Submillimetre observations of galaxy clusters with the BLAST: the star formation activity in Abell 3112
Identifieur interne : 001F71 ( Istex/Corpus ); précédent : 001F70; suivant : 001F72Submillimetre observations of galaxy clusters with the BLAST: the star formation activity in Abell 3112
Auteurs : Filiberto G. Braglia ; Peter A. R. Ade ; James J. Bock ; Edward L. Chapin ; Mark J. Devlin ; Alastair Edge ; Matthew Griffin ; Joshua O. Gundersen ; Mark Halpern ; Peter C. Hargrave ; David H. Hughes ; Jeff Klein ; Gaelen Marsden ; Philip Mauskopf ; Lorenzo Moncelsi ; Calvin B. Netterfield ; Henry Ngo ; Luca Olmi ; Enzo Pascale ; Guillaume Patanchon ; Kevin A. Pimbblet ; Marie Rex ; Douglas Scott ; Christopher Semisch ; Nicholas Thomas ; Matthew D. P. Truch ; Carole Tucker ; Gregory S. Tucker ; Elisabetta Valiante ; Marco P. Viero ; Donald V. WiebeSource :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2011-04-01.
English descriptors
- KwdEn :
- Abell, Average ssfr, Biviano, Blast, Blast bands, Blast catalogue, Blast counterparts, Blast data, Blast maps, Blast observations, Blast sources, Blast wavelengths, Blue galaxies, Boxes mark, Braglia, Brightest cluster galaxy, California institute, Central galaxy, Characteristic magnitude, Cluster, Cluster centre, Cluster core, Cluster diagram, Cluster galaxies, Cluster member, Cluster member catalogue, Cluster members, Cluster redshift, Clustercentric, Clustercentric distances, Clustercentric radius, Cold dust, Colour, Colours, Devlin, Distance scale, Dust content, Dust masses, Emission lines, Environmental effects, Flux densities, Galaxy, Galaxy clusters, Galaxy geometry, Global decrease, Good agreement, Haines, Inclination angle, Individual sources, Infall region, Instrumental counts, Instrumental noise, Ira, Iras source, Lamentary structures, Large aperture submillimeter telescope, Large fraction, Large sample, Large spirals, Largest part, Line marks, Lines mark, Luminosity, Mnras, Monthly notices, Normal galaxies, Normal starforming galaxies, Notable drop, Number counts, Optical cluster members, Optical colour, Optical colours, Optical counterparts, Optical spectra, Optical spectroscopy, Optical spectrum, Panels show, Pascale, Photometry, Physics astronomy, Pierini, Porter raychaudhury, Positional uncertainty, Potential cluster members, Previous results, Previous studies, Propulsion laboratory, Radial bins, Radial distribution, Radial peak, Radial trends, Random occurrence, Redshift, Rejection probability, Robust, Same area, Same method, Seds, Sfrs, Solid line, Source catalogue, Source extraction, Spectral region, Spectroscopic, Spectroscopic catalogue, Ssfr, Star formation, Star formation activity, Stellar, Stellar mass, Stellar masses, Stellar population, Submm, Submm emission, Submm wavelengths, Unobscured star formation activity, Upper limit, Vertical lines mark, Wavelength.
- Teeft :
- Abell, Average ssfr, Biviano, Blast, Blast bands, Blast catalogue, Blast counterparts, Blast data, Blast maps, Blast observations, Blast sources, Blast wavelengths, Blue galaxies, Boxes mark, Braglia, Brightest cluster galaxy, California institute, Central galaxy, Characteristic magnitude, Cluster, Cluster centre, Cluster core, Cluster diagram, Cluster galaxies, Cluster member, Cluster member catalogue, Cluster members, Cluster redshift, Clustercentric, Clustercentric distances, Clustercentric radius, Cold dust, Colour, Colours, Devlin, Distance scale, Dust content, Dust masses, Emission lines, Environmental effects, Flux densities, Galaxy, Galaxy clusters, Galaxy geometry, Global decrease, Good agreement, Haines, Inclination angle, Individual sources, Infall region, Instrumental counts, Instrumental noise, Ira, Iras source, Lamentary structures, Large aperture submillimeter telescope, Large fraction, Large sample, Large spirals, Largest part, Line marks, Lines mark, Luminosity, Mnras, Monthly notices, Normal galaxies, Normal starforming galaxies, Notable drop, Number counts, Optical cluster members, Optical colour, Optical colours, Optical counterparts, Optical spectra, Optical spectroscopy, Optical spectrum, Panels show, Pascale, Photometry, Physics astronomy, Pierini, Porter raychaudhury, Positional uncertainty, Potential cluster members, Previous results, Previous studies, Propulsion laboratory, Radial bins, Radial distribution, Radial peak, Radial trends, Random occurrence, Redshift, Rejection probability, Robust, Same area, Same method, Seds, Sfrs, Solid line, Source catalogue, Source extraction, Spectral region, Spectroscopic, Spectroscopic catalogue, Ssfr, Star formation, Star formation activity, Stellar, Stellar mass, Stellar masses, Stellar population, Submm, Submm emission, Submm wavelengths, Unobscured star formation activity, Upper limit, Vertical lines mark, Wavelength.
Abstract
We present observations at 250, 350 and 500 μm of the nearby galaxy cluster Abell 3112 (z= 0.075) carried out with the Balloon‐borne Large Aperture Submillimeter Telescope. Five cluster members are individually detected as bright submillimetre (submm) sources. Their far‐infrared spectral energy distributions and optical colours identify them as normal star‐forming galaxies of high mass, with globally evolved stellar populations. They all have (B−R) colours of 1.38 ± 0.08, transitional between the blue, active population and the red, evolved galaxies that dominate the cluster core. We stack to estimate the mean submm emission from all cluster members, which is determined to be 16.6 ± 2.5, 6.1 ± 1.9 and 1.5 ± 1.3 mJy at 250, 350 and 500 μm, respectively. Stacking analyses of the submm emission of cluster members reveal trends in the mean far‐infrared luminosity with respect to clustercentric radius and KS‐band magnitude. We find that a large fraction of submm emission comes from the boundary of the inner, virialized region of the cluster, at clustercentric distances around R500. Stacking also shows that the bulk of the submm emission arises in intermediate‐mass galaxies with KS magnitude ∼1 mag fainter than the characteristic magnitude . The results and constraints obtained in this work will provide a useful reference for the forthcoming surveys to be conducted on galaxy clusters by Herschel.
Url:
DOI: 10.1111/j.1365-2966.2010.17973.x
Links to Exploration step
ISTEX:A6B192742E968B4F255CC383950810AB9DB59FB4Le document en format XML
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Postal 51 y 72000 Puebla, Mexico</mods:affiliation></affiliation></author><author><name sortKey="Klein, Jeff" sort="Klein, Jeff" uniqKey="Klein J" first="Jeff" last="Klein">Jeff Klein</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</mods:affiliation></affiliation></author><author><name sortKey="Marsden, Gaelen" sort="Marsden, Gaelen" uniqKey="Marsden G" first="Gaelen" last="Marsden">Gaelen Marsden</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></affiliation></author><author><name sortKey="Mauskopf, Philip" sort="Mauskopf, Philip" uniqKey="Mauskopf P" first="Philip" last="Mauskopf">Philip Mauskopf</name><affiliation><mods:affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</mods:affiliation></affiliation></author><author><name sortKey="Moncelsi, Lorenzo" sort="Moncelsi, Lorenzo" uniqKey="Moncelsi L" first="Lorenzo" last="Moncelsi">Lorenzo Moncelsi</name><affiliation><mods:affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</mods:affiliation></affiliation></author><author><name sortKey="Netterfield, Calvin B" sort="Netterfield, Calvin B" uniqKey="Netterfield C" first="Calvin B." last="Netterfield">Calvin B. Netterfield</name><affiliation><mods:affiliation>Department of Astronomy & Astrophysics, University of Toronto, 50 St George Street Toronto, ON M5S 3H4, Canada</mods:affiliation></affiliation><affiliation><mods:affiliation>Department of Physics, University of Toronto, 60 St George Street, Toronto, ON M5S 1A7, Canada</mods:affiliation></affiliation></author><author><name sortKey="Ngo, Henry" sort="Ngo, Henry" uniqKey="Ngo H" first="Henry" last="Ngo">Henry Ngo</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></affiliation></author><author><name sortKey="Olmi, Luca" sort="Olmi, Luca" uniqKey="Olmi L" first="Luca" last="Olmi">Luca Olmi</name><affiliation><mods:affiliation>Physics Department, University of Puerto Rico, Rio Piedras Campus, Box 23343, UPR station, PR 00931, USA</mods:affiliation></affiliation><affiliation><mods:affiliation>INAF ‐ Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I‐50125 Firenze, Italy</mods:affiliation></affiliation></author><author><name sortKey="Pascale, Enzo" sort="Pascale, Enzo" uniqKey="Pascale E" first="Enzo" last="Pascale">Enzo Pascale</name><affiliation><mods:affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</mods:affiliation></affiliation></author><author><name sortKey="Patanchon, Guillaume" sort="Patanchon, Guillaume" uniqKey="Patanchon G" first="Guillaume" last="Patanchon">Guillaume Patanchon</name><affiliation><mods:affiliation>Université Paris Diderot, Laboratoire APC, 10, rue Alice Domon et Léonie Duquet, 75205 Paris, France</mods:affiliation></affiliation></author><author><name sortKey="Pimbblet, Kevin A" sort="Pimbblet, Kevin A" uniqKey="Pimbblet K" first="Kevin A." last="Pimbblet">Kevin A. Pimbblet</name><affiliation><mods:affiliation>School of Physics, Monash University, Clayton, VIC 3800, Australia</mods:affiliation></affiliation></author><author><name sortKey="Rex, Marie" sort="Rex, Marie" uniqKey="Rex M" first="Marie" last="Rex">Marie Rex</name><affiliation><mods:affiliation>Steward Observatory, University of Arizona, 933 N. Chery Ave, Tucson, AZ 85721, USA</mods:affiliation></affiliation></author><author><name sortKey="Scott, Douglas" sort="Scott, Douglas" uniqKey="Scott D" first="Douglas" last="Scott">Douglas Scott</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></affiliation></author><author><name sortKey="Semisch, Christopher" sort="Semisch, Christopher" uniqKey="Semisch C" first="Christopher" last="Semisch">Christopher Semisch</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</mods:affiliation></affiliation></author><author><name sortKey="Thomas, Nicholas" sort="Thomas, Nicholas" uniqKey="Thomas N" first="Nicholas" last="Thomas">Nicholas Thomas</name><affiliation><mods:affiliation>Department of Physics, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33146, USA</mods:affiliation></affiliation></author><author><name sortKey="Truch, Matthew D P" sort="Truch, Matthew D P" uniqKey="Truch M" first="Matthew D. P." last="Truch">Matthew D. P. Truch</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</mods:affiliation></affiliation></author><author><name sortKey="Tucker, Carole" sort="Tucker, Carole" uniqKey="Tucker