Submillimetre observations of galaxy clusters with the BLAST: the star formation activity in Abell 3112
Identifieur interne : 006323 ( Main/Exploration ); précédent : 006322; suivant : 006324Submillimetre observations of galaxy clusters with the BLAST: the star formation activity in Abell 3112
Auteurs : Filiberto G. Braglia [Canada] ; Peter A. R. Ade ; James J. Bock [États-Unis] ; Edward L. Chapin [Canada] ; Mark J. Devlin [États-Unis] ; Alastair Edge ; Matthew Griffin ; Joshua O. Gundersen [États-Unis] ; Mark Halpern [Canada] ; Peter C. Hargrave ; David H. Hughes [Mexique] ; Jeff Klein [États-Unis] ; Gaelen Marsden [Canada] ; Philip Mauskopf ; Lorenzo Moncelsi ; Calvin B. Netterfield [Canada] ; Henry Ngo [Canada] ; Luca Olmi [États-Unis, Italie] ; Enzo Pascale ; Guillaume Patanchon [France] ; Kevin A. Pimbblet [Australie] ; Marie Rex [États-Unis] ; Douglas Scott [Canada] ; Christopher Semisch [États-Unis] ; Nicholas Thomas [États-Unis] ; Matthew D. P. Truch [États-Unis] ; Carole Tucker ; Gregory S. Tucker [États-Unis] ; Elisabetta Valiante [Canada] ; Marco P. Viero [États-Unis] ; Donald V. Wiebe [Canada]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2011-04-01.
Descripteurs français
- Pascal (Inist)
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, Color, Colour, Colours, Devlin, Distance scale, Dust content, Dust masses, Emission lines, Environmental effects, Flux densities, Galaxy, Galaxy clusters, Galaxy evolution, Galaxy formation, Galaxy geometry, Global decrease, Good agreement, Haines, Inclination angle, Individual sources, Infall region, Infrared galaxies, 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, Radio observation, Random occurrence, Redshift, Rejection probability, Robust, Same area, Same method, Seds, Sfrs, Solid line, Source catalogue, Source extraction, Spectral energy distribution, Spectral region, Spectroscopic, Spectroscopic catalogue, Ssfr, Star formation, Star formation activity, Stellar, Stellar activity, Stellar mass, Stellar masses, Stellar population, Submillimeter wave radiation, 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
Affiliations:
- Australie, Canada, France, Italie, Mexique, États-Unis
- Arizona, Californie, Floride, Ontario, Pennsylvanie, Rhode Island, Île-de-France
- Paris, Providence (Rhode Island), Toronto
- Université Brown, Université de Toronto
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Le document en format XML
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Pimbblet</name><affiliation wicri:level="1"><country xml:lang="fr">Australie</country><wicri:regionArea>School of Physics, Monash University, Clayton, VIC 3800</wicri:regionArea><wicri:noRegion>VIC 3800</wicri:noRegion></affiliation></author><author><name sortKey="Rex, Marie" sort="Rex, Marie" uniqKey="Rex M" first="Marie" last="Rex">Marie Rex</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Steward Observatory, University of Arizona, 933 N. Chery Ave, Tucson, AZ 85721</wicri:regionArea><placeName><region type="state">Arizona</region></placeName></affiliation></author><author><name sortKey="Scott, Douglas" sort="Scott, Douglas" uniqKey="Scott D" first="Douglas" last="Scott">Douglas Scott</name><affiliation wicri:level="1"><country xml:lang="fr">Canada</country><wicri:regionArea>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1</wicri:regionArea><wicri:noRegion>BC V6T 1Z1</wicri:noRegion></affiliation></author><author><name sortKey="Semisch, Christopher" sort="Semisch, Christopher" uniqKey="Semisch C" first="Christopher" last="Semisch">Christopher Semisch</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104</wicri:regionArea><placeName><region type="state">Pennsylvanie</region></placeName></affiliation></author><author><name sortKey="Thomas, Nicholas" sort="Thomas, Nicholas" uniqKey="Thomas N" first="Nicholas" last="Thomas">Nicholas Thomas</name><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Physics, University of Miami, 1320 Campo Sano Drive, Coral Gables, FL 33146</wicri:regionArea><placeName><region