A POPULATION OF z > 2 FAR-INFRARED HERSCHEL-SPIRE-SELECTED STARBURSTS

We present spectroscopic observations for a sample of 36 Herschel-SPIRE 250-500 [mu]m selected galaxies (HSGs) at 2 > z < 5 from the Herschel Multi-tiered Extragalactic Survey. Redshifts are confirmed as part of a large redshift survey of Herschel-SPIRE-selected sources covering ~0.93 deg supe...

Full description

Saved in:
Bibliographic Details
Published in:The Astrophysical journal 2012-12, Vol.761 (2), p.1-24
Main Authors: CASEY, C. M, BERTA, S, CONSELICE, C. J, COORAY, A, FARRAH, D, HATZIMINAOGLOU, E, IVISON, R. J, LEFLOC'H, E, LUTZ, D, MAGDIS, G, MAGNELLI, B, OLIVER, S. J, BETHERMIN, M, PAGE, M. J, POZZI, F, RIGOPOULOU, D, RIGUCCINI, L, ROSEBOOM, I. G, SANDERS, D. B, SCOTT, Douglas, SEYMOUR, N, VALTCHANOV, I, VIEIRA, J. D, BOCK, J, VIERO, M, WARDLOW, J, BRIDGE, C, BURGARELLA, D, CHAPIN, E, CHAPMAN, S. C, CLEMENTS, D. L, CONLEY, A
Format: Article
Language:English
Subjects:
Astrometry
ASTRONOMY
ASTROPHYSICS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Construction
Earth, ocean, space
EMISSION SPECTROSCOPY
ENERGY SPECTRA
Exact sciences and technology
GALAXIES
GHZ RANGE
Imaging
Infrared
INFRARED RADIATION
INFRARED SPECTRA
LUMINOSITY
MASS
RED SHIFT
RESOLUTION
Spectral energy distribution
Spectroscopy
STAR EVOLUTION
STARS
ULTRAVIOLET SPECTRA
UNIVERSE
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c373t-bd9ad75f1af87aaa5e8ef59645801aba32eaecfa143eff9b57cbce83e0b2d7f73
cites cdi_FETCH-LOGICAL-c373t-bd9ad75f1af87aaa5e8ef59645801aba32eaecfa143eff9b57cbce83e0b2d7f73
container_end_page 24
container_issue 2
container_start_page 1
container_title The Astrophysical journal
container_volume 761
creator CASEY, C. M
BERTA, S
CONSELICE, C. J
COORAY, A
FARRAH, D
HATZIMINAOGLOU, E
IVISON, R. J
LEFLOC'H, E
LUTZ, D
MAGDIS, G
MAGNELLI, B
OLIVER, S. J
BETHERMIN, M
PAGE, M. J
POZZI, F
RIGOPOULOU, D
RIGUCCINI, L
ROSEBOOM, I. G
SANDERS, D. B
SCOTT, Douglas
SEYMOUR, N
VALTCHANOV, I
VIEIRA, J. D
BOCK, J
VIERO, M
WARDLOW, J
BRIDGE, C
BURGARELLA, D
CHAPIN, E
CHAPMAN, S. C
CLEMENTS, D. L
CONLEY, A
description We present spectroscopic observations for a sample of 36 Herschel-SPIRE 250-500 [mu]m selected galaxies (HSGs) at 2 > z < 5 from the Herschel Multi-tiered Extragalactic Survey. Redshifts are confirmed as part of a large redshift survey of Herschel-SPIRE-selected sources covering ~0.93 deg super(2) in six extragalactic legacy fields. Observations were taken with the Keck I Low Resolution Imaging Speedometer and the Keck II DEep Imaging Multi-Object Spectrograph. Precise astrometry, needed for spectroscopic follow-up, is determined by identification of counterparts at 24 [mu]m or 1.4 GHz using a cross-identification likelihood matching method. We present both individual and composite rest-frame ultraviolet spectra and infrared spectral energy distributions. The