C" first="Carole" last="Tucker">Carole Tucker</name><affiliation><mods:affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</mods:affiliation></affiliation></author><author><name sortKey="Tucker, Gregory S" sort="Tucker, Gregory S" uniqKey="Tucker G" first="Gregory S." last="Tucker">Gregory S. Tucker</name><affiliation><mods:affiliation>Department of Physics, Brown University, 182 Hope Street, Providence, RI 02912, USA</mods:affiliation></affiliation></author><author><name sortKey="Valiante, Elisabetta" sort="Valiante, Elisabetta" uniqKey="Valiante E" first="Elisabetta" last="Valiante">Elisabetta Valiante</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></affiliation></author><author><name sortKey="Viero, Marco P" sort="Viero, Marco P" uniqKey="Viero M" first="Marco P." last="Viero">Marco P. Viero</name><affiliation><mods:affiliation>California Institute of Technology, 1200 E. California Blvd, Pasadena, CA 91125, USA</mods:affiliation></affiliation></author><author><name sortKey="Wiebe, Donald V" sort="Wiebe, Donald V" uniqKey="Wiebe D" first="Donald V." last="Wiebe">Donald V. Wiebe</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></affiliation></author></titleStmt><publicationStmt><idno type="wicri:source">ISTEX</idno><idno type="RBID">ISTEX:A6B192742E968B4F255CC383950810AB9DB59FB4</idno><date when="2011" year="2011">2011</date><idno type="doi">10.1111/j.1365-2966.2010.17973.x</idno><idno type="url">https://api.istex.fr/document/A6B192742E968B4F255CC383950810AB9DB59FB4/fulltext/pdf</idno><idno type="wicri:Area/Istex/Corpus">001F71</idno><idno type="wicri:explorRef" wicri:stream="Istex" wicri:step="Corpus" wicri:corpus="ISTEX">001F71</idno></publicationStmt><sourceDesc><biblStruct><analytic><title level="a" type="main">Submillimetre observations of galaxy clusters with the BLAST: the star formation activity in Abell 3112</title><author><name sortKey="Braglia, Filiberto G" sort="Braglia, Filiberto G" uniqKey="Braglia F" first="Filiberto G." last="Braglia">Filiberto G. Braglia</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></affiliation><affiliation><mods:affiliation>E-mail: fbraglia@phas.ubc.ca</mods:affiliation></affiliation></author><author><name sortKey="Ade, Peter A R" sort="Ade, Peter A R" uniqKey="Ade P" first="Peter A. R." last="Ade">Peter A. R. Ade</name><affiliation><mods:affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</mods:affiliation></affiliation></author><author><name sortKey="Bock, James J" sort="Bock, James J" uniqKey="Bock J" first="James J." last="Bock">James J. Bock</name><affiliation><mods:affiliation>Jet Propulsion Laboratory, Pasadena, CA 91109‐8099, USA</mods:affiliation></affiliation></author><author><name sortKey="Chapin, Edward L" sort="Chapin, Edward L" uniqKey="Chapin E" first="Edward L." last="Chapin">Edward L. Chapin</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></affiliation></author><author><name sortKey="Devlin, Mark J" sort="Devlin, Mark J" uniqKey="Devlin M" first="Mark J." last="Devlin">Mark J. Devlin</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</mods:affiliation></affiliation></author><author><name sortKey="Edge, Alastair" sort="Edge, Alastair" uniqKey="Edge A" first="Alastair" last="Edge">Alastair Edge</name><affiliation><mods:affiliation>Department of Physics, Durham University, South Road, Durham DH1 3LE</mods:affiliation></affiliation></author><author><name sortKey="Griffin, Matthew" sort="Griffin, Matthew" uniqKey="Griffin M" first="Matthew" last="Griffin">Matthew Griffin</name><affiliation><mods:affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</mods:affiliation></affiliation></author><author><name sortKey="Gundersen, Joshua O" sort="Gundersen, Joshua O" uniqKey="Gundersen J" first="Joshua O." last="Gundersen">Joshua O. Gundersen</name><affiliation><mods:affiliation>Department of Physics, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33146, USA</mods:affiliation></affiliation></author><author><name sortKey="Halpern, Mark" sort="Halpern, Mark" uniqKey="Halpern M" first="Mark" last="Halpern">Mark Halpern</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></affiliation></author><author><name sortKey="Hargrave, Peter C" sort="Hargrave, Peter C" uniqKey="Hargrave P" first="Peter C." last="Hargrave">Peter C. Hargrave</name><affiliation><mods:affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</mods:affiliation></affiliation></author><author><name sortKey="Hughes, David H" sort="Hughes, David H" uniqKey="Hughes D" first="David H." last="Hughes">David H. Hughes</name><affiliation><mods:affiliation>Instituto Nacional de Astrofísica Óptica y Electrónica (INAOE), Aptdo. Postal 51 y 72000 Puebla, Mexico</mods:affiliation></affiliation></author><author><name sortKey="Klein, Jeff" sort="Klein, Jeff" uniqKey="Klein J" first="Jeff" last="Klein">Jeff Klein</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</mods:affiliation></affiliation></author><author><name sortKey="Marsden, Gaelen" sort="Marsden, Gaelen" uniqKey="Marsden G" first="Gaelen" last="Marsden">Gaelen Marsden</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></affiliation></author><author><name sortKey="Mauskopf, Philip" sort="Mauskopf, Philip" uniqKey="Mauskopf P" first="Philip" last="Mauskopf">Philip Mauskopf</name><affiliation><mods:affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</mods:affiliation></affiliation></author><author><name sortKey="Moncelsi, Lorenzo" sort="Moncelsi, Lorenzo" uniqKey="Moncelsi L" first="Lorenzo" last="Moncelsi">Lorenzo Moncelsi</name><affiliation><mods:affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</mods:affiliation></affiliation></author><author><name sortKey="Netterfield, Calvin B" sort="Netterfield, Calvin B" uniqKey="Netterfield C" first="Calvin B." last="Netterfield">Calvin B. Netterfield</name><affiliation><mods:affiliation>Department of Astronomy & Astrophysics, University of Toronto, 50 St George Street Toronto, ON M5S 3H4, Canada</mods:affiliation></affiliation><affiliation><mods:affiliation>Department of Physics, University of Toronto, 60 St George Street, Toronto, ON M5S 1A7, Canada</mods:affiliation></affiliation></author><author><name sortKey="Ngo, Henry" sort="Ngo, Henry" uniqKey="Ngo H" first="Henry" last="Ngo">Henry Ngo</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></affiliation></author><author><name sortKey="Olmi, Luca" sort="Olmi, Luca" uniqKey="Olmi L" first="Luca" last="Olmi">Luca Olmi</name><affiliation><mods:affiliation>Physics Department, University of Puerto Rico, Rio Piedras Campus, Box 23343, UPR station, PR 00931, USA</mods:affiliation></affiliation><affiliation><mods:affiliation>INAF ‐ Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I‐50125 Firenze, Italy</mods:affiliation></affiliation></author><author><name sortKey="Pascale, Enzo" sort="Pascale, Enzo" uniqKey="Pascale E" first="Enzo" last="Pascale">Enzo Pascale</name><affiliation><mods:affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</mods:affiliation></affiliation></author><author><name sortKey="Patanchon, Guillaume" sort="Patanchon, Guillaume" uniqKey="Patanchon G" first="Guillaume" last="Patanchon">Guillaume Patanchon</name><affiliation><mods:affiliation>Université Paris Diderot, Laboratoire APC, 10, rue Alice Domon et Léonie Duquet, 75205 Paris, France</mods:affiliation></affiliation></author><author><name sortKey="Pimbblet, Kevin A" sort="Pimbblet, Kevin A" uniqKey="Pimbblet K" first="Kevin A." last="Pimbblet">Kevin A. Pimbblet</name><affiliation><mods:affiliation>School of Physics, Monash University, Clayton, VIC 3800, Australia</mods:affiliation></affiliation></author><author><name sortKey="Rex, Marie" sort="Rex, Marie" uniqKey="Rex M" first="Marie" last="Rex">Marie Rex</name><affiliation><mods:affiliation>Steward Observatory, University of Arizona, 933 N. Chery Ave, Tucson, AZ 85721, USA</mods:affiliation></affiliation></author><author><name sortKey="Scott, Douglas" sort="Scott, Douglas" uniqKey="Scott D" first="Douglas" last="Scott">Douglas Scott</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></affiliation></author><author><name sortKey="Semisch, Christopher" sort="Semisch, Christopher" uniqKey="Semisch C" first="Christopher" last="Semisch">Christopher Semisch</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</mods:affiliation></affiliation></author><author><name sortKey="Thomas, Nicholas" sort="Thomas, Nicholas" uniqKey="Thomas N" first="Nicholas" last="Thomas">Nicholas Thomas</name><affiliation><mods:affiliation>Department of Physics, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33146, USA</mods:affiliation></affiliation></author><author><name sortKey="Truch, Matthew D P" sort="Truch, Matthew D P" uniqKey="Truch M" first="Matthew D. P." last="Truch">Matthew D. P. Truch</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</mods:affiliation></affiliation></author><author><name sortKey="Tucker, Carole" sort="Tucker, Carole" uniqKey="Tucker C" first="Carole" last="Tucker">Carole Tucker</name><affiliation><mods:affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</mods:affiliation></affiliation></author><author><name sortKey="Tucker, Gregory S" sort="Tucker, Gregory S" uniqKey="Tucker G" first="Gregory S." last="Tucker">Gregory S. Tucker</name><affiliation><mods:affiliation>Department of Physics, Brown University, 182 Hope Street, Providence, RI 02912, USA</mods:affiliation></affiliation></author><author><name sortKey="Valiante, Elisabetta" sort="Valiante, Elisabetta" uniqKey="Valiante E" first="Elisabetta" last="Valiante">Elisabetta Valiante</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></affiliation></author><author><name sortKey="Viero, Marco P" sort="Viero, Marco P" uniqKey="Viero M" first="Marco P." last="Viero">Marco P. Viero</name><affiliation><mods:affiliation>California Institute of Technology, 1200 E. California Blvd, Pasadena, CA 91125, USA</mods:affiliation></affiliation></author><author><name sortKey="Wiebe, Donald V" sort="Wiebe, Donald V" uniqKey="Wiebe D" first="Donald V." last="Wiebe">Donald V. Wiebe</name><affiliation><mods:affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation></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">412</biblScope><biblScope unit="issue">2</biblScope><biblScope unit="page" from="1187">1187</biblScope><biblScope unit="page" to="1202">1202</biblScope><biblScope unit="page-count">16</biblScope><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2011-04-01">2011-04-01</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>Abell</term><term>Average ssfr</term><term>Biviano</term><term>Blast</term><term>Blast bands</term><term>Blast catalogue</term><term>Blast counterparts</term><term>Blast