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 : 006513 ( Main/Curation ); précédent : 006512; suivant : 006514

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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Links to Exploration step

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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<region type="région" nuts="1">Angleterre de l'Est</region>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Urquhart, J S" sort="Urquhart, J S" uniqKey="Urquhart J" first="J. S." last="Urquhart">J. S. Urquhart</name>
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<country xml:lang="fr">Australie</country>
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</affiliation>
</author>
<author>
<name sortKey="Vaccari, Mattia" sort="Vaccari, Mattia" uniqKey="Vaccari M" first="Mattia" last="Vaccari">Mattia Vaccari</name>
<affiliation wicri:level="1">
<country xml:lang="fr">Italie</country>
<wicri:regionArea>Department of Astronomy, University of Padova, Vicolo Osservatorio 3, I‐35122 Padova</wicri:regionArea>
<wicri:noRegion>I‐35122 Padova</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Weferling, Bernd" sort="Weferling, Bernd" uniqKey="Weferling B" first="Bernd" last="Weferling">Bernd Weferling</name>
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<country xml:lang="fr">Allemagne</country>
<wicri:regionArea>University Bamberg, Markusplatz 3, 96045 Bamberg</wicri:regionArea>
<wicri:noRegion>96045 Bamberg</wicri:noRegion>
<wicri:noRegion>96045 Bamberg</wicri:noRegion>
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</author>
<author>
<name sortKey="White, Glenn" sort="White, Glenn" uniqKey="White G" first="Glenn" last="White">Glenn White</name>
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<wicri:noCountry code="subField">0QX</wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Zhu, Ming" sort="Zhu, Ming" uniqKey="Zhu M" first="Ming" last="Zhu">Ming Zhu</name>
<affiliation wicri:level="3">
<country xml:lang="fr">République populaire de Chine</country>
<wicri:regionArea>National Astronomical Observatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing</wicri:regionArea>
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<settlement type="city">Pékin</settlement>
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<series>
<title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title>
<title level="j" type="alt">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</title>
<idno type="ISSN">0035-8711</idno>
<idno type="eISSN">1365-2966</idno>
<imprint>
<biblScope unit="vol">415</biblScope>
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<date type="published" when="2011-08-01">2011-08-01</date>
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<idno type="ISSN">0035-8711</idno>
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<idno type="ISSN">0035-8711</idno>
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<term>Akari</term>
<term>Ancillary data</term>
<term>Approximate centre</term>
<term>Arcsec</term>
<term>Astrophysics group</term>
<term>Average integration time</term>
<term>Background subtraction</term>
<term>Blackbody</term>
<term>Blackbody spectrum</term>
<term>Blackford hill</term>
<term>Brightest source</term>
<term>California institute</term>
<term>Candidate sources</term>
<term>Cent uncorrelated uncertainty</term>
<term>Central portion</term>
<term>Centre</term>
<term>Chapin</term>
<term>Cold core</term>
<term>Cold source</term>
<term>Colour scale ranges</term>
<term>Compact sources</term>
<term>Data reduction</term>
<term>Different choices</term>
<term>Diffuse structure</term>
<term>Draine</term>
<term>Dust emissivity index</term>
<term>Dust mass</term>
<term>Dust models</term>
<term>Excellent agreement</term>
<term>Extragalactic</term>
<term>Extragalactic observations</term>
<term>Extragalactic sources</term>
<term>Free parameter</term>
<term>Galactic</term>
<term>Galactic cirrus</term>
<term>Galactic plane</term>
<term>Galaxies</term>
<term>Galaxy</term>
<term>HII regions</term>
<term>Histogram</term>
<term>Hydrogen atom</term>
<term>Ira</term>
<term>Iras data</term>
<term>James clerk maxwell telescope</term>
<term>Jenness</term>
<term>Karr martin</term>
<term>Large maps</term>
<term>Lter</term>
<term>Mnras</term>
<term>Monthly notices</term>
<term>National research council</term>
<term>Nearby galaxy</term>
<term>Next section</term>
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<term>Noise level</term>
<term>Optical image</term>
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<term>Outer region</term>
<term>Outer regions</term>
<term>Peak values</term>
<term>Physical quantities</term>
<term>Pilot study</term>
<term>Pilot survey</term>
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<term>Point sources</term>
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<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>
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<term>Submm wavelengths</term>
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<term>Etude ciel</term>
