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A pilot study for the SCUBA-2 'All-Sky' Survey

Identifieur interne : 001A86 ( PascalFrancis/Corpus ); précédent : 001A85; suivant : 001A87

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 : Pascal:11-0336540

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 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 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.

Notice en format standard (ISO 2709)

Pour connaître la documentation sur le format Inist Standard.

pA  
A01 01  1    @0 0035-8711
A02 01      @0 MNRAA4
A03   1    @0 Mon. Not. R. Astron. Soc.
A05       @2 415
A06       @2 2
A08 01  1  ENG  @1 A pilot study for the SCUBA-2 'All-Sky' Survey
A11 01  1    @1 MACKENZIE (Todd)
A11 02  1    @1 BRAGLIA (Filiberto G.)
A11 03  1    @1 GIBB (Andy G.)
A11 04  1    @1 SCOTT (Douglas)
A11 05  1    @1 JENNESS (Tim)
A11 06  1    @1 SERJEANT (Stephen)
A11 07  1    @1 THOMPSON (Mark)
A11 08  1    @1 BERRY (David)
A11 09  1    @1 BRUNT (Christopher M.)
A11 10  1    @1 CHAPIN (Edward)
A11 11  1    @1 CHRYSOSTOMOU (Antonio)
A11 12  1    @1 CLEMENTS (Dave)
A11 13  1    @1 COPPIN (Kristen)
A11 14  1    @1 ECONOMOU (Frossie)
A11 15  1    @1 EVANS (A.)
A11 16  1    @1 FRIBERG (Per)
A11 17  1    @1 GREAVES (Jane)
A11 18  1    @1 HILL (T.)
A11 19  1    @1 HOLLAND (Wayne)
A11 20  1    @1 IVISON (R. J.)
A11 21  1    @1 KNAPEN (Johan H.)
A11 22  1    @1 JACKSON (Neal)
A11 23  1    @1 JONCAS (Gilles)
A11 24  1    @1 MORGAN (Larry)
A11 25  1    @1 MORTIER (Angela)
A11 26  1    @1 PEARSON (Chris)
A11 27  1    @1 PESTALOZZI (Michele)
A11 28  1    @1 POPE (Alexandra)
A11 29  1    @1 RICHER (John)
A11 30  1    @1 URQUHART (J. S.)
A11 31  1    @1 VACCARI (Mattia)
A11 32  1    @1 WEFERLING (Bernd)
A11 33  1    @1 WHITE (Glenn)
A11 34  1    @1 MING ZHU
A14 01      @1 Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road @2 Vancouver, BC V6T 1Z1 @3 CAN @Z 1 aut. @Z 2 aut. @Z 3 aut. @Z 4 aut. @Z 10 aut.
A14 02      @1 Joint Astronomy Centre, 660 North A'ohoku Place @2 Hilo, HI 96720 @3 USA @Z 5 aut. @Z 8 aut. @Z 11 aut. @Z 14 aut. @Z 16 aut.
A14 03      @1 Department of Physics and Astronomy, The Open University @2 Milton Keynes MK7 6BJ @3 GBR @Z 6 aut. @Z 26 aut. @Z 33 aut.
A14 04      @1 Centre for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, College Lane @2 Hatfield AL10 9AB @3 GBR @Z 7 aut.
A14 05      @1 School of Physics, Stocker Road @2 Exeter EX4 4QL @3 GBR @Z 9 aut.
A14 06      @1 Imperial College London, South Kensington Campus @2 London SW7 2AZ @3 GBR @Z 12 aut. @Z 25 aut.
A14 07      @1 Department of Physics, McGill University, 3600 rue University @2 Montreal, QC H3A 2T8 @3 CAN @Z 13 aut.
A14 08      @1 Institute for Computational Cosmology, Durham University, South Road @2 Durham DH1 3LE @3 GBR @Z 13 aut.
A14 09      @1 Astrophysics Group, Keele University @2 Keele, Staffordshire ST5 5BG @3 GBR @Z 15 aut.
