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/Exploration ); 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


Affiliations:


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Le document en format XML

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<name sortKey="Weferling, Bernd" sort="Weferling, Bernd" uniqKey="Weferling B" first="Bernd" last="Weferling">Bernd Weferling</name>
<affiliation wicri:level="1">
<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>
</affiliation>
</author>
<author>
<name sortKey="White, Glenn" sort="White, Glenn" uniqKey="White G" first="Glenn" last="White">Glenn White</name>
<affiliation></affiliation>
<affiliation>
<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>
<placeName>
<settlement type="city">Pékin</settlement>
</placeName>
</affiliation>
</author>
</analytic>
<monogr></monogr>
<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>
<biblScope unit="issue">2</biblScope>
<biblScope unit="page" from="1950">1950</biblScope>
<biblScope unit="page" to="1960">1960</biblScope>
<biblScope unit="page-count">11</biblScope>
<publisher>Blackwell Publishing Ltd</publisher>
<pubPlace>Oxford, UK</pubPlace>
<date type="published" when="2011-08-01">2011-08-01</date>
</imprint>
<idno type="ISSN">0035-8711</idno>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt>
<idno type="ISSN">0035-8711</idno>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<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>
<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>Signal-to-noise ratio</term>
<term>Sky surveys</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="Pascal" xml:lang="fr">
<term>Etude ciel</term>
<term>Galaxies</term>
<term>Rapport signal bruit</term>
<term>Réduction donnée</term>
<term>Région HII</term>
</keywords>
<keywords scheme="Teeft" xml:lang="en">
<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>
<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>
<affiliations>
<list>
<country>
<li>Allemagne</li>
<li>Australie</li>
<li>Canada</li>
<li>Espagne</li>
<li>France</li>
<li>Italie</li>
<li>Royaume-Uni</li>
<li>République populaire de Chine</li>
<li>États-Unis</li>
</country>
<region>
<li>Angleterre</li>
<li>Angleterre de l'Est</li>
<li>Grand Manchester</li>
<li>Hawaï</li>
<li>Massachusetts</li>
<li>Québec</li>
<li>Écosse</li>
</region>
<settlement>
<li>Amherst (Massachusetts)</li>
<li>Cambridge</li>
<li>Manchester</li>
<li>Montréal</li>
<li>Pékin</li>
<li>Édimbourg</li>
</settlement>
<orgName>
<li>Université McGill</li>
<li>Université d'Édimbourg</li>
<li>Université de Cambridge</li>
<li>Université de Manchester</li>
<li>Université du Massachusetts</li>
</orgName>
</list>
<tree>
<noCountry>
<name sortKey="Brunt, Christopher M" sort="Brunt, Christopher M" uniqKey="Brunt C" first="Christopher M." last="Brunt">Christopher M. Brunt</name>
<name sortKey="Clements, Dave" sort="Clements, Dave" uniqKey="Clements D" first="Dave" last="Clements">Dave Clements</name>
<name sortKey="Evans, A" sort="Evans, A" uniqKey="Evans A" first="A." last="Evans">A. Evans</name>
<name sortKey="Greaves, Jane" sort="Greaves, Jane" uniqKey="Greaves J" first="Jane" last="Greaves">Jane Greaves</name>
<name sortKey="Morgan, Larry" sort="Morgan, Larry" uniqKey="Morgan L" first="Larry" last="Morgan">Larry Morgan</name>
<name sortKey="Mortier, Angela" sort="Mortier, Angela" uniqKey="Mortier A" first="Angela" last="Mortier">Angela Mortier</name>
<name sortKey="Serjeant, Stephen" sort="Serjeant, Stephen" uniqKey="Serjeant S" first="Stephen" last="Serjeant">Stephen Serjeant</name>
<name sortKey="Thompson, Mark" sort="Thompson, Mark" uniqKey="Thompson M" first="Mark" last="Thompson">Mark Thompson</name>
<name sortKey="White, Glenn" sort="White, Glenn" uniqKey="White G" first="Glenn" last="White">Glenn White</name>
</noCountry>