<term>Galaxies</term>
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<term>Région HII</term>
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<term>Akari</term>
<term>Ancillary data</term>
<term>Approximate centre</term>
<term>Arcsec</term>
<term>Astrophysics group</term>
<term>Average integration time</term>
<term>Background subtraction</term>
<term>Blackbody</term>
<term>Blackbody spectrum</term>
<term>Blackford hill</term>
<term>Brightest source</term>
<term>California institute</term>
<term>Candidate sources</term>
<term>Cent uncorrelated uncertainty</term>
<term>Central portion</term>
<term>Centre</term>
<term>Chapin</term>
<term>Cold core</term>
<term>Cold source</term>
<term>Colour scale ranges</term>
<term>Compact sources</term>
<term>Different choices</term>
<term>Diffuse structure</term>
<term>Draine</term>
<term>Dust emissivity index</term>
<term>Dust mass</term>
<term>Dust models</term>
<term>Excellent agreement</term>
<term>Extragalactic</term>
<term>Extragalactic observations</term>
<term>Extragalactic sources</term>
<term>Free parameter</term>
<term>Galactic</term>
<term>Galactic cirrus</term>
<term>Galactic plane</term>
<term>Galaxy</term>
<term>Histogram</term>
<term>Hydrogen atom</term>
<term>Ira</term>
<term>Iras data</term>
<term>James clerk maxwell telescope</term>
<term>Jenness</term>
<term>Karr martin</term>
<term>Large maps</term>
<term>Lter</term>
<term>Mnras</term>
<term>Monthly notices</term>
<term>National research council</term>
<term>Nearby galaxy</term>
<term>Next section</term>
<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>
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<term>Target sensitivity</term>
<term>Upper limit</term>
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<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>
<double idat="0035-8711:2011:Mackenzie T:a:pilot:study">
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<title xml:lang="en" level="a">A pilot study for the SCUBA-2 'All-Sky' Survey</title>
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<name sortKey="Mackenzie, Todd" sort="Mackenzie, Todd" uniqKey="Mackenzie T" first="Todd" last="Mackenzie">Todd Mackenzie</name>
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<s1>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road</s1>
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<country>Canada</country>
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<name sortKey="Braglia, Filiberto G" sort="Braglia, Filiberto G" uniqKey="Braglia F" first="Filiberto G." last="Braglia">Filiberto G. Braglia</name>
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<s1>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road</s1>
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<name sortKey="Scott, Douglas" sort="Scott, Douglas" uniqKey="Scott D" first="Douglas" last="Scott">Douglas Scott</name>
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<s1>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road</s1>
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<country>Canada</country>
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<name sortKey="Jenness, Tim" sort="Jenness, Tim" uniqKey="Jenness T" first="Tim" last="Jenness">Tim Jenness</name>
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<s1>Joint Astronomy Centre, 660 North A'ohoku Place</s1>
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<country>États-Unis</country>
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<name sortKey="Serjeant, Stephen" sort="Serjeant, Stephen" uniqKey="Serjeant S" first="Stephen" last="Serjeant">Stephen Serjeant</name>
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<s1>Department of Physics and Astronomy, The Open University</s1>
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<country>Royaume-Uni</country>
<wicri:noRegion>Milton Keynes MK7 6BJ</wicri:noRegion>
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<author>
<name sortKey="Thompson, Mark" sort="Thompson, Mark" uniqKey="Thompson M" first="Mark" last="Thompson">Mark Thompson</name>
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<s1>Centre for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, College Lane</s1>
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<country>Royaume-Uni</country>
<wicri:noRegion>Hatfield AL10 9AB</wicri:noRegion>
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<author>
<name sortKey="Berry, David" sort="Berry, David" uniqKey="Berry D" first="David" last="Berry">David Berry</name>
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<inist:fA14 i1="02">
<s1>Joint Astronomy Centre, 660 North A'ohoku Place</s1>
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<country>États-Unis</country>
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</affiliation>
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<author>
<name sortKey="Brunt, Christopher M" sort="Brunt, Christopher M" uniqKey="Brunt C" first="Christopher M." last="Brunt">Christopher M. Brunt</name>
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<s1>School of Physics, Stocker Road</s1>