A14 10      @1 School of Physics and Astronomy, University of St Andrews, North Haugh @2 St Andrews KY16 9SS @3 GBR @Z 17 aut.
A14 11      @1 Laboratoire AIM, CEA/IRFU - CNRS/INSU - Université Paris Diderot, CEA-Saclay @2 91191 Gif-sur-Yvette @3 FRA @Z 18 aut.
A14 12      @1 UK Astronomy Technology Centre, Royal Observatory, Blackford Hill @2 Edinburgh EH9 3HJ @3 GBR @Z 19 aut. @Z 20 aut.
A14 13      @1 Institute for Astronomy, University of Edinburgh, Blackford Hill @2 Edinburgh EH9 3HJ @3 GBR @Z 19 aut. @Z 20 aut.
A14 14      @1 Instituto de Astrofísica de Canarias @2 38200 La Laguna, Tenerife @3 ESP @Z 21 aut.
A14 15      @1 Departamento de Astrofísica, Universidad de La Laguna @2 38205 La Laguna, Tenerife @3 ESP @Z 21 aut.
A14 16      @1 Jodrell Bank Centre forAstrophysics, Alan Turing Building, School of Physics and Astronomy, University of Manchester, Oxford Road @2 Manchester M13 9PL @3 GBR @Z 22 aut.
A14 17      @1 Dépt. de physique, de génie physique et d'optique and Centre de recherche en astrophysique du Québec, Université Laval @2 Quebec G1V 0A6 @3 CAN @Z 23 aut.
A14 18      @1 Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf @2 Birkenhead, Wirral CH41 ILD @3 GBR @Z 24 aut.
A14 19      @1 RAL Space, Rutherford Appleton Laboratory, Chilton @2 Didcot, Oxfordshire OX11 OQX @3 GBR @Z 26 aut. @Z 33 aut.
A14 20      @1 Institute for Space Imaging Science, University of Lethbridge @2 Lethbridge, Alberta T1K 3M4 @3 CAN @Z 26 aut.
A14 21      @1 IFSI/INAF, via del Fosso del Cavaliere 100 @2 00173 Roma @3 ITA @Z 27 aut.
A14 22      @1 Department, of Astronomy, University of Massachusetts, 710 North Pleasant Street @2 Amherst, MA 01003-9305 @3 USA @Z 28 aut.
A14 23      @1 Astrophysics Group, Cavendish Laboratory, J. J. Thomson Avenue @2 Cambridge CB3 OHE @3 GBR @Z 29 aut.
A14 24      @1 Kavli Institute for Cosmology, c/o Institute of Astronomy, University of Cambridge, Madingley Road @2 Cambridge CB3 0HA @3 GBR @Z 29 aut.
A14 25      @1 Australia Telescope National Facility, CSIRO Astronomy and Space Science @2 Sydney, NSW 2052 @3 AUS @Z 30 aut.
A20       @1 1950-1960
A21       @1 2011
A23 01      @0 ENG
A43 01      @1 INIST @2 2067 @5 354000509466990770
A44       @0 0000 @1 © 2011 INIST-CNRS. All rights reserved.
A45       @0 1/2 p.
A47 01  1    @0 11-0336540
A60       @1 P
A61       @0 A
A64 01  1    @0 Monthly Notices of the Royal Astronomical Society
A66 01      @0 USA
C01 01    ENG  @0 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 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.
C02 01  3    @0 001E03
C03 01  3  FRE  @0 Etude ciel @5 26
C03 01  3  ENG  @0 Sky surveys @5 26
C03 02  3  FRE  @0 Réduction donnée @5 27
C03 02  3  ENG  @0 Data reduction @5 27
C03 03  3  FRE  @0 Galaxies @5 28
C03 03  3  ENG  @0 Galaxies @5 28
C03 04  3  FRE  @0 Région HII @5 29
C03 04  3  ENG  @0 HII regions @5 29
C03 05  3  FRE  @0 Rapport signal bruit @5 30
C03 05  3  ENG  @0 Signal-to-noise ratio @5 30
N21       @1 227
N44 01      @1 OTO
N82       @1 OTO