<country name="Canada">
<noRegion>
<name sortKey="Mackenzie, Todd" sort="Mackenzie, Todd" uniqKey="Mackenzie T" first="Todd" last="Mackenzie">Todd Mackenzie</name>
</noRegion>
<name sortKey="Braglia, Filiberto G" sort="Braglia, Filiberto G" uniqKey="Braglia F" first="Filiberto G." last="Braglia">Filiberto G. Braglia</name>
<name sortKey="Chapin, Edward" sort="Chapin, Edward" uniqKey="Chapin E" first="Edward" last="Chapin">Edward Chapin</name>
<name sortKey="Coppin, Kristen" sort="Coppin, Kristen" uniqKey="Coppin K" first="Kristen" last="Coppin">Kristen Coppin</name>
<name sortKey="Gibb, Andy G" sort="Gibb, Andy G" uniqKey="Gibb A" first="Andy G." last="Gibb">Andy G. Gibb</name>
<name sortKey="Joncas, Gilles" sort="Joncas, Gilles" uniqKey="Joncas G" first="Gilles" last="Joncas">Gilles Joncas</name>
<name sortKey="Mackenzie, Todd" sort="Mackenzie, Todd" uniqKey="Mackenzie T" first="Todd" last="Mackenzie">Todd Mackenzie</name>
<name sortKey="Pearson, Chris" sort="Pearson, Chris" uniqKey="Pearson C" first="Chris" last="Pearson">Chris Pearson</name>
<name sortKey="Scott, Douglas" sort="Scott, Douglas" uniqKey="Scott D" first="Douglas" last="Scott">Douglas Scott</name>
</country>
<country name="États-Unis">
<region name="Hawaï">
<name sortKey="Jenness, Tim" sort="Jenness, Tim" uniqKey="Jenness T" first="Tim" last="Jenness">Tim Jenness</name>
</region>
<name sortKey="Berry, David" sort="Berry, David" uniqKey="Berry D" first="David" last="Berry">David Berry</name>
<name sortKey="Chrysostomou, Antonio" sort="Chrysostomou, Antonio" uniqKey="Chrysostomou A" first="Antonio" last="Chrysostomou">Antonio Chrysostomou</name>
<name sortKey="Economou, Frossie" sort="Economou, Frossie" uniqKey="Economou F" first="Frossie" last="Economou">Frossie Economou</name>
<name sortKey="Friberg, Per" sort="Friberg, Per" uniqKey="Friberg P" first="Per" last="Friberg">Per Friberg</name>
<name sortKey="Pope, Alexandra" sort="Pope, Alexandra" uniqKey="Pope A" first="Alexandra" last="Pope">Alexandra Pope</name>
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<country name="France">
<noRegion>
<name sortKey="Hill, T" sort="Hill, T" uniqKey="Hill T" first="T." last="Hill">T. Hill</name>
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</country>
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<region name="Écosse">
<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>
<name sortKey="Jackson, Neal" sort="Jackson, Neal" uniqKey="Jackson N" first="Neal" last="Jackson">Neal Jackson</name>
<name sortKey="Richer, John" sort="Richer, John" uniqKey="Richer J" first="John" last="Richer">John Richer</name>
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<noRegion>
<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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<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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<country name="Italie">
<noRegion>
<name sortKey="Pestalozzi, Michele" sort="Pestalozzi, Michele" uniqKey="Pestalozzi M" first="Michele" last="Pestalozzi">Michele Pestalozzi</name>
</noRegion>
<name sortKey="Vaccari, Mattia" sort="Vaccari, Mattia" uniqKey="Vaccari M" first="Mattia" last="Vaccari">Mattia Vaccari</name>
</country>
<country name="Australie">
<noRegion>
<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 name="Allemagne">
<noRegion>
<name sortKey="Weferling, Bernd" sort="Weferling, Bernd" uniqKey="Weferling B" first="Bernd" last="Weferling">Bernd Weferling</name>
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</country>
<country name="République populaire de Chine">
<noRegion>
<name sortKey="Zhu, Ming" sort="Zhu, Ming" uniqKey="Zhu M" first="Ming" last="Zhu">Ming Zhu</name>
</noRegion>
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</affiliations>
</record>

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