data</term><term>Blast maps</term><term>Blast observations</term><term>Blast sources</term><term>Blast wavelengths</term><term>Blue galaxies</term><term>Boxes mark</term><term>Braglia</term><term>Brightest cluster galaxy</term><term>California institute</term><term>Central galaxy</term><term>Characteristic magnitude</term><term>Cluster</term><term>Cluster centre</term><term>Cluster core</term><term>Cluster diagram</term><term>Cluster galaxies</term><term>Cluster member</term><term>Cluster member catalogue</term><term>Cluster members</term><term>Cluster redshift</term><term>Clustercentric</term><term>Clustercentric distances</term><term>Clustercentric radius</term><term>Cold dust</term><term>Colour</term><term>Colours</term><term>Devlin</term><term>Distance scale</term><term>Dust content</term><term>Dust masses</term><term>Emission lines</term><term>Environmental effects</term><term>Flux densities</term><term>Galaxy</term><term>Galaxy clusters</term><term>Galaxy geometry</term><term>Global decrease</term><term>Good agreement</term><term>Haines</term><term>Inclination angle</term><term>Individual sources</term><term>Infall region</term><term>Instrumental counts</term><term>Instrumental noise</term><term>Ira</term><term>Iras source</term><term>Lamentary structures</term><term>Large aperture submillimeter telescope</term><term>Large fraction</term><term>Large sample</term><term>Large spirals</term><term>Largest part</term><term>Line marks</term><term>Lines mark</term><term>Luminosity</term><term>Mnras</term><term>Monthly notices</term><term>Normal galaxies</term><term>Normal starforming galaxies</term><term>Notable drop</term><term>Number counts</term><term>Optical cluster members</term><term>Optical colour</term><term>Optical colours</term><term>Optical counterparts</term><term>Optical spectra</term><term>Optical spectroscopy</term><term>Optical spectrum</term><term>Panels show</term><term>Pascale</term><term>Photometry</term><term>Physics astronomy</term><term>Pierini</term><term>Porter raychaudhury</term><term>Positional uncertainty</term><term>Potential cluster members</term><term>Previous results</term><term>Previous studies</term><term>Propulsion laboratory</term><term>Radial bins</term><term>Radial distribution</term><term>Radial peak</term><term>Radial trends</term><term>Random occurrence</term><term>Redshift</term><term>Rejection probability</term><term>Robust</term><term>Same area</term><term>Same method</term><term>Seds</term><term>Sfrs</term><term>Solid line</term><term>Source catalogue</term><term>Source extraction</term><term>Spectral region</term><term>Spectroscopic</term><term>Spectroscopic catalogue</term><term>Ssfr</term><term>Star formation</term><term>Star formation activity</term><term>Stellar</term><term>Stellar mass</term><term>Stellar masses</term><term>Stellar population</term><term>Submm</term><term>Submm emission</term><term>Submm wavelengths</term><term>Unobscured star formation activity</term><term>Upper limit</term><term>Vertical lines mark</term><term>Wavelength</term></keywords><keywords scheme="Teeft" xml:lang="en"><term>Abell</term><term>Average ssfr</term><term>Biviano</term><term>Blast</term><term>Blast bands</term><term>Blast catalogue</term><term>Blast counterparts</term><term>Blast data</term><term>Blast maps</term><term>Blast observations</term><term>Blast sources</term><term>Blast wavelengths</term><term>Blue galaxies</term><term>Boxes mark</term><term>Braglia</term><term>Brightest cluster galaxy</term><term>California institute</term><term>Central galaxy</term><term>Characteristic magnitude</term><term>Cluster</term><term>Cluster centre</term><term>Cluster core</term><term>Cluster diagram</term><term>Cluster galaxies</term><term>Cluster member</term><term>Cluster member catalogue</term><term>Cluster members</term><term>Cluster redshift</term><term>Clustercentric</term><term>Clustercentric distances</term><term>Clustercentric radius</term><term>Cold dust</term><term>Colour</term><term>Colours</term><term>Devlin</term><term>Distance scale</term><term>Dust content</term><term>Dust masses</term><term>Emission lines</term><term>Environmental effects</term><term>Flux densities</term><term>Galaxy</term><term>Galaxy clusters</term><term>Galaxy geometry</term><term>Global decrease</term><term>Good agreement</term><term>Haines</term><term>Inclination angle</term><term>Individual sources</term><term>Infall region</term><term>Instrumental counts</term><term>Instrumental noise</term><term>Ira</term><term>Iras source</term><term>Lamentary structures</term><term>Large aperture submillimeter telescope</term><term>Large fraction</term><term>Large sample</term><term>Large spirals</term><term>Largest part</term><term>Line marks</term><term>Lines mark</term><term>Luminosity</term><term>Mnras</term><term>Monthly notices</term><term>Normal galaxies</term><term>Normal starforming galaxies</term><term>Notable drop</term><term>Number counts</term><term>Optical cluster members</term><term>Optical colour</term><term>Optical colours</term><term>Optical counterparts</term><term>Optical spectra</term><term>Optical spectroscopy</term><term>Optical spectrum</term><term>Panels show</term><term>Pascale</term><term>Photometry</term><term>Physics astronomy</term><term>Pierini</term><term>Porter raychaudhury</term><term>Positional uncertainty</term><term>Potential cluster members</term><term>Previous results</term><term>Previous studies</term><term>Propulsion laboratory</term><term>Radial bins</term><term>Radial distribution</term><term>Radial peak</term><term>Radial trends</term><term>Random occurrence</term><term>Redshift</term><term>Rejection probability</term><term>Robust</term><term>Same area</term><term>Same method</term><term>Seds</term><term>Sfrs</term><term>Solid line</term><term>Source catalogue</term><term>Source extraction</term><term>Spectral region</term><term>Spectroscopic</term><term>Spectroscopic catalogue</term><term>Ssfr</term><term>Star formation</term><term>Star formation activity</term><term>Stellar</term><term>Stellar mass</term><term>Stellar masses</term><term>Stellar population</term><term>Submm</term><term>Submm emission</term><term>Submm wavelengths</term><term>Unobscured star formation activity</term><term>Upper limit</term><term>Vertical lines mark</term><term>Wavelength</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We present observations at 250, 350 and 500 μm of the nearby galaxy cluster Abell 3112 (z= 0.075) carried out with the Balloon‐borne Large Aperture Submillimeter Telescope. Five cluster members are individually detected as bright submillimetre (submm) sources. Their far‐infrared spectral energy distributions and optical colours identify them as normal star‐forming galaxies of high mass, with globally evolved stellar populations. They all have (B−R) colours of 1.38 ± 0.08, transitional between the blue, active population and the red, evolved galaxies that dominate the cluster core. We stack to estimate the mean submm emission from all cluster members, which is determined to be 16.6 ± 2.5, 6.1 ± 1.9 and 1.5 ± 1.3 mJy at 250, 350 and 500 μm, respectively. Stacking analyses of the submm emission of cluster members reveal trends in the mean far‐infrared luminosity with respect to clustercentric radius and KS‐band magnitude. We find that a large fraction of submm emission comes from the boundary of the inner, virialized region of the cluster, at clustercentric distances around R500. Stacking also shows that the bulk of the submm emission arises in intermediate‐mass galaxies with KS magnitude ∼1 mag fainter than the characteristic magnitude . The results and constraints obtained in this work will provide a useful reference for the forthcoming surveys to be conducted on galaxy clusters by Herschel.</div></front></TEI><istex><corpusName>wiley</corpusName><keywords><teeft><json:string>cluster members</json:string><json:string>submm</json:string><json:string>mnras</json:string><json:string>redshift</json:string><json:string>galaxy</json:string><json:string>colour</json:string><json:string>submm emission</json:string><json:string>monthly notices</json:string><json:string>cluster galaxies</json:string><json:string>star formation activity</json:string><json:string>braglia</json:string><json:string>pierini</json:string><json:string>clustercentric</json:string><json:string>ssfr</json:string><json:string>robust</json:string><json:string>spectroscopic</json:string><json:string>blast counterparts</json:string><json:string>photometry</json:string><json:string>colours</json:string><json:string>biviano</json:string><json:string>blast observations</json:string><json:string>luminosity</json:string><json:string>blast sources</json:string><json:string>haines</json:string><json:string>galaxy clusters</json:string><json:string>star formation</json:string><json:string>devlin</json:string><json:string>seds</json:string><json:string>sfrs</json:string><json:string>pascale</json:string><json:string>abell</json:string><json:string>cluster</json:string><json:string>submm wavelengths</json:string><json:string>stellar mass</json:string><json:string>stellar</json:string><json:string>blue galaxies</json:string><json:string>environmental effects</json:string><json:string>individual sources</json:string><json:string>cluster redshift</json:string><json:string>positional uncertainty</json:string><json:string>large fraction</json:string><json:string>cluster member</json:string><json:string>clustercentric radius</json:string><json:string>blast maps</json:string><json:string>blast wavelengths</json:string><json:string>normal galaxies</json:string><json:string>dust content</json:string><json:string>ira</json:string><json:string>blast</json:string><json:string>propulsion laboratory</json:string><json:string>optical colours</json:string><json:string>california institute</json:string><json:string>spectral region</json:string><json:string>brightest cluster galaxy</json:string><json:string>upper limit</json:string><json:string>optical cluster members</json:string><json:string>cluster centre</json:string><json:string>lines mark</json:string><json:string>characteristic magnitude</json:string><json:string>central galaxy</json:string><json:string>dust masses</json:string><json:string>cluster core</json:string><json:string>spectroscopic catalogue</json:string><json:string>physics astronomy</json:string><json:string>wavelength</json:string><json:string>solid line</json:string><json:string>instrumental noise</json:string><json:string>optical counterparts</json:string><json:string>lamentary structures</json:string><json:string>number counts</json:string><json:string>same area</json:string><json:string>optical