Format Inist (serveur)

NO : PASCAL 11-0336540 INIST
ET : A pilot study for the SCUBA-2 'All-Sky' Survey
AU : MACKENZIE (Todd); BRAGLIA (Filiberto G.); GIBB (Andy G.); SCOTT (Douglas); JENNESS (Tim); SERJEANT (Stephen); THOMPSON (Mark); BERRY (David); BRUNT (Christopher M.); CHAPIN (Edward); CHRYSOSTOMOU (Antonio); CLEMENTS (Dave); COPPIN (Kristen); ECONOMOU (Frossie); EVANS (A.); FRIBERG (Per); GREAVES (Jane); HILL (T.); HOLLAND (Wayne); IVISON (R. J.); KNAPEN (Johan H.); JACKSON (Neal); JONCAS (Gilles); MORGAN (Larry); MORTIER (Angela); PEARSON (Chris); PESTALOZZI (Michele); POPE (Alexandra); RICHER (John); URQUHART (J. S.); VACCARI (Mattia); WEFERLING (Bernd); WHITE (Glenn); MING ZHU
AF : Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road/Vancouver, BC V6T 1Z1/Canada (1 aut., 2 aut., 3 aut., 4 aut., 10 aut.); Joint Astronomy Centre, 660 North A'ohoku Place/Hilo, HI 96720/Etats-Unis (5 aut., 8 aut., 11 aut., 14 aut., 16 aut.); Department of Physics and Astronomy, The Open University/Milton Keynes MK7 6BJ/Royaume-Uni (6 aut., 26 aut., 33 aut.); Centre for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, College Lane/Hatfield AL10 9AB/Royaume-Uni (7 aut.); School of Physics, Stocker Road/Exeter EX4 4QL/Royaume-Uni (9 aut.); Imperial College London, South Kensington Campus/London SW7 2AZ/Royaume-Uni (12 aut., 25 aut.); Department of Physics, McGill University, 3600 rue University/Montreal, QC H3A 2T8/Canada (13 aut.); Institute for Computational Cosmology, Durham University, South Road/Durham DH1 3LE/Royaume-Uni (13 aut.); Astrophysics Group, Keele University/Keele, Staffordshire ST5 5BG/Royaume-Uni (15 aut.); School of Physics and Astronomy, University of St Andrews, North Haugh/St Andrews KY16 9SS/Royaume-Uni (17 aut.); Laboratoire AIM, CEA/IRFU - CNRS/INSU - Université Paris Diderot, CEA-Saclay/91191 Gif-sur-Yvette/France (18 aut.); UK Astronomy Technology Centre, Royal Observatory, Blackford Hill/Edinburgh EH9 3HJ/Royaume-Uni (19 aut., 20 aut.); Institute for Astronomy, University of Edinburgh, Blackford Hill/Edinburgh EH9 3HJ/Royaume-Uni (19 aut., 20 aut.); Instituto de Astrofísica de Canarias/38200 La Laguna, Tenerife/Espagne (21 aut.); Departamento de Astrofísica, Universidad de La Laguna/38205 La Laguna, Tenerife/Espagne (21 aut.); Jodrell Bank Centre forAstrophysics, Alan Turing Building, School of Physics and Astronomy, University of Manchester, Oxford Road/Manchester M13 9PL/Royaume-Uni (22 aut.); Dépt. de physique, de génie physique et d'optique and Centre de recherche en astrophysique du Québec, Université Laval/Quebec G1V 0A6/Canada (23 aut.); Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf/Birkenhead, Wirral CH41 ILD/Royaume-Uni (24 aut.); RAL Space, Rutherford Appleton Laboratory, Chilton/Didcot, Oxfordshire OX11 OQX/Royaume-Uni (26 aut., 33 aut.); Institute for Space Imaging Science, University of Lethbridge/Lethbridge, Alberta T1K 3M4/Canada (26 aut.); IFSI/INAF, via del Fosso del Cavaliere 100/00173 Roma/Italie (27 aut.); Department, of Astronomy, University of Massachusetts, 710 North Pleasant Street/Amherst, MA 01003-9305/Etats-Unis (28 aut.); Astrophysics Group, Cavendish Laboratory, J. J. Thomson Avenue/Cambridge CB3 OHE/Royaume-Uni (29 aut.); Kavli Institute for Cosmology, c/o Institute of Astronomy, University of Cambridge, Madingley Road/Cambridge CB3 0HA/Royaume-Uni (29 aut.); Australia Telescope National Facility, CSIRO Astronomy and Space Science/Sydney, NSW 2052/Australie (30 aut.)
DT : Publication en série; Niveau analytique
SO : Monthly Notices of the Royal Astronomical Society; ISSN 0035-8711; Coden MNRAA4; Etats-Unis; Da. 2011; Vol. 415; No. 2; Pp. 1950-1960; Bibl. 1/2 p.
LA : Anglais
EA : 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 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.
CC : 001E03
FD : Etude ciel; Réduction donnée; Galaxies; Région HII; Rapport signal bruit
ED : Sky surveys; Data reduction; Galaxies; HII regions; Signal-to-noise ratio
LO : INIST-2067.354000509466990770
ID : 11-0336540

