Serveur d'exploration sur les relations entre la France et l'Australie

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A pilot study for the SCUBA‐2 ‘All‐Sky’ Survey

Identifieur interne : 002752 ( Istex/Curation ); précédent : 002751; suivant : 002753

A pilot study for the SCUBA‐2 ‘All‐Sky’ Survey

Auteurs : Todd Mackenzie [Canada] ; Filiberto G. Braglia [Canada] ; Andy G. Gibb [Canada] ; Douglas Scott [Canada] ; Tim Jenness [États-Unis] ; Stephen Serjeant ; Mark Thompson ; David Berry [États-Unis] ; Christopher M. Brunt ; Edward Chapin [Canada] ; Antonio Chrysostomou [États-Unis] ; Dave Clements ; Kristen Coppin [Canada] ; Frossie Economou [États-Unis] ; A. Evans ; Per Friberg [États-Unis] ; Jane Greaves ; T. Hill [France] ; Wayne Holland [Royaume-Uni] ; R. J. Ivison [Royaume-Uni] ; Johan H. Knapen [Espagne] ; Neal Jackson [Royaume-Uni] ; Gilles Joncas [Canada] ; Larry Morgan ; Angela Mortier ; Chris Pearson [Canada] ; Michele Pestalozzi [Italie] ; Alexandra Pope [États-Unis] ; John Richer [Royaume-Uni] ; J. S. Urquhart [Australie] ; Mattia Vaccari [Italie] ; Bernd Weferling [Allemagne] ; Glenn White ; Ming Zhu [République populaire de Chine]

Source :

RBID : ISTEX:D3AEB0B34F47F7449B9735E70BD8BD35701E7B63

Descripteurs français

English descriptors

Abstract

We have carried out a pilot study for the Submillimetre Common‐User Bolometer Array 2 (SCUBA‐2) ‘All‐Sky’ Survey (SASSy), a wide and shallow mapping project at 850 μm, designed to find rare objects, both Galactic and extragalactic. Two distinct sets of exploratory observations were undertaken and used to test the SASSy approach and data‐reduction pipeline. The first was a 05 × 05 map around the nearby galaxy NGC 2559. The galaxy was easily detected at 156 mJy, but no other convincing sources are present in the map. Comparison with other galaxies with similar wavelength coverage indicates that NGC 2559 has relatively warm dust. The second observations cover 1 deg2 around the W5‐E H ii region. As well as diffuse structure in the map, a filtering approach was able to extract 27 compact sources with signal‐to‐noise ratio greater than 6. By matching with data at other wavelengths we can see that the SCUBA‐2 data can be used to discriminate the colder cores. Together these observations show that the SASSy project will be able to meet its original goals of detecting new bright sources which will be ideal for follow‐up observations with other facilities.

Url:
DOI: 10.1111/j.1365-2966.2011.18840.x

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ISTEX:D3AEB0B34F47F7449B9735E70BD8BD35701E7B63

Curation

No country items

Stephen Serjeant
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Mark Thompson
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Christopher M. Brunt
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Dave Clements
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A. Evans
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Jane Greaves
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Larry Morgan
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Angela Mortier
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Glenn White
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<name sortKey="Richer, John" sort="Richer, John" uniqKey="Richer J" first="John" last="Richer">John Richer</name>
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<name sortKey="Zhu, Ming" sort="Zhu, Ming" uniqKey="Zhu M" first="Ming" last="Zhu">Ming Zhu</name>
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<term>Noise excursions</term>
<term>Noise level</term>
<term>Optical image</term>
<term>Other galaxies</term>
<term>Outer region</term>
<term>Outer regions</term>
<term>Peak values</term>
<term>Physical quantities</term>
<term>Pilot study</term>
<term>Pilot survey</term>
<term>Pixel</term>
<term>Pixel values</term>
<term>Point source</term>
<term>Point sources</term>
<term>Propulsion laboratory</term>
<term>Qpah</term>
<term>Qpah umin umax</term>
<term>Sassy</term>
<term>Scuba</term>
<term>Source catalogue</term>
<term>Spatial noise</term>
<term>Spie</term>
<term>Spitzer</term>
<term>Spitzer contours</term>
<term>Spitzer image</term>
<term>Starlight intensity</term>
<term>Starlink user note</term>
<term>Submillimeter detectors</term>
<term>Submillimetre bolometer array</term>
<term>Submm</term>
<term>Submm wavelengths</term>
<term>Survey figure</term>
<term>Target sensitivity</term>
<term>Upper limit</term>
</keywords>
<keywords scheme="Wicri" type="topic" xml:lang="fr">
<term>Niveau sonore</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">We have carried out a pilot study for the Submillimetre Common‐User Bolometer Array 2 (SCUBA‐2) ‘All‐Sky’ Survey (SASSy), a wide and shallow mapping project at 850 μm, designed to find rare objects, both Galactic and extragalactic. Two distinct sets of exploratory observations were undertaken and used to test the SASSy approach and data‐reduction pipeline. The first was a 05 × 05 map around the nearby galaxy NGC 2559. The galaxy was easily detected at 156 mJy, but no other convincing sources are present in the map. Comparison with other galaxies with similar wavelength coverage indicates that NGC 2559 has relatively warm dust. The second observations cover 1 deg2 around the W5‐E H ii region. As well as diffuse structure in the map, a filtering approach was able to extract 27 compact sources with signal‐to‐noise ratio greater than 6. By matching with data at other wavelengths we can see that the SCUBA‐2 data can be used to discriminate the colder cores. Together these observations show that the SASSy project will be able to meet its original goals of detecting new bright sources which will be ideal for follow‐up observations with other facilities.</div>
</front>
</TEI>
</record>

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