Dunlop ; Loretta Dunne ; Rob Ivison ; Jeff Wagg [États-Unis, Mexique] ; Itziar Aretxaga [Mexique] ; Elia Battistelli [Canada] ; Andrew Benson [États-Unis] ; Andrew Blain [États-Unis] ; Scott Chapman [États-Unis] ; Dave Clements ; Simon Dye ; Duncan Farrah [États-Unis] ; David Hughes [Mexique] ; Tim Jenness [États-Unis] ; Eelco Van Kampen [Autriche] ; Cedric Lacey ; Angela Mortier ; Alexandra Pope [Canada] ; Robert Priddey ; Stephen Serjeant ; Ian Smail ; Jason Stevens ; Mattia Vaccari [Italie]

Source :

RBID : ISTEX:686F3D9D39250268692A10BF27632C25218497FD

Abstract

A follow-up survey using the Submillimetre High-Angular Resolution Camera (SHARC-II) at 350 μm has been carried out to map the regions around several 850-μm-selected sources from the Submillimetre HAlf Degree Extragalactic Survey (SHADES). These observations probe the infrared (IR) luminosities and hence star formation rates in the largest existing, most robust sample of submillimetre galaxies (SMGs). We measure 350-μm flux densities for 24 850-μm sources, seven of which are detected at ≥2.5σ within a 10 arcsec search radius of the 850-μm positions. When results from the literature are included the total number of 350-μm flux density constraints of SHADES SMGs is 31, with 15 detections. We fit a modified blackbody to the far-IR (FIR) photometry of each SMG, and confirm that typical SMGs are dust-rich (Mdust≃ 9 × 108M⊙), luminous (LFIR≃ 2 × 1012L⊙) star-forming galaxies with intrinsic dust temperatures of ≃35 K and star formation rates of ≃400 M⊙ yr−1. We have measured the temperature distribution of SMGs and find that the underlying distribution is slightly broader than implied by the error bars, and that most SMGs are at 28 K with a few hotter. We also place new constraints on the 350-μm source counts, N350(>25 mJy) ∼ 200–500 deg−2.

Url:
DOI: 10.1111/j.1365-2966.2007.12808.x


Affiliations:


Links toward previous steps (curation, corpus...)


Le document en format XML

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<div type="abstract">A follow-up survey using the Submillimetre High-Angular Resolution Camera (SHARC-II) at 350 μm has been carried out to map the regions around several 850-μm-selected sources from the Submillimetre HAlf Degree Extragalactic Survey (SHADES). These observations probe the infrared (IR) luminosities and hence star formation rates in the largest existing, most robust sample of submillimetre galaxies (SMGs). We measure 350-μm flux densities for 24 850-μm sources, seven of which are detected at ≥2.5σ within a 10 arcsec search radius of the 850-μm positions. When results from the literature are included the total number of 350-μm flux density constraints of SHADES SMGs is 31, with 15 detections. We fit a modified blackbody to the far-IR (FIR) photometry of each SMG, and confirm that typical SMGs are dust-rich (Mdust≃ 9 × 108M⊙), luminous (LFIR≃ 2 × 1012L⊙) star-forming galaxies with intrinsic dust temperatures of ≃35 K and star formation rates of ≃400 M⊙ yr−1. We have measured the temperature distribution of SMGs and find that the underlying distribution is slightly broader than implied by the error bars, and that most SMGs are at 28 K with a few hotter. We also place new constraints on the 350-μm source counts, N350(>25 mJy) ∼ 200–500 deg−2.</div>
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