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<country>Royaume-Uni</country>
<wicri:noRegion>Exeter EX4 4QL</wicri:noRegion>
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</author>
<author>
<name sortKey="Chapin, Edward" sort="Chapin, Edward" uniqKey="Chapin E" first="Edward" last="Chapin">Edward Chapin</name>
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<s1>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road</s1>
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<country>Canada</country>
<wicri:noRegion>Vancouver, BC V6T 1Z1</wicri:noRegion>
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</author>
<author>
<name sortKey="Chrysostomou, Antonio" sort="Chrysostomou, Antonio" uniqKey="Chrysostomou A" first="Antonio" last="Chrysostomou">Antonio Chrysostomou</name>
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<s1>Joint Astronomy Centre, 660 North A'ohoku Place</s1>
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<country>États-Unis</country>
<wicri:noRegion>Hilo, HI 96720</wicri:noRegion>
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</author>
<author>
<name sortKey="Clements, Dave" sort="Clements, Dave" uniqKey="Clements D" first="Dave" last="Clements">Dave Clements</name>
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<inist:fA14 i1="06">
<s1>Imperial College London, South Kensington Campus</s1>
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<country>Royaume-Uni</country>
<wicri:noRegion>London SW7 2AZ</wicri:noRegion>
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</author>
<author>
<name sortKey="Coppin, Kristen" sort="Coppin, Kristen" uniqKey="Coppin K" first="Kristen" last="Coppin">Kristen Coppin</name>
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<inist:fA14 i1="07">
<s1>Department of Physics, McGill University, 3600 rue University</s1>
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</inist:fA14>
<country>Canada</country>
<wicri:noRegion>Montreal, QC H3A 2T8</wicri:noRegion>
<orgName type="university">Université McGill</orgName>
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<settlement type="city">Montréal</settlement>
<region type="state">Québec</region>
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<s1>Institute for Computational Cosmology, Durham University, South Road</s1>
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<country>Royaume-Uni</country>
<wicri:noRegion>Durham DH1 3LE</wicri:noRegion>
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<author>
<name sortKey="Economou, Frossie" sort="Economou, Frossie" uniqKey="Economou F" first="Frossie" last="Economou">Frossie Economou</name>
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<inist:fA14 i1="02">
<s1>Joint Astronomy Centre, 660 North A'ohoku Place</s1>
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<sZ>5 aut.</sZ>
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<country>États-Unis</country>
<wicri:noRegion>Hilo, HI 96720</wicri:noRegion>
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<author>
<name sortKey="Evans, A" sort="Evans, A" uniqKey="Evans A" first="A." last="Evans">A. Evans</name>
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<inist:fA14 i1="09">
<s1>Astrophysics Group, Keele University</s1>
<s2>Keele, Staffordshire ST5 5BG</s2>
<s3>GBR</s3>
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<country>Royaume-Uni</country>
<wicri:noRegion>Keele, Staffordshire ST5 5BG</wicri:noRegion>
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<author>
<name sortKey="Friberg, Per" sort="Friberg, Per" uniqKey="Friberg P" first="Per" last="Friberg">Per Friberg</name>
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<inist:fA14 i1="02">
<s1>Joint Astronomy Centre, 660 North A'ohoku Place</s1>
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<sZ>8 aut.</sZ>
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<country>États-Unis</country>
<wicri:noRegion>Hilo, HI 96720</wicri:noRegion>
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</author>
<author>
<name sortKey="Greaves, Jane" sort="Greaves, Jane" uniqKey="Greaves J" first="Jane" last="Greaves">Jane Greaves</name>
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<inist:fA14 i1="10">
<s1>School of Physics and Astronomy, University of St Andrews, North Haugh</s1>
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<sZ>17 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>St Andrews KY16 9SS</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Hill, T" sort="Hill, T" uniqKey="Hill T" first="T." last="Hill">T. Hill</name>
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<inist:fA14 i1="11">
<s1>Laboratoire AIM, CEA/IRFU - CNRS/INSU - Université Paris Diderot, CEA-Saclay</s1>
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<s3>FRA</s3>
<sZ>18 aut.</sZ>
</inist:fA14>
<country>France</country>
<wicri:noRegion>91191 Gif-sur-Yvette</wicri:noRegion>
<wicri:noRegion>CEA-Saclay</wicri:noRegion>
<wicri:noRegion>91191 Gif-sur-Yvette</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Holland, Wayne" sort="Holland, Wayne" uniqKey="Holland W" first="Wayne" last="Holland">Wayne Holland</name>