spectroscopy</json:string><json:string>global decrease</json:string><json:string>blast catalogue</json:string><json:string>flux densities</json:string><json:string>boxes mark</json:string><json:string>unobscured star formation activity</json:string><json:string>largest part</json:string><json:string>source catalogue</json:string><json:string>previous studies</json:string><json:string>clustercentric distances</json:string><json:string>distance scale</json:string><json:string>large aperture submillimeter telescope</json:string><json:string>cluster diagram</json:string><json:string>normal starforming galaxies</json:string><json:string>stellar masses</json:string><json:string>cluster member catalogue</json:string><json:string>blast bands</json:string><json:string>good agreement</json:string><json:string>infall region</json:string><json:string>iras source</json:string><json:string>same method</json:string><json:string>large sample</json:string><json:string>blast data</json:string><json:string>previous results</json:string><json:string>large spirals</json:string><json:string>emission lines</json:string><json:string>optical spectrum</json:string><json:string>optical spectra</json:string><json:string>vertical lines mark</json:string><json:string>instrumental counts</json:string><json:string>source extraction</json:string><json:string>cold dust</json:string><json:string>stellar population</json:string><json:string>optical colour</json:string><json:string>inclination angle</json:string><json:string>radial distribution</json:string><json:string>galaxy geometry</json:string><json:string>porter raychaudhury</json:string><json:string>panels show</json:string><json:string>random occurrence</json:string><json:string>radial peak</json:string><json:string>rejection probability</json:string><json:string>notable drop</json:string><json:string>radial bins</json:string><json:string>average ssfr</json:string><json:string>radial trends</json:string><json:string>line marks</json:string><json:string>potential cluster members</json:string></teeft></keywords><author><json:item><name>Filiberto G. Braglia</name><affiliations><json:string>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</json:string><json:string>E-mail: fbraglia@phas.ubc.ca</json:string></affiliations></json:item><json:item><name>Peter A. R. Ade</name><affiliations><json:string>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</json:string></affiliations></json:item><json:item><name>James J. Bock</name><affiliations><json:string>Jet Propulsion Laboratory, Pasadena, CA 91109‐8099, USA</json:string></affiliations></json:item><json:item><name>Edward L. Chapin</name><affiliations><json:string>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</json:string></affiliations></json:item><json:item><name>Mark J. Devlin</name><affiliations><json:string>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</json:string></affiliations></json:item><json:item><name>Alastair Edge</name><affiliations><json:string>Department of Physics, Durham University, South Road, Durham DH1 3LE</json:string></affiliations></json:item><json:item><name>Matthew Griffin</name><affiliations><json:string>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</json:string></affiliations></json:item><json:item><name>Joshua O. Gundersen</name><affiliations><json:string>Department of Physics, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33146, USA</json:string></affiliations></json:item><json:item><name>Mark Halpern</name><affiliations><json:string>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</json:string></affiliations></json:item><json:item><name>Peter C. Hargrave</name><affiliations><json:string>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</json:string></affiliations></json:item><json:item><name>David H. Hughes</name><affiliations><json:string>Instituto Nacional de Astrofísica Óptica y Electrónica (INAOE), Aptdo. Postal 51 y 72000 Puebla, Mexico</json:string></affiliations></json:item><json:item><name>Jeff Klein</name><affiliations><json:string>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</json:string></affiliations></json:item><json:item><name>Gaelen Marsden</name><affiliations><json:string>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</json:string></affiliations></json:item><json:item><name>Philip Mauskopf</name><affiliations><json:string>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</json:string></affiliations></json:item><json:item><name>Lorenzo Moncelsi</name><affiliations><json:string>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</json:string></affiliations></json:item><json:item><name>Calvin B. Netterfield</name><affiliations><json:string>Department of Astronomy & Astrophysics, University of Toronto, 50 St George Street Toronto, ON M5S 3H4, Canada</json:string><json:string>Department of Physics, University of Toronto, 60 St George Street, Toronto, ON M5S 1A7, Canada</json:string></affiliations></json:item><json:item><name>Henry Ngo</name><affiliations><json:string>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</json:string></affiliations></json:item><json:item><name>Luca Olmi</name><affiliations><json:string>Physics Department, University of Puerto Rico, Rio Piedras Campus, Box 23343, UPR station, PR 00931, USA</json:string><json:string>INAF ‐ Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I‐50125 Firenze, Italy</json:string></affiliations></json:item><json:item><name>Enzo Pascale</name><affiliations><json:string>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</json:string></affiliations></json:item><json:item><name>Guillaume Patanchon</name><affiliations><json:string>Université Paris Diderot, Laboratoire APC, 10, rue Alice Domon et Léonie Duquet, 75205 Paris, France</json:string></affiliations></json:item><json:item><name>Kevin A. Pimbblet</name><affiliations><json:string>School of Physics, Monash University, Clayton, VIC 3800, Australia</json:string></affiliations></json:item><json:item><name>Marie Rex</name><affiliations><json:string>Steward Observatory, University of Arizona, 933 N. Chery Ave, Tucson, AZ 85721, USA</json:string></affiliations></json:item><json:item><name>Douglas Scott</name><affiliations><json:string>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</json:string></affiliations></json:item><json:item><name>Christopher Semisch</name><affiliations><json:string>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</json:string></affiliations></json:item><json:item><name>Nicholas Thomas</name><affiliations><json:string>Department of Physics, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33146, USA</json:string></affiliations></json:item><json:item><name>Matthew D. P. Truch</name><affiliations><json:string>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</json:string></affiliations></json:item><json:item><name>Carole Tucker</name><affiliations><json:string>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</json:string></affiliations></json:item><json:item><name>Gregory S. Tucker</name><affiliations><json:string>Department of Physics, Brown University, 182 Hope Street, Providence, RI 02912, USA</json:string></affiliations></json:item><json:item><name>Elisabetta Valiante</name><affiliations><json:string>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</json:string></affiliations></json:item><json:item><name>Marco P. Viero</name><affiliations><json:string>California Institute of Technology, 1200 E. California Blvd, Pasadena, CA 91125, USA</json:string></affiliations></json:item><json:item><name>Donald V. Wiebe</name><affiliations><json:string>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</json:string></affiliations></json:item></author><subject><json:item><lang><json:string>eng</json:string></lang><value>galaxies: clusters: general</value></json:item><json:item><lang><json:string>eng</json:string></lang><value>galaxies: clusters: individual: A3112</value></json:item><json:item><lang><json:string>eng</json:string></lang><value>galaxies: evolution</value></json:item><json:item><lang><json:string>eng</json:string></lang><value>galaxies: star formation</value></json:item><json:item><lang><json:string>eng</json:string></lang><value>infrared: galaxies</value></json:item><json:item><lang><json:string>eng</json:string></lang><value>submillimetre: galaxies</value></json:item></subject><articleId><json:string>MNR17973</json:string></articleId><arkIstex>ark:/67375/WNG-GCRTFB37-C</arkIstex><language><json:string>eng</json:string></language><originalGenre><json:string>article</json:string></originalGenre><abstract>We present observations at 250, 350 and 500 μm of the nearby galaxy cluster Abell 3112 (z= 0.075) carried out with the Balloon‐borne Large Aperture Submillimeter Telescope. Five cluster members are individually detected as bright submillimetre (submm) sources. Their far‐infrared spectral energy distributions and optical colours identify them as normal star‐forming galaxies of high mass, with globally evolved stellar populations. They all have (B−R) colours of 1.38 ± 0.08, transitional between the blue, active population and the red, evolved galaxies that dominate the cluster core. We stack to estimate the mean submm emission from all cluster members, which is determined to be 16.6 ± 2.5, 6.1 ± 1.9 and 1.5 ± 1.3 mJy at 250, 350 and 500 μm, respectively. Stacking analyses of the submm emission of cluster members reveal trends in the mean far‐infrared luminosity with respect to clustercentric radius and KS‐band magnitude. We find that a large fraction of submm emission comes from the boundary of the inner, virialized region of the cluster, at clustercentric distances around R500. Stacking also shows that the bulk of the submm emission arises in intermediate‐mass galaxies with KS magnitude ∼1 mag fainter than the characteristic magnitude . The results and constraints obtained in this work will provide a useful reference for the forthcoming surveys to be conducted on galaxy clusters by Herschel.