Links to Exploration step

Pascal:11-0336540

Le document en format XML

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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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<s1>Institute for Computational Cosmology, Durham University, South Road</s1>
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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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<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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<s1>Department, of Astronomy, University of Massachusetts, 710 North Pleasant Street</s1>
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<s1>Astrophysics Group, Cavendish Laboratory, J. J. Thomson Avenue</s1>
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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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<inist:fA14 i1="01">
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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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<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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<sup>2</sup>
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<ET>A pilot study for the SCUBA-2 'All-Sky' Survey</ET>
<AU>MACKENZIE (Todd); BRAGLIA (Filiberto G.); GIBB (Andy G.); SCOTT (Douglas); JENNESS (Tim); SERJEANT (Stephen); THOMPSON (Mark); BERRY (David); BRUNT (Christopher M.); CHAPIN (Edward); CHRYSOSTOMOU (Antonio); CLEMENTS (Dave); COPPIN (Kristen); ECONOMOU (Frossie); EVANS (A.); FRIBERG (Per); GREAVES (Jane); HILL (T.); HOLLAND (Wayne); IVISON (R. J.); KNAPEN (Johan H.); JACKSON (Neal); JONCAS (Gilles); MORGAN (Larry); MORTIER (Angela); PEARSON (Chris); PESTALOZZI (Michele); POPE (Alexandra); RICHER (John); URQUHART (J. S.); VACCARI (Mattia); WEFERLING (Bernd); WHITE (Glenn); MING ZHU</AU>
<AF>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road/Vancouver, BC V6T 1Z1/Canada (1 aut., 2 aut., 3 aut., 4 aut., 10 aut.); Joint Astronomy Centre, 660 North A'ohoku Place/Hilo, HI 96720/Etats-Unis (5 aut., 8 aut., 11 aut., 14 aut., 16 aut.); Department of Physics and Astronomy, The Open University/Milton Keynes MK7 6BJ/Royaume-Uni (6 aut., 26 aut., 33 aut.); Centre for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, College Lane/Hatfield AL10 9AB/Royaume-Uni (7 aut.); School of Physics, Stocker Road/Exeter EX4 4QL/Royaume-Uni (9 aut.); Imperial College London, South Kensington Campus/London SW7 2AZ/Royaume-Uni (12 aut., 25 aut.); Department of Physics, McGill University, 3600 rue University/Montreal, QC H3A 2T8/Canada (13 aut.); Institute for Computational Cosmology, Durham University, South Road/Durham DH1 3LE/Royaume-Uni (13 aut.); Astrophysics Group, Keele University/Keele, Staffordshire ST5 5BG/Royaume-Uni (15 aut.); School of Physics and Astronomy, University of St Andrews, North Haugh/St Andrews KY16 9SS/Royaume-Uni (17 aut.); Laboratoire AIM, CEA/IRFU - CNRS/INSU - Université Paris Diderot, CEA-Saclay/91191 Gif-sur-Yvette/France (18 aut.); UK Astronomy Technology Centre, Royal Observatory, Blackford Hill/Edinburgh EH9 3HJ/Royaume-Uni (19 aut., 20 aut.); Institute for Astronomy, University of Edinburgh, Blackford Hill/Edinburgh EH9 3HJ/Royaume-Uni (19 aut., 20 aut.); Instituto de Astrofísica de Canarias/38200 La Laguna, Tenerife/Espagne (21 aut.); Departamento de Astrofísica, Universidad de La Laguna/38205 La Laguna, Tenerife/Espagne (21 aut.); Jodrell Bank Centre forAstrophysics, Alan Turing Building, School of Physics and Astronomy, University of Manchester, Oxford Road/Manchester M13 9PL/Royaume-Uni (22 aut.); Dépt. de physique, de génie physique et d'optique and Centre de recherche en astrophysique du Québec, Université Laval/Quebec G1V 0A6/Canada (23 aut.); Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf/Birkenhead, Wirral CH41 ILD/Royaume-Uni (24 aut.); RAL Space, Rutherford Appleton Laboratory, Chilton/Didcot, Oxfordshire OX11 OQX/Royaume-Uni (26 aut., 33 aut.); Institute for Space Imaging Science, University of Lethbridge/Lethbridge, Alberta T1K 3M4/Canada (26 aut.); IFSI/INAF, via del Fosso del Cavaliere 100/00173 Roma/Italie (27 aut.); Department, of Astronomy, University of Massachusetts, 710 North Pleasant Street/Amherst, MA 01003-9305/Etats-Unis (28 aut.); Astrophysics Group, Cavendish Laboratory, J. J. Thomson Avenue/Cambridge CB3 OHE/Royaume-Uni (29 aut.); Kavli Institute for Cosmology, c/o Institute of Astronomy, University of Cambridge, Madingley Road/Cambridge CB3 0HA/Royaume-Uni (29 aut.); Australia Telescope National Facility, CSIRO Astronomy and Space Science/Sydney, NSW 2052/Australie (30 aut.)</AF>
<DT>Publication en série; Niveau analytique</DT>
<SO>Monthly Notices of the Royal Astronomical Society; ISSN 0035-8711; Coden MNRAA4; Etats-Unis; Da. 2011; Vol. 415; No. 2; Pp. 1950-1960; Bibl. 1/2 p.</SO>
<LA>Anglais</LA>
<EA>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.</EA>
<CC>001E03</CC>
<FD>Etude ciel; Réduction donnée; Galaxies; Région HII; Rapport signal bruit</FD>
<ED>Sky surveys; Data reduction; Galaxies; HII regions; Signal-to-noise ratio</ED>
<LO>INIST-2067.354000509466990770</LO>
<ID>11-0336540</ID>
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