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<inist:fA14 i1="12">
<s1>UK Astronomy Technology Centre, Royal Observatory, Blackford Hill</s1>
<s2>Edinburgh EH9 3HJ</s2>
<s3>GBR</s3>
<sZ>19 aut.</sZ>
<sZ>20 aut.</sZ>
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<country>Royaume-Uni</country>
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<s1>Joint Astronomy Centre, 660 North A'ohoku Place</s1>
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<s1>School of Physics, Stocker Road</s1>
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<name sortKey="Mortier, Angela" sort="Mortier, Angela" uniqKey="Mortier A" first="Angela" last="Mortier">Angela Mortier</name>
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<s1>Imperial College London, South Kensington Campus</s1>
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<wicri:noRegion>London SW7 2AZ</wicri:noRegion>
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<s1>RAL Space, Rutherford Appleton Laboratory, Chilton</s1>
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<affiliation wicri:level="1">
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<s1>Institute for Space Imaging Science, University of Lethbridge</s1>
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<country>Canada</country>
<wicri:noRegion>Lethbridge, Alberta T1K 3M4</wicri:noRegion>
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<name sortKey="Pestalozzi, Michele" sort="Pestalozzi, Michele" uniqKey="Pestalozzi M" first="Michele" last="Pestalozzi">Michele Pestalozzi</name>
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<s1>IFSI/INAF, via del Fosso del Cavaliere 100</s1>
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<country>Italie</country>
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<settlement type="city">Rome</settlement>
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<name sortKey="Pope, Alexandra" sort="Pope, Alexandra" uniqKey="Pope A" first="Alexandra" last="Pope">Alexandra Pope</name>
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<s1>Department, of Astronomy, University of Massachusetts, 710 North Pleasant Street</s1>
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<country>États-Unis</country>
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<s1>Astrophysics Group, Cavendish Laboratory, J. J. Thomson Avenue</s1>
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<s1>Kavli Institute for Cosmology, c/o Institute of Astronomy, University of Cambridge, Madingley Road</s1>
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<name sortKey="Urquhart, J S" sort="Urquhart, J S" uniqKey="Urquhart J" first="J. S." last="Urquhart">J. S. Urquhart</name>
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<s1>Australia Telescope National Facility, CSIRO Astronomy and Space Science</s1>
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<country>Australie</country>
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<author>
<name sortKey="Vaccari, Mattia" sort="Vaccari, Mattia" uniqKey="Vaccari M" first="Mattia" last="Vaccari">Mattia Vaccari</name>
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<author>
<name sortKey="Weferling, Bernd" sort="Weferling, Bernd" uniqKey="Weferling B" first="Bernd" last="Weferling">Bernd Weferling</name>
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<name sortKey="White, Glenn" sort="White, Glenn" uniqKey="White G" first="Glenn" last="White">Glenn White</name>
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<s1>Department of Physics and Astronomy, The Open University</s1>
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<author>
<name sortKey="Ming Zhu" sort="Ming Zhu" uniqKey="Ming Zhu" last="Ming Zhu">MING ZHU</name>
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<title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title>
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<term>Data reduction</term>
<term>Galaxies</term>
<term>HII regions</term>
<term>Signal-to-noise ratio</term>
<term>Sky surveys</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Etude ciel</term>
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<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 0.5 x 0.5 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 deg
<sup>2</sup>
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>
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<title xml:lang="en">A pilot study for the SCUBA‐2 ‘All‐Sky’ Survey</title>
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<name sortKey="Mackenzie, Todd" sort="Mackenzie, Todd" uniqKey="Mackenzie T" first="Todd" last="Mackenzie">Todd Mackenzie</name>
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<author>
<name sortKey="Braglia, Filiberto G" sort="Braglia, Filiberto G" uniqKey="Braglia F" first="Filiberto G." last="Braglia">Filiberto G. Braglia</name>
</author>
<author>
<name sortKey="Gibb, Andy G" sort="Gibb, Andy G" uniqKey="Gibb A" first="Andy G." last="Gibb">Andy G. Gibb</name>
</author>
<author>