type="state">Floride</region></placeName></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 wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Physics & Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104</wicri:regionArea><placeName><region type="state">Pennsylvanie</region></placeName></affiliation></author><author><name sortKey="Tucker, Carole" sort="Tucker, Carole" uniqKey="Tucker C" first="Carole" last="Tucker">Carole Tucker</name><affiliation><wicri:noCountry code="subField">3AA</wicri:noCountry></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 wicri:level="4"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Physics, Brown University, 182 Hope Street, Providence, RI 02912</wicri:regionArea><placeName><region type="state">Rhode Island</region><settlement type="city">Providence (Rhode Island)</settlement></placeName><orgName type="university">Université Brown</orgName></affiliation></author><author><name sortKey="Valiante, Elisabetta" sort="Valiante, Elisabetta" uniqKey="Valiante E" first="Elisabetta" last="Valiante">Elisabetta Valiante</name><affiliation wicri:level="1"><country xml:lang="fr">Canada</country><wicri:regionArea>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1</wicri:regionArea><wicri:noRegion>BC V6T 1Z1</wicri:noRegion></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 wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>California Institute of Technology, 1200 E. California Blvd, Pasadena, CA 91125</wicri:regionArea><placeName><region type="state">Californie</region></placeName></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 wicri:level="1"><country xml:lang="fr">Canada</country><wicri:regionArea>Department of Physics & Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1</wicri:regionArea><wicri:noRegion>BC V6T 1Z1</wicri:noRegion></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>Color</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 evolution</term><term>Galaxy formation</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>Infrared galaxies</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>Radio observation</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 energy distribution</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 activity</term><term>Stellar mass</term><term>Stellar masses</term><term>Stellar population</term><term>Submillimeter wave radiation</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="Pascal" xml:lang="fr"><term>Activité stellaire</term><term>Amas galaxies</term><term>Couleur</term><term>Densité spectrale énergie</term><term>Evolution galaxies</term><term>Formation galaxies</term><term>Formation stellaire</term><term>Galaxies infrarouges</term><term>Luminosité</term><term>Observation radio</term><term>Onde submillimétrique</term><term>Population stellaire</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><affiliations><list><country><li>Australie</li><li>Canada</li><li>France</li><li>Italie</li><li>Mexique</li><li>États-Unis</li></country><region><li>Arizona</li><li>Californie</li><li>Floride</li><li>Ontario</li><li>Pennsylvanie</li><li>Rhode Island</li><li>Île-de-France</li></region><settlement><li>Paris</li><li>Providence (Rhode Island)</li><li>Toronto</li></settlement><orgName><li>Université Brown</li><li>Université de Toronto</li></orgName></list><tree><noCountry><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><name sortKey="Edge, Alastair" sort="Edge, Alastair" uniqKey="Edge A" first="Alastair" last="Edge">Alastair Edge</name><name sortKey="Griffin, Matthew" sort="Griffin, Matthew" uniqKey="Griffin M" first="Matthew" last="Griffin">Matthew Griffin</name><name sortKey="Hargrave, Peter C" sort="Hargrave, Peter C" uniqKey="Hargrave P" first="Peter C." last="Hargrave">Peter C. Hargrave</name><name sortKey="Mauskopf, Philip" sort="Mauskopf, Philip" uniqKey="Mauskopf P" first="Philip" last="Mauskopf">Philip Mauskopf</name><name sortKey="Moncelsi, Lorenzo" sort="Moncelsi, Lorenzo" uniqKey="Moncelsi