</abstract><qualityIndicators><score>9.616</score><pdfWordCount>10521</pdfWordCount><pdfCharCount>57451</pdfCharCount><pdfVersion>1.4</pdfVersion><pdfPageCount>16</pdfPageCount><pdfPageSize>595.274 x 782.286 pts</pdfPageSize><refBibsNative>true</refBibsNative><abstractWordCount>218</abstractWordCount><abstractCharCount>1413</abstractCharCount><keywordCount>6</keywordCount></qualityIndicators><title>Submillimetre observations of galaxy clusters with the BLAST: the star formation activity in Abell 3112</title><genre><json:string>article</json:string></genre><host><title>Monthly Notices of the Royal Astronomical Society</title><language><json:string>unknown</json:string></language><doi><json:string>10.1111/(ISSN)1365-2966</json:string></doi><issn><json:string>0035-8711</json:string></issn><eissn><json:string>1365-2966</json:string></eissn><publisherId><json:string>MNR</json:string></publisherId><volume>412</volume><issue>2</issue><pages><first>1187</first><last>1202</last><total>16</total></pages><genre><json:string>journal</json:string></genre></host><namedEntities><unitex><date><json:string>2011</json:string><json:string>2006</json:string></date><geogName></geogName><orgName><json:string>Department of Physics, University of Toronto</json:string><json:string>University of Toronto</json:string><json:string>National Science Foundation</json:string><json:string>Department of Physics, Durham University, South Road, Durham DH</json:string><json:string>Cardiff University</json:string><json:string>Monash University</json:string><json:string>University of Arizona</json:string><json:string>NSERC</json:string><json:string>Engineering Research Council</json:string><json:string>University of Massachusetts</json:string><json:string>Infrared Processing and Analysis Center</json:string><json:string>California Institute of Technology</json:string><json:string>Jet Propulsion Laboratory, Pasadena, CA</json:string><json:string>Jet Propulsion Laboratory, California Institute of Technology</json:string><json:string>Department of Physics</json:string><json:string>Canada, and the UK Science and Technology</json:string><json:string>Department of Physics, Brown University</json:string><json:string>Canada of Physics</json:string><json:string>Department of Astronomy</json:string><json:string>University of Pennsylvania</json:string><json:string>Physics Department, University of Puerto Rico, Rio Piedras Campus, Box</json:string><json:string>Canadian Space Agency</json:string></orgName><orgName_funder></orgName_funder><orgName_provider></orgName_provider><persName><json:string>Hope Street</json:string><json:string>Sky Survey</json:string><json:string>Nicholas Thomas</json:string><json:string>Stacking</json:string><json:string>Joshua O. Gundersen</json:string><json:string>Jeff Klein</json:string><json:string>Christopher Semisch</json:string><json:string>Edward L. Chapin</json:string><json:string>Daniele Pierini</json:string><json:string>Alastair Edge</json:string><json:string>Mark J. Devlin</json:string><json:string>D. P. Truch</json:string><json:string>David H. Hughes</json:string><json:string>Lorenzo Moncelsi</json:string><json:string>Coral Gables</json:string><json:string>A. R. Ade</json:string><json:string>Filiberto G. Braglia</json:string><json:string>Paris Diderot</json:string><json:string>Luca Olmi</json:string><json:string>Gregory S. Tucker</json:string><json:string>James J. Bock</json:string><json:string>Alice Domon</json:string><json:string>Marie Rex</json:string><json:string>Discs</json:string><json:string>Observatory</json:string><json:string>Guillaume Patanchon</json:string><json:string>Henry Ngo</json:string><json:string>Mark Halpern</json:string><json:string>Largo E. Fermi</json:string><json:string>Donald V. Wiebe</json:string><json:string>E. California</json:string><json:string>Carole Tucker</json:string><json:string>Calvin B. Netter</json:string><json:string>Enzo Pascale</json:string><json:string>Philip Mauskopf</json:string><json:string>Marco P. Viero</json:string><json:string>George Street</json:string><json:string>Douglas Scott</json:string><json:string>Peter C. Hargrave</json:string><json:string>Kevin A. 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(2009)</json:string><json:string>Gallazzi et al. 2009</json:string><json:string>Marsden et al. 2009</json:string><json:string>Sanderson et al. 2003</json:string></ref_bibl><bibl></bibl></unitex></namedEntities><ark><json:string>ark:/67375/WNG-GCRTFB37-C</json:string></ark><categories><wos><json:string>1 - science</json:string><json:string>2 - astronomy & astrophysics</json:string></wos><scienceMetrix><json:string>1 - natural sciences</json:string><json:string>2 - physics & astronomy</json:string><json:string>3 - astronomy & astrophysics</json:string></scienceMetrix><scopus><json:string>1 - Physical Sciences</json:string><json:string>2 - Earth and Planetary Sciences</json:string><json:string>3 - Space and Planetary Science</json:string><json:string>1 - Physical Sciences</json:string><json:string>2 - Physics and Astronomy</json:string><json:string>3 - Astronomy and Astrophysics</json:string></scopus><inist><json:string>1 - sciences appliquees, technologies et medecines</json:string><json:string>2 - sciences exactes et technologie</json:string><json:string>3 - terre, ocean, espace</json:string><json:string>4 - astronomie</json:string></inist></categories><publicationDate>2011</publicationDate><copyrightDate>2011</copyrightDate><doi><json:string>10.1111/j.1365-2966.2010.17973.x</json:string></doi><id>A6B192742E968B4F255CC383950810AB9DB59FB4</id><score>1</score><fulltext><json:item><extension>pdf</extension><original>true</original><mimetype>application/pdf</mimetype><uri>https://api.istex.fr/document/A6B192742E968B4F255CC383950810AB9DB59FB4/fulltext/pdf</uri></json:item><json:item><extension>zip</extension><original>false</original><mimetype>application/zip</mimetype><uri>https://api.istex.fr/document/A6B192742E968B4F255CC383950810AB9DB59FB4/fulltext/zip</uri></json:item><istex:fulltextTEI uri="https://api.istex.fr/document/A6B192742E968B4F255CC383950810AB9DB59FB4/fulltext/tei"><teiHeader><fileDesc><titleStmt><title level="a" type="main">Submillimetre observations of galaxy clusters with the BLAST: the star formation activity in Abell 3112</title></titleStmt><publicationStmt><authority>ISTEX</authority><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><availability><licence>© 2010 The Authors Monthly Notices of the Royal Astronomical Society © 2010 RAS</licence></availability><date type="published" when="2011-04-01"></date></publicationStmt><notesStmt><note type="content-type" subtype="article" source="article" scheme="https://content-type.data.istex.fr/ark:/67375/XTP-6N5SZHKN-D">article</note><note type="publication-type" subtype="journal" scheme="https://publication-type.data.istex.fr/ark:/67375/JMC-0GLKJH51-B">journal</note></notesStmt><sourceDesc><biblStruct type="article"><analytic><title level="a" type="main">Submillimetre observations of galaxy clusters with the BLAST: the star formation activity in Abell 3112</title><title level="a" type="short">BLAST observations of Abell 3112</title><author xml:id="author-0000" role="corresp"><persName><forename type="first">Filiberto G.</forename><surname>Braglia</surname></persName><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada<address><country key="CA"></country></address></affiliation><affiliation>E‐mail: fbraglia@phas.ubc.ca</affiliation></author><author xml:id="author-0001"><persName><forename type="first">Peter A. R.</forename><surname>Ade</surname></persName><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation></author><author xml:id="author-0002"><persName><forename type="first">James J.</forename><surname>Bock</surname></persName><affiliation>Jet Propulsion Laboratory, Pasadena, CA 91109‐8099, USA<address><country key="US"></country></address></affiliation></author><author xml:id="author-0003"><persName><forename type="first">Edward L.</forename><surname>Chapin</surname></persName><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada<address><country key="CA"></country></address></affiliation></author><author xml:id="author-0004"><persName><forename type="first">Mark J.</forename><surname>Devlin</surname></persName><affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA<address><country key="US"></country></address></affiliation></author><author xml:id="author-0005"><persName><forename type="first">Alastair</forename><surname>Edge</surname></persName><affiliation>Department of Physics, Durham University, South Road, Durham DH1 3LE</affiliation></author><author xml:id="author-0006"><persName><forename type="first">Matthew</forename><surname>Griffin</surname></persName><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation></author><author xml:id="author-0007"><persName><forename type="first">Joshua O.</forename><surname>Gundersen</surname></persName><affiliation>Department of Physics, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33146, USA<address><country key="US"></country></address></affiliation></author><author xml:id="author-0008"><persName><forename type="first">Mark</forename><surname>Halpern</surname></persName><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada<address><country key="CA"></country></address></affiliation></author><author xml:id="author-0009"><persName><forename type="first">Peter C.</forename><surname>Hargrave</surname></persName><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation></author><author xml:id="author-0010"><persName><forename type="first">David H.</forename><surname>Hughes</surname></persName><affiliation>Instituto Nacional de Astrofísica Óptica y Electrónica (INAOE), Aptdo. Postal 51 y 72000 Puebla, Mexico<address><country key="MX"></country></address></affiliation></author><author xml:id="author-0011"><persName><forename type="first">Jeff</forename><surname>Klein</surname></persName><affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA<address><country key="US"></country></address></affiliation></author><author xml:id="author-0012"><persName><forename type="first">Gaelen</forename><surname>Marsden</surname></persName><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada<address><country key="CA"></country></address></affiliation></author><author xml:id="author-0013"><persName><forename type="first">Philip</forename><surname>Mauskopf</surname></persName><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation></author><author xml:id="author-0014"><persName><forename type="first">Lorenzo</forename><surname>Moncelsi</surname></persName><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation></author><author xml:id="author-0015"><persName><forename type="first">Calvin B.</forename><surname>Netterfield</surname></persName><affiliation>Department of Astronomy & Astrophysics, University of Toronto, 50 St George Street Toronto, ON M5S 3H4, Canada<address><country key="CA"></country></address></affiliation><affiliation>Department of Physics, University of Toronto, 60 St George Street, Toronto, ON M5S 1A7, Canada<address><country key="CA"></country></address></affiliation></author><author xml:id="author-0016"><persName><forename type="first">Henry</forename><surname>Ngo</surname></persName><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada<address><country key="CA"></country></address></affiliation></author><author xml:id="author-0017"><persName><forename type="first">Luca</forename><surname>Olmi</surname></persName><affiliation>Physics Department, University of Puerto Rico, Rio Piedras Campus, Box 23343, UPR station, PR 00931, USA<address><country key="US"></country></address></affiliation><affiliation>INAF ‐ Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I‐50125 Firenze, Italy<address><country key="IT"></country></address></affiliation></author><author xml:id="author-0018"><persName><forename type="first">Enzo</forename><surname>Pascale</surname></persName><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation></author><author xml:id="author-0019"><persName><forename type="first">Guillaume</forename><surname>Patanchon</surname></persName><affiliation>Université Paris Diderot, Laboratoire APC, 10, rue Alice Domon et Léonie Duquet, 75205 Paris, France<address><country key="FR"></country></address></affiliation></author><author xml:id="author-0020"><persName><forename type="first">Kevin A.</forename><surname>Pimbblet</surname></persName><affiliation>School of Physics, Monash University, Clayton, VIC 3800, Australia<address><country key="AU"></country></address></affiliation><note type="foot">Correction added after online publication 2011 February 22: author affiliation amended.</note></author><author xml:id="author-0021"><persName><forename type="first">Marie</forename><surname>Rex</surname></persName><affiliation>Steward Observatory, University of Arizona, 933 N. Chery Ave, Tucson, AZ 85721, USA<address><country key="US"></country></address></affiliation></author><author xml:id="author-0022"><persName><forename type="first">Douglas</forename><surname>Scott</surname></persName><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada<address><country key="CA"></country></address></affiliation></author><author xml:id="author-0023"><persName><forename type="first">Christopher</forename><surname>Semisch</surname></persName><affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA<address><country key="US"></country></address></affiliation></author><author xml:id="author-0024"><persName><forename type="first">Nicholas</forename><surname>Thomas</surname></persName><affiliation>Department of Physics, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33146, USA<address><country key="US"></country></address></affiliation></author><author xml:id="author-0025"><persName><forename type="first">Matthew D. P.</forename><surname>Truch</surname></persName><affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA<address><country key="US"></country></address></affiliation></author><author xml:id="author-0026"><persName><forename type="first">Carole</forename><surname>Tucker</surname></persName><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation></author><author xml:id="author-0027"><persName><forename type="first">Gregory S.</forename><surname>Tucker</surname></persName><affiliation>Department of Physics, Brown University, 182 Hope Street, Providence, RI 02912, USA<address><country key="US"></country></address></affiliation></author><author xml:id="author-0028"><persName><forename type="first">Elisabetta</forename><surname>Valiante</surname></persName><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada<address><country key="CA"></country></address></affiliation></author><author xml:id="author-0029"><persName><forename type="first">Marco P.</forename><surname>Viero</surname></persName><affiliation>California Institute of Technology, 1200 E. California Blvd, Pasadena, CA 91125, USA<address><country key="US"></country></address></affiliation></author><author xml:id="author-0030"><persName><forename type="first">Donald V.</forename><surname>Wiebe</surname></persName><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada<address><country key="CA"></country></address></affiliation></author><idno type="istex">A6B192742E968B4F255CC383950810AB9DB59FB4</idno><idno type="ark">ark:/67375/WNG-GCRTFB37-C</idno><idno type="DOI">10.1111/j.1365-2966.2010.17973.x</idno><idno type="unit">MNR17973</idno><idno type="toTypesetVersion">file:MNR.MNR17973.pdf</idno></analytic><monogr><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="pISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><idno type="book-DOI">10.1111/(ISSN)1365-2966</idno><idno type="book-part-DOI">10.1111/mnr.2011.412.issue-2</idno><idno type="product">MNR</idno><idno type="publisherDivision">ST</idno><imprint><biblScope unit="vol">412</biblScope><biblScope unit="issue">2</biblScope><biblScope unit="page" from="1187">1187</biblScope><biblScope unit="page" to="1202">1202</biblScope><biblScope unit="page-count">16</biblScope><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2011-04-01"></date></imprint></monogr></biblStruct></sourceDesc></fileDesc><profileDesc><abstract xml:lang="en" style="main"><head>ABSTRACT</head><p>We present observations at 250, 350 and 500 μm of the nearby galaxy cluster Abell 3112 (<hi rend="italic">z</hi>= 0.075) carried out with the Balloon‐borne Large Aperture Submillimeter Telescope. Five cluster members are individually detected as bright submillimetre (submm) sources. Their far‐infrared spectral energy distributions and optical colours identify them as normal star‐forming galaxies of high mass, with globally evolved stellar populations. They all have <emph><span>(<hi rend="italic">B</hi>−<hi rend="italic">R</hi>)</span></emph> colours of 1.38 ± 0.08, transitional between the blue, active population and the red, evolved galaxies that dominate the cluster core. We stack to estimate the mean submm emission from all cluster members, which is determined to be 16.6 ± 2.5, 6.1 ± 1.9 and 1.5 ± 1.3 mJy at 250, 350 and 500 μm, respectively. Stacking analyses of the submm emission of cluster members reveal trends in the mean far‐infrared luminosity with respect to clustercentric radius and <hi rend="italic">K</hi><hi rend="subscript">S</hi>‐band magnitude. We find that a large fraction of submm emission comes from the boundary of the inner, virialized region of the cluster, at clustercentric distances around <hi rend="italic">R</hi><hi rend="subscript">500</hi>. Stacking also shows that the bulk of the submm emission arises in intermediate‐mass galaxies with <hi rend="italic">K</hi><hi rend="subscript">S</hi> magnitude ∼1 mag fainter than the characteristic magnitude <graphic url="equation/MNR_17973_mu1.gif" rend="inline image"></graphic>. The results and constraints obtained in this work will provide a useful reference for the forthcoming surveys to be conducted on galaxy clusters by <hi rend="italic">Herschel</hi>.</p></abstract><textClass><keywords xml:lang="en"><term xml:id="k1">galaxies: clusters: general</term><term xml:id="k2">galaxies: clusters: individual: A3112</term><term xml:id="k3">galaxies: evolution</term><term xml:id="k4">galaxies: star formation</term><term xml:id="k5">infrared: galaxies</term><term xml:id="k6">submillimetre: galaxies</term></keywords><keywords rend="tocHeading1"><term>Papers</term></keywords></textClass><langUsage><language ident="en"></language></langUsage></profileDesc></teiHeader></istex:fulltextTEI><json:item><extension>txt</extension><original>false</original><mimetype>text/plain</mimetype><uri>https://api.istex.fr/document/A6B192742E968B4F255CC383950810AB9DB59FB4/fulltext/txt</uri></json:item></fulltext><metadata><istex:metadataXml wicri:clean="Wiley, elements deleted: body"><istex:xmlDeclaration>version="1.0" encoding="UTF-8" standalone="yes"</istex:xmlDeclaration><istex:document><component version="2.0" type="serialArticle" xml:lang="en"><header><publicationMeta level="product"><publisherInfo><publisherName>Blackwell Publishing Ltd</publisherName><publisherLoc>Oxford, UK</publisherLoc></publisherInfo><doi origin="wiley" registered="yes">10.1111/(ISSN)1365-2966</doi><issn type="print">0035-8711</issn><issn type="electronic">1365-2966</issn><idGroup><id type="product" value="MNR"></id><id type="publisherDivision" value="ST"></id></idGroup><titleGroup><title type="main" sort="MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY">Monthly Notices of the Royal Astronomical Society</title></titleGroup></publicationMeta><publicationMeta level="part" position="04102"><doi origin="wiley">10.1111/mnr.2011.412.issue-2</doi><numberingGroup><numbering type="journalVolume" number="412">412</numbering><numbering type="journalIssue" number="2">2</numbering></numberingGroup><coverDate startDate="2011-04-01">April 2011</coverDate></publicationMeta><publicationMeta level="unit" type="article" position="38" status="forIssue"><doi origin="wiley">10.1111/j.1365-2966.2010.17973.x</doi><idGroup><id type="unit" value="MNR17973"></id></idGroup><countGroup><count type="pageTotal" number="16"></count></countGroup><titleGroup><title type="tocHeading1">Papers</title></titleGroup><copyright>© 2010 The Authors Monthly Notices of the Royal Astronomical Society © 2010 RAS</copyright><eventGroup><event type="xmlConverted" agent="Converter:BPG_TO_WML3G version:2.4.7 mode:FullText" date="2011-03-17"></event><event type="publishedOnlineEarlyUnpaginated" date="2010-12-30"></event><event type="firstOnline" date="2010-12-30"></event><event type="publishedOnlineFinalForm" date="2011-03-17"></event><event type="xmlConverted" agent="Converter:WILEY_ML3G_TO_WILEY_ML3GV2 version:3.8.8" date="2014-02-03"></event><event type="xmlConverted" agent="Converter:WML3G_To_WML3G version:4.1.7 mode:FullText,remove_FC" date="2014-10-31"></event></eventGroup><numberingGroup><numbering type="pageFirst" number="1187">1187</numbering><numbering type="pageLast" number="1202">1202</numbering></numberingGroup><correspondenceTo>
E‐mail: <email>fbraglia@phas.ubc.ca</email></correspondenceTo><linkGroup><link type="toTypesetVersion" href="file:MNR.MNR17973.pdf"></link></linkGroup></publicationMeta><contentMeta><unparsedEditorialHistory>Accepted 2010 November 3. Received 2010 November 2; in original form 2010 March 9</unparsedEditorialHistory><countGroup><count type="figureTotal" number="14"></count><count type="tableTotal" number="4"></count><count type="formulaTotal" number="160"></count><count type="referenceTotal" number="73"></count><count type="linksCrossRef" number="196"></count></countGroup><titleGroup><title type="main">Submillimetre observations of galaxy clusters with the BLAST: the star formation activity in Abell 3112</title><title type="shortAuthors"><i>F. G. Braglia et al.</i></title><title type="short"><i>BLAST observations of Abell 3112</i></title></titleGroup><creators><creator creatorRole="author" xml:id="cr1" affiliationRef="#a1" corresponding="yes"><personName><givenNames>Filiberto G.</givenNames><familyName>Braglia</familyName></personName></creator><creator creatorRole="author" xml:id="cr2" affiliationRef="#a2"><personName><givenNames>Peter A. R.</givenNames><familyName>Ade</familyName></personName></creator><creator creatorRole="author" xml:id="cr3" affiliationRef="#a3"><personName><givenNames>James J.</givenNames><familyName>Bock</familyName></personName></creator><creator creatorRole="author" xml:id="cr4" affiliationRef="#a1"><personName><givenNames>Edward L.</givenNames><familyName>Chapin</familyName></personName></creator><creator creatorRole="author" xml:id="cr5" affiliationRef="#a4"><personName><givenNames>Mark J.</givenNames><familyName>Devlin</familyName></personName></creator><creator creatorRole="author" xml:id="cr6" affiliationRef="#a5"><personName><givenNames>Alastair</givenNames><familyName>Edge</familyName></personName></creator><creator creatorRole="author" xml:id="cr7" affiliationRef="#a2"><personName><givenNames>Matthew</givenNames><familyName>Griffin</familyName></personName></creator><creator creatorRole="author" xml:id="cr8" affiliationRef="#a6"><personName><givenNames>Joshua O.</givenNames><familyName>Gundersen</familyName></personName></creator><creator creatorRole="author" xml:id="cr9" affiliationRef="#a1"><personName><givenNames>Mark</givenNames><familyName>Halpern</familyName></personName></creator><creator creatorRole="author" xml:id="cr10" affiliationRef="#a2"><personName><givenNames>Peter C.</givenNames><familyName>Hargrave</familyName></personName></creator><creator creatorRole="author" xml:id="cr11" affiliationRef="#a7"><personName><givenNames>David H.</givenNames><familyName>Hughes</familyName></personName></creator><creator creatorRole="author" xml:id="cr12" affiliationRef="#a4"><personName><givenNames>Jeff</givenNames><familyName>Klein</familyName></personName></creator><creator creatorRole="author" xml:id="cr13" affiliationRef="#a1"><personName><givenNames>Gaelen</givenNames><familyName>Marsden</familyName></personName></creator><creator creatorRole="author" xml:id="cr14" affiliationRef="#a2"><personName><givenNames>Philip</givenNames><familyName>Mauskopf</familyName></personName></creator><creator creatorRole="author" xml:id="cr15" affiliationRef="#a2"><personName><givenNames>Lorenzo</givenNames><familyName>Moncelsi</familyName></personName></creator><creator creatorRole="author" xml:id="cr16" affiliationRef="#a8 #a9"><personName><givenNames>Calvin B.</givenNames><familyName>Netterfield</familyName></personName></creator><creator creatorRole="author" xml:id="cr17" affiliationRef="#a1"><personName><givenNames>Henry</givenNames><familyName>Ngo</familyName></personName></creator><creator creatorRole="author" xml:id="cr18" affiliationRef="#a10 #a11"><personName><givenNames>Luca</givenNames><familyName>Olmi</familyName></personName></creator><creator creatorRole="author" xml:id="cr19" affiliationRef="#a2"><personName><givenNames>Enzo</givenNames><familyName>Pascale</familyName></personName></creator><creator creatorRole="author" xml:id="cr20" affiliationRef="#a12"><personName><givenNames>Guillaume</givenNames><familyName>Patanchon</familyName></personName></creator><creator creatorRole="author" xml:id="cr21" affiliationRef="#a13" noteRef="#fn4"><personName><givenNames>Kevin A.</givenNames><familyName>Pimbblet</familyName></personName></creator><creator creatorRole="author" xml:id="cr22" affiliationRef="#a14"><personName><givenNames>Marie</givenNames><familyName>Rex</familyName></personName></creator><creator creatorRole="author" xml:id="cr23" affiliationRef="#a1"><personName><givenNames>Douglas</givenNames><familyName>Scott</familyName></personName></creator><creator creatorRole="author" xml:id="cr24" affiliationRef="#a4"><personName><givenNames>Christopher</givenNames><familyName>Semisch</familyName></personName></creator><creator creatorRole="author" xml:id="cr25" affiliationRef="#a6"><personName><givenNames>Nicholas</givenNames><familyName>Thomas</familyName></personName></creator><creator creatorRole="author" xml:id="cr26" affiliationRef="#a4"><personName><givenNames>Matthew D. P.</givenNames><familyName>Truch</familyName></personName></creator><creator creatorRole="author" xml:id="cr27" affiliationRef="#a2"><personName><givenNames>Carole</givenNames><familyName>Tucker</familyName></personName></creator><creator creatorRole="author" xml:id="cr28" affiliationRef="#a15"><personName><givenNames>Gregory S.</givenNames><familyName>Tucker</familyName></personName></creator><creator creatorRole="author" xml:id="cr29" affiliationRef="#a1"><personName><givenNames>Elisabetta</givenNames><familyName>Valiante</familyName></personName></creator><creator creatorRole="author" xml:id="cr30" affiliationRef="#a16"><personName><givenNames>Marco P.</givenNames><familyName>Viero</familyName></personName></creator><creator creatorRole="author" xml:id="cr31" affiliationRef="#a1"><personName><givenNames>Donald V.</givenNames><familyName>Wiebe</familyName></personName></creator></creators><affiliationGroup><affiliation xml:id="a1" countryCode="CA"><unparsedAffiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</unparsedAffiliation></affiliation><affiliation xml:id="a2"><unparsedAffiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</unparsedAffiliation></affiliation><affiliation xml:id="a3" countryCode="US"><unparsedAffiliation>Jet Propulsion Laboratory, Pasadena, CA 91109‐8099, USA</unparsedAffiliation></affiliation><affiliation xml:id="a4" countryCode="US"><unparsedAffiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</unparsedAffiliation></affiliation><affiliation xml:id="a5"><unparsedAffiliation>Department of Physics, Durham University, South Road, Durham DH1 3LE</unparsedAffiliation></affiliation><affiliation xml:id="a6" countryCode="US"><unparsedAffiliation>Department of Physics, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33146, USA</unparsedAffiliation></affiliation><affiliation xml:id="a7" countryCode="MX"><unparsedAffiliation>Instituto Nacional de Astrofísica Óptica y Electrónica (INAOE), Aptdo. Postal 51 y 72000 Puebla, Mexico</unparsedAffiliation></affiliation><affiliation xml:id="a8" countryCode="CA"><unparsedAffiliation>Department of Astronomy & Astrophysics, University of Toronto, 50 St George Street Toronto, ON M5S 3H4, Canada</unparsedAffiliation></affiliation><affiliation xml:id="a9" countryCode="CA"><unparsedAffiliation>Department of Physics, University of Toronto, 60 St George Street, Toronto, ON M5S 1A7, Canada</unparsedAffiliation></affiliation><affiliation xml:id="a10" countryCode="US"><unparsedAffiliation>Physics Department, University of Puerto Rico, Rio Piedras Campus, Box 23343, UPR station, PR 00931, USA</unparsedAffiliation></affiliation><affiliation xml:id="a11" countryCode="IT"><unparsedAffiliation>INAF ‐ Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I‐50125 Firenze, Italy</unparsedAffiliation></affiliation><affiliation xml:id="a12" countryCode="FR"><unparsedAffiliation>Université Paris Diderot, Laboratoire APC, 10, rue Alice Domon et Léonie Duquet, 75205 Paris, France</unparsedAffiliation></affiliation><affiliation xml:id="a13" countryCode="AU"><unparsedAffiliation>School of Physics, Monash University, Clayton, VIC 3800, Australia</unparsedAffiliation></affiliation><affiliation xml:id="a14" countryCode="US"><unparsedAffiliation>Steward Observatory, University of Arizona, 933 N. Chery Ave, Tucson, AZ 85721, USA</unparsedAffiliation></affiliation><affiliation xml:id="a15" countryCode="US"><unparsedAffiliation>Department of Physics, Brown University, 182 Hope Street, Providence, RI 02912, USA</unparsedAffiliation></affiliation><affiliation xml:id="a16" countryCode="US"><unparsedAffiliation>California Institute of Technology, 1200 E. California Blvd, Pasadena, CA 91125, USA</unparsedAffiliation></affiliation></affiliationGroup><keywordGroup xml:lang="en"><keyword xml:id="k1">galaxies: clusters: general</keyword><keyword xml:id="k2">galaxies: clusters: individual: A3112</keyword><keyword xml:id="k3">galaxies: evolution</keyword><keyword xml:id="k4">galaxies: star formation</keyword><keyword xml:id="k5">infrared: galaxies</keyword><keyword xml:id="k6">submillimetre: galaxies</keyword></keywordGroup><supportingInformation><p><b>Table 1.</b> Combined BLAST catalogue of objects in the field of A3112.</p><supportingInfoItem><mediaResource alt="supporting info item" href="urn-x:wiley:00358711:media:mnr17973:MNR_17973_sm_asciitable1"></mediaResource><caption>Supporting info item</caption></supportingInfoItem><supportingInfoItem><mediaResource alt="supporting info item" href="urn-x:wiley:00358711:media:mnr17973:MNR_17973_sm_latextable1"></mediaResource><caption>Supporting info item</caption></supportingInfoItem><supportingInfoItem><mediaResource alt="supporting info item" href="urn-x:wiley:00358711:media:mnr17973:MNR_17973_sm_pdftable1"></mediaResource><caption>Supporting info item</caption></supportingInfoItem></supportingInformation><abstractGroup><abstract type="main" xml:lang="en"><title type="main">ABSTRACT</title><p>We present observations at 250, 350 and 500 μm of the nearby galaxy cluster Abell 3112 (<i>z</i>= 0.075) carried out with the Balloon‐borne Large Aperture Submillimeter Telescope. Five cluster members are individually detected as bright submillimetre (submm) sources. Their far‐infrared spectral energy distributions and optical colours identify them as normal star‐forming galaxies of high mass, with globally evolved stellar populations. They all have <span type="mathematics">(<i>B</i>−<i>R</i>)</span> colours of 1.38 ± 0.08, transitional between the blue, active population and the red, evolved galaxies that dominate the cluster core. We stack to estimate the mean submm emission from all cluster members, which is determined to be 16.6 ± 2.5, 6.1 ± 1.9 and 1.5 ± 1.3 mJy at 250, 350 and 500 μm, respectively. Stacking analyses of the submm emission of cluster members reveal trends in the mean far‐infrared luminosity with respect to clustercentric radius and <i>K</i><sub>S</sub>‐band magnitude. We find that a large fraction of submm emission comes from the boundary of the inner, virialized region of the cluster, at clustercentric distances around <i>R</i><sub>500</sub>. Stacking also shows that the bulk of the submm emission arises in intermediate‐mass galaxies with <i>K</i><sub>S</sub> magnitude ∼1 mag fainter than the characteristic magnitude <inlineGraphic alt="inline image" location="equation/MNR_17973_mu1.gif" href=""></inlineGraphic>. The results and constraints obtained in this work will provide a useful reference for the forthcoming surveys to be conducted on galaxy clusters by <i>Herschel</i>.