<name sortKey="Scott, Douglas" sort="Scott, Douglas" uniqKey="Scott D" first="Douglas" last="Scott">Douglas Scott</name>
</author>
<author>
<name sortKey="Jenness, Tim" sort="Jenness, Tim" uniqKey="Jenness T" first="Tim" last="Jenness">Tim Jenness</name>
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<author>
<name sortKey="Serjeant, Stephen" sort="Serjeant, Stephen" uniqKey="Serjeant S" first="Stephen" last="Serjeant">Stephen Serjeant</name>
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<author>
<name sortKey="Thompson, Mark" sort="Thompson, Mark" uniqKey="Thompson M" first="Mark" last="Thompson">Mark Thompson</name>
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<author>
<name sortKey="Berry, David" sort="Berry, David" uniqKey="Berry D" first="David" last="Berry">David Berry</name>
</author>
<author>
<name sortKey="Brunt, Christopher M" sort="Brunt, Christopher M" uniqKey="Brunt C" first="Christopher M." last="Brunt">Christopher M. Brunt</name>
</author>
<author>
<name sortKey="Chapin, Edward" sort="Chapin, Edward" uniqKey="Chapin E" first="Edward" last="Chapin">Edward Chapin</name>
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<name sortKey="Chrysostomou, Antonio" sort="Chrysostomou, Antonio" uniqKey="Chrysostomou A" first="Antonio" last="Chrysostomou">Antonio Chrysostomou</name>
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<name sortKey="Clements, Dave" sort="Clements, Dave" uniqKey="Clements D" first="Dave" last="Clements">Dave Clements</name>
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<author>
<name sortKey="Coppin, Kristen" sort="Coppin, Kristen" uniqKey="Coppin K" first="Kristen" last="Coppin">Kristen Coppin</name>
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<name sortKey="Economou, Frossie" sort="Economou, Frossie" uniqKey="Economou F" first="Frossie" last="Economou">Frossie Economou</name>
</author>
<author>
<name sortKey="Evans, A" sort="Evans, A" uniqKey="Evans A" first="A." last="Evans">A. Evans</name>
</author>
<author>
<name sortKey="Friberg, Per" sort="Friberg, Per" uniqKey="Friberg P" first="Per" last="Friberg">Per Friberg</name>
</author>
<author>
<name sortKey="Greaves, Jane" sort="Greaves, Jane" uniqKey="Greaves J" first="Jane" last="Greaves">Jane Greaves</name>
</author>
<author>
<name sortKey="Hill, T" sort="Hill, T" uniqKey="Hill T" first="T." last="Hill">T. Hill</name>
</author>
<author>
<name sortKey="Holland, Wayne" sort="Holland, Wayne" uniqKey="Holland W" first="Wayne" last="Holland">Wayne Holland</name>
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<name sortKey="Ivison, R J" sort="Ivison, R J" uniqKey="Ivison R" first="R. J." last="Ivison">R. J. Ivison</name>
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<name sortKey="Knapen, Johan H" sort="Knapen, Johan H" uniqKey="Knapen J" first="Johan H." last="Knapen">Johan H. Knapen</name>
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<author>
<name sortKey="Jackson, Neal" sort="Jackson, Neal" uniqKey="Jackson N" first="Neal" last="Jackson">Neal Jackson</name>
</author>
<author>
<name sortKey="Joncas, Gilles" sort="Joncas, Gilles" uniqKey="Joncas G" first="Gilles" last="Joncas">Gilles Joncas</name>
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<name sortKey="Morgan, Larry" sort="Morgan, Larry" uniqKey="Morgan L" first="Larry" last="Morgan">Larry Morgan</name>
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<name sortKey="Mortier, Angela" sort="Mortier, Angela" uniqKey="Mortier A" first="Angela" last="Mortier">Angela Mortier</name>
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<name sortKey="Pearson, Chris" sort="Pearson, Chris" uniqKey="Pearson C" first="Chris" last="Pearson">Chris Pearson</name>
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<author>
<name sortKey="Pestalozzi, Michele" sort="Pestalozzi, Michele" uniqKey="Pestalozzi M" first="Michele" last="Pestalozzi">Michele Pestalozzi</name>
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<name sortKey="Pope, Alexandra" sort="Pope, Alexandra" uniqKey="Pope A" first="Alexandra" last="Pope">Alexandra Pope</name>
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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="Urquhart, J S" sort="Urquhart, J S" uniqKey="Urquhart J" first="J. S." last="Urquhart">J. S. Urquhart</name>
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<author>
<name sortKey="Vaccari, Mattia" sort="Vaccari, Mattia" uniqKey="Vaccari M" first="Mattia" last="Vaccari">Mattia Vaccari</name>
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<author>
<name sortKey="Weferling, Bernd" sort="Weferling, Bernd" uniqKey="Weferling B" first="Bernd" last="Weferling">Bernd Weferling</name>
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<author>
<name sortKey="White, Glenn" sort="White, Glenn" uniqKey="White G" first="Glenn" last="White">Glenn White</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>Blackbody spectrum</term>
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<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>
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