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

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

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

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

Source :

RBID : ISTEX:D3AEB0B34F47F7449B9735E70BD8BD35701E7B63

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

Links to Exploration step

ISTEX:D3AEB0B34F47F7449B9735E70BD8BD35701E7B63

Le document en format XML

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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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<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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<title level="a" type="main">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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<mods:affiliation>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation>
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<mods:affiliation>Correspondence address: E‐mail: todd@phas.ubc.ca</mods:affiliation>
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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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<name sortKey="Gibb, Andy G" sort="Gibb, Andy G" uniqKey="Gibb A" first="Andy G." last="Gibb">Andy G. Gibb</name>
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<mods:affiliation>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation>
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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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<mods:affiliation>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation>
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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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<name sortKey="Serjeant, Stephen" sort="Serjeant, Stephen" uniqKey="Serjeant S" first="Stephen" last="Serjeant">Stephen Serjeant</name>
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<name sortKey="Thompson, Mark" sort="Thompson, Mark" uniqKey="Thompson M" first="Mark" last="Thompson">Mark Thompson</name>
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<name sortKey="Berry, David" sort="Berry, David" uniqKey="Berry D" first="David" last="Berry">David Berry</name>
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<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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<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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<name sortKey="Coppin, Kristen" sort="Coppin, Kristen" uniqKey="Coppin K" first="Kristen" last="Coppin">Kristen Coppin</name>
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<mods:affiliation>Department of Physics, McGill University, 3600 rue University, Montréal, QC H3A 2T8, Canada</mods:affiliation>
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<affiliation>
<mods:affiliation>Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE</mods:affiliation>
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<name sortKey="Economou, Frossie" sort="Economou, Frossie" uniqKey="Economou F" first="Frossie" last="Economou">Frossie Economou</name>
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<name sortKey="Evans, A" sort="Evans, A" uniqKey="Evans A" first="A." last="Evans">A. Evans</name>
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<mods:affiliation>Astrophysics Group, Keele University, Keele, Staffordshire ST5 5BG</mods:affiliation>
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<name sortKey="Friberg, Per" sort="Friberg, Per" uniqKey="Friberg P" first="Per" last="Friberg">Per Friberg</name>
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<name sortKey="Greaves, Jane" sort="Greaves, Jane" uniqKey="Greaves J" first="Jane" last="Greaves">Jane Greaves</name>
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<name sortKey="Hill, T" sort="Hill, T" uniqKey="Hill T" first="T." last="Hill">T. Hill</name>
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</author>
<author>
<name sortKey="Holland, Wayne" sort="Holland, Wayne" uniqKey="Holland W" first="Wayne" last="Holland">Wayne Holland</name>
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<mods:affiliation>UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ</mods:affiliation>
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<affiliation>
<mods:affiliation>Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ</mods:affiliation>
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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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<mods:affiliation>UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ</mods:affiliation>
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<affiliation>
<mods:affiliation>Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ</mods:affiliation>
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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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<mods:affiliation>Instituto de Astrofísica de Canarias, E‐38200 La Laguna, Tenerife, Spain</mods:affiliation>
</affiliation>
<affiliation>
<mods:affiliation>Departamento de Astrofísica, Universidad de La Laguna, E‐38205 La Laguna, Tenerife, Spain</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Jackson, Neal" sort="Jackson, Neal" uniqKey="Jackson N" first="Neal" last="Jackson">Neal Jackson</name>
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<mods:affiliation>Jodrell Bank Centre for Astrophysics, Alan Turing Building, School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Joncas, Gilles" sort="Joncas, Gilles" uniqKey="Joncas G" first="Gilles" last="Joncas">Gilles Joncas</name>
<affiliation>
<mods:affiliation>Dépt. de physique, de génie physique et d’optique and Centre de recherche en astrophysique du Québec, Université Laval, Québec G1V 0A6, Canada</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Morgan, Larry" sort="Morgan, Larry" uniqKey="Morgan L" first="Larry" last="Morgan">Larry Morgan</name>
<affiliation>
<mods:affiliation>Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead, Wirral CH41 1LD</mods:affiliation>
</affiliation>
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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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<mods:affiliation>Imperial College London, South Kensington Campus, London SW7 2AZ</mods:affiliation>
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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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<name sortKey="Pestalozzi, Michele" sort="Pestalozzi, Michele" uniqKey="Pestalozzi M" first="Michele" last="Pestalozzi">Michele Pestalozzi</name>
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<mods:affiliation>IFSI/INAF, via del Fosso del Cavaliere 100, I–00173 Roma, Italy</mods:affiliation>
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<author>
<name sortKey="Pope, Alexandra" sort="Pope, Alexandra" uniqKey="Pope A" first="Alexandra" last="Pope">Alexandra Pope</name>
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<mods:affiliation>Department of Astronomy, University of Massachusetts, 710 North Pleasant Street, Amherst, MA 01003‐9305, USA</mods:affiliation>
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<author>
<name sortKey="Richer, John" sort="Richer, John" uniqKey="Richer J" first="John" last="Richer">John Richer</name>
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<affiliation>
<mods:affiliation>Kavli Institute for Cosmology, c/o Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA</mods:affiliation>
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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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<mods:affiliation>Department of Astronomy, University of Padova, Vicolo Osservatorio 3, I‐35122 Padova, Italy</mods:affiliation>
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<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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<mods:affiliation>Department of Physics and Astronomy, The Open University, Milton Keynes MK7 6BJ</mods:affiliation>
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<affiliation>
<mods:affiliation>RAL Space, Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 0QX</mods:affiliation>
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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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<mods:affiliation>National Astronomical Observatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing, China</mods:affiliation>
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<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>
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<biblScope unit="vol">415</biblScope>
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<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>
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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>Average integration time</term>
<term>Background subtraction</term>
<term>Blackbody</term>
<term>Blackbody spectrum</term>
<term>Blackford hill</term>
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<term>Cent uncorrelated uncertainty</term>
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<term>Dust emissivity index</term>
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<term>Extragalactic observations</term>
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<term>Free parameter</term>
<term>Galactic</term>
<term>Galactic cirrus</term>
<term>Galactic plane</term>
<term>Galaxy</term>
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<term>Hydrogen atom</term>
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<term>Iras data</term>
<term>James clerk maxwell telescope</term>
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<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>
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<term>Outer region</term>
<term>Outer regions</term>
<term>Peak values</term>
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<term>Iras data</term>
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<term>Noise excursions</term>
<term>Noise level</term>
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<term>Outer regions</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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<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.</abstract>
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<affiliation>Institute for Astronomy, University of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ</affiliation>
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<namePart type="given">Chris</namePart>
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<affiliation>Institute for Space Imaging Science, University of Lethbridge, Lethbridge, Alberta T1K 3M4, Canada</affiliation>
<affiliation>Department of Physics and Astronomy, The Open University, Milton Keynes MK7 6BJ</affiliation>
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<affiliation>Kavli Institute for Cosmology, c/o Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA</affiliation>
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<namePart type="family">Vaccari</namePart>
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<namePart type="given">Bernd</namePart>
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<affiliation>University Bamberg, Markusplatz 3, 96045 Bamberg, Germany</affiliation>
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<affiliation>RAL Space, Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 0QX</affiliation>
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<namePart type="given">Ming</namePart>
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<abstract 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.</abstract>
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<accessCondition type="use and reproduction" contentType="copyright">© 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS</accessCondition>
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