</p></abstract></abstractGroup></contentMeta><noteGroup><note xml:id="fn4"><p>Correction added after online publication 2011 February 22: author affiliation amended.</p></note></noteGroup></header></component></istex:document></istex:metadataXml><mods version="3.6"><titleInfo lang="en"><title>Submillimetre observations of galaxy clusters with the BLAST: the star formation activity in Abell 3112</title></titleInfo><titleInfo type="abbreviated" lang="en"><title>BLAST observations of Abell 3112</title></titleInfo><titleInfo type="alternative" contentType="CDATA" lang="en"><title>Submillimetre observations of galaxy clusters with the BLAST: the star formation activity in Abell 3112</title></titleInfo><name type="personal"><namePart type="given">Filiberto G.</namePart><namePart type="family">Braglia</namePart><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</affiliation><affiliation>E-mail: fbraglia@phas.ubc.ca</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Peter A. R.</namePart><namePart type="family">Ade</namePart><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">James J.</namePart><namePart type="family">Bock</namePart><affiliation>Jet Propulsion Laboratory, Pasadena, CA 91109‐8099, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Edward L.</namePart><namePart type="family">Chapin</namePart><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Mark J.</namePart><namePart type="family">Devlin</namePart><affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Alastair</namePart><namePart type="family">Edge</namePart><affiliation>Department of Physics, Durham University, South Road, Durham DH1 3LE</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Matthew</namePart><namePart type="family">Griffin</namePart><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Joshua O.</namePart><namePart type="family">Gundersen</namePart><affiliation>Department of Physics, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33146, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Mark</namePart><namePart type="family">Halpern</namePart><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Peter C.</namePart><namePart type="family">Hargrave</namePart><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">David H.</namePart><namePart type="family">Hughes</namePart><affiliation>Instituto Nacional de Astrofísica Óptica y Electrónica (INAOE), Aptdo. Postal 51 y 72000 Puebla, Mexico</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Jeff</namePart><namePart type="family">Klein</namePart><affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Gaelen</namePart><namePart type="family">Marsden</namePart><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Philip</namePart><namePart type="family">Mauskopf</namePart><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Lorenzo</namePart><namePart type="family">Moncelsi</namePart><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Calvin B.</namePart><namePart type="family">Netterfield</namePart><affiliation>Department of Astronomy & Astrophysics, University of Toronto, 50 St George Street Toronto, ON M5S 3H4, Canada</affiliation><affiliation>Department of Physics, University of Toronto, 60 St George Street, Toronto, ON M5S 1A7, Canada</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Henry</namePart><namePart type="family">Ngo</namePart><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Luca</namePart><namePart type="family">Olmi</namePart><affiliation>Physics Department, University of Puerto Rico, Rio Piedras Campus, Box 23343, UPR station, PR 00931, USA</affiliation><affiliation>INAF ‐ Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I‐50125 Firenze, Italy</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Enzo</namePart><namePart type="family">Pascale</namePart><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Guillaume</namePart><namePart type="family">Patanchon</namePart><affiliation>Université Paris Diderot, Laboratoire APC, 10, rue Alice Domon et Léonie Duquet, 75205 Paris, France</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Kevin A.</namePart><namePart type="family">Pimbblet</namePart><affiliation>School of Physics, Monash University, Clayton, VIC 3800, Australia</affiliation><description>Correction added after online publication 2011 February 22: author affiliation amended.</description><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Marie</namePart><namePart type="family">Rex</namePart><affiliation>Steward Observatory, University of Arizona, 933 N. Chery Ave, Tucson, AZ 85721, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Douglas</namePart><namePart type="family">Scott</namePart><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Christopher</namePart><namePart type="family">Semisch</namePart><affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Nicholas</namePart><namePart type="family">Thomas</namePart><affiliation>Department of Physics, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33146, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Matthew D. P.</namePart><namePart type="family">Truch</namePart><affiliation>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Carole</namePart><namePart type="family">Tucker</namePart><affiliation>School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3AA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Gregory S.</namePart><namePart type="family">Tucker</namePart><affiliation>Department of Physics, Brown University, 182 Hope Street, Providence, RI 02912, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Elisabetta</namePart><namePart type="family">Valiante</namePart><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Marco P.</namePart><namePart type="family">Viero</namePart><affiliation>California Institute of Technology, 1200 E. California Blvd, Pasadena, CA 91125, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">Donald V.</namePart><namePart type="family">Wiebe</namePart><affiliation>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</affiliation><role><roleTerm type="text">author</roleTerm></role></name><typeOfResource>text</typeOfResource><genre type="article" displayLabel="article" authority="ISTEX" authorityURI="https://content-type.data.istex.fr" valueURI="https://content-type.data.istex.fr/ark:/67375/XTP-6N5SZHKN-D">article</genre><originInfo><publisher>Blackwell Publishing Ltd</publisher><place><placeTerm type="text">Oxford, UK</placeTerm></place><dateIssued encoding="w3cdtf">2011-04-01</dateIssued><edition>Accepted 2010 November 3. Received 2010 November 2; in original form 2010 March 9</edition><copyrightDate encoding="w3cdtf">2011</copyrightDate></originInfo><language><languageTerm type="code" authority="rfc3066">en</languageTerm><languageTerm type="code" authority="iso639-2b">eng</languageTerm></language><physicalDescription><extent unit="figures">14</extent><extent unit="tables">4</extent><extent unit="formulas">160</extent><extent unit="references">73</extent><extent unit="linksCrossRef">196</extent></physicalDescription><abstract lang="en">We present observations at 250, 350 and 500 μm of the nearby galaxy cluster Abell 3112 (z= 0.075) carried out with the Balloon‐borne Large Aperture Submillimeter Telescope. Five cluster members are individually detected as bright submillimetre (submm) sources. Their far‐infrared spectral energy distributions and optical colours identify them as normal star‐forming galaxies of high mass, with globally evolved stellar populations. They all have (B−R) colours of 1.38 ± 0.08, transitional between the blue, active population and the red, evolved galaxies that dominate the cluster core. We stack to estimate the mean submm emission from all cluster members, which is determined to be 16.6 ± 2.5, 6.1 ± 1.9 and 1.5 ± 1.3 mJy at 250, 350 and 500 μm, respectively. Stacking analyses of the submm emission of cluster members reveal trends in the mean far‐infrared luminosity with respect to clustercentric radius and KS‐band magnitude. We find that a large fraction of submm emission comes from the boundary of the inner, virialized region of the cluster, at clustercentric distances around R500. Stacking also shows that the bulk of the submm emission arises in intermediate‐mass galaxies with KS magnitude ∼1 mag fainter than the characteristic magnitude . The results and constraints obtained in this work will provide a useful reference for the forthcoming surveys to be conducted on galaxy clusters by Herschel.</abstract><subject lang="en"><genre>keywords</genre><topic>galaxies: clusters: general</topic><topic>galaxies: clusters: individual: A3112</topic><topic>galaxies: evolution</topic><topic>galaxies: star formation</topic><topic>infrared: galaxies</topic><topic>submillimetre: galaxies</topic></subject><relatedItem type="host"><titleInfo><title>Monthly Notices of the Royal Astronomical Society</title></titleInfo><genre type="journal" authority="ISTEX" authorityURI="https://publication-type.data.istex.fr" valueURI="https://publication-type.data.istex.fr/ark:/67375/JMC-0GLKJH51-B">journal</genre><note type="content"> Table 1. Combined BLAST catalogue of objects in the field of A3112.Supporting Info Item: Supporting info item - Supporting info item - Supporting info item - </note><identifier type="ISSN">0035-8711</identifier><identifier type="eISSN">1365-2966</identifier><identifier type="DOI">10.1111/(ISSN)1365-2966</identifier><identifier type="PublisherID">MNR</identifier><part><date>2011</date><detail type="volume"><caption>vol.</caption><number>412</number></detail><detail type="issue"><caption>no.</caption><number>2</number></detail><extent unit="pages"><start>1187</start><end>1202</end><total>16</total></extent></part></relatedItem><identifier type="istex">A6B192742E968B4F255CC383950810AB9DB59FB4</identifier><identifier type="ark">ark:/67375/WNG-GCRTFB37-C</identifier><identifier type="DOI">10.1111/j.1365-2966.2010.17973.x</identifier><identifier type="ArticleID">MNR17973</identifier><accessCondition type="use and reproduction" contentType="copyright">© 2010 The Authors Monthly Notices of the Royal Astronomical Society © 2010 RAS</accessCondition><recordInfo><recordContentSource authority="ISTEX" authorityURI="https://loaded-corpus.data.istex.fr" valueURI="https://loaded-corpus.data.istex.fr/ark:/67375/XBH-L0C46X92-X">wiley</recordContentSource><recordOrigin>Blackwell Publishing Ltd</recordOrigin></recordInfo></mods><json:item><extension>json</extension><original>false</original><mimetype>application/json</mimetype><uri>https://api.istex.fr/document/A6B192742E968B4F255CC383950810AB9DB59FB4/metadata/json</uri></json:item></metadata><serie></serie></istex></record>Pour manipuler ce document sous Unix (Dilib)
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