L" first="Lorenzo" last="Moncelsi">Lorenzo Moncelsi</name><name sortKey="Pascale, Enzo" sort="Pascale, Enzo" uniqKey="Pascale E" first="Enzo" last="Pascale">Enzo Pascale</name><name sortKey="Tucker, Carole" sort="Tucker, Carole" uniqKey="Tucker C" first="Carole" last="Tucker">Carole Tucker</name></noCountry><country name="Canada"><noRegion><name sortKey="Braglia, Filiberto G" sort="Braglia, Filiberto G" uniqKey="Braglia F" first="Filiberto G." last="Braglia">Filiberto G. Braglia</name></noRegion><name sortKey="Braglia, Filiberto G" sort="Braglia, Filiberto G" uniqKey="Braglia F" first="Filiberto G." last="Braglia">Filiberto G. Braglia</name><name sortKey="Chapin, Edward L" sort="Chapin, Edward L" uniqKey="Chapin E" first="Edward L." last="Chapin">Edward L. Chapin</name><name sortKey="Halpern, Mark" sort="Halpern, Mark" uniqKey="Halpern M" first="Mark" last="Halpern">Mark Halpern</name><name sortKey="Marsden, Gaelen" sort="Marsden, Gaelen" uniqKey="Marsden G" first="Gaelen" last="Marsden">Gaelen Marsden</name><name sortKey="Netterfield, Calvin B" sort="Netterfield, Calvin B" uniqKey="Netterfield C" first="Calvin B." last="Netterfield">Calvin B. Netterfield</name><name sortKey="Netterfield, Calvin B" sort="Netterfield, Calvin B" uniqKey="Netterfield C" first="Calvin B." last="Netterfield">Calvin B. Netterfield</name><name sortKey="Ngo, Henry" sort="Ngo, Henry" uniqKey="Ngo H" first="Henry" last="Ngo">Henry Ngo</name><name sortKey="Scott, Douglas" sort="Scott, Douglas" uniqKey="Scott D" first="Douglas" last="Scott">Douglas Scott</name><name sortKey="Valiante, Elisabetta" sort="Valiante, Elisabetta" uniqKey="Valiante E" first="Elisabetta" last="Valiante">Elisabetta Valiante</name><name sortKey="Wiebe, Donald V" sort="Wiebe, Donald V" uniqKey="Wiebe D" first="Donald V." last="Wiebe">Donald V. Wiebe</name></country><country name="États-Unis"><region name="Californie"><name sortKey="Bock, James J" sort="Bock, James J" uniqKey="Bock J" first="James J." last="Bock">James J. Bock</name></region><name sortKey="Devlin, Mark J" sort="Devlin, Mark J" uniqKey="Devlin M" first="Mark J." last="Devlin">Mark J. Devlin</name><name sortKey="Gundersen, Joshua O" sort="Gundersen, Joshua O" uniqKey="Gundersen J" first="Joshua O." last="Gundersen">Joshua O. Gundersen</name><name sortKey="Klein, Jeff" sort="Klein, Jeff" uniqKey="Klein J" first="Jeff" last="Klein">Jeff Klein</name><name sortKey="Olmi, Luca" sort="Olmi, Luca" uniqKey="Olmi L" first="Luca" last="Olmi">Luca Olmi</name><name sortKey="Rex, Marie" sort="Rex, Marie" uniqKey="Rex M" first="Marie" last="Rex">Marie Rex</name><name sortKey="Semisch, Christopher" sort="Semisch, Christopher" uniqKey="Semisch C" first="Christopher" last="Semisch">Christopher Semisch</name><name sortKey="Thomas, Nicholas" sort="Thomas, Nicholas" uniqKey="Thomas N" first="Nicholas" last="Thomas">Nicholas Thomas</name><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><name sortKey="Tucker, Gregory S" sort="Tucker, Gregory S" uniqKey="Tucker G" first="Gregory S." last="Tucker">Gregory S. Tucker</name><name sortKey="Viero, Marco P" sort="Viero, Marco P" uniqKey="Viero M" first="Marco P." last="Viero">Marco P. Viero</name></country><country name="Mexique"><noRegion><name sortKey="Hughes, David H" sort="Hughes, David H" uniqKey="Hughes D" first="David H." last="Hughes">David H. Hughes</name></noRegion></country><country name="Italie"><noRegion><name sortKey="Olmi, Luca" sort="Olmi, Luca" uniqKey="Olmi L" first="Luca" last="Olmi">Luca Olmi</name></noRegion></country><country name="France"><region name="Île-de-France"><name sortKey="Patanchon, Guillaume" sort="Patanchon, Guillaume" uniqKey="Patanchon G" first="Guillaume" last="Patanchon">Guillaume Patanchon</name></region></country><country name="Australie"><noRegion><name sortKey="Pimbblet, Kevin A" sort="Pimbblet, Kevin A" uniqKey="Pimbblet K" first="Kevin A." last="Pimbblet">Kevin A. Pimbblet</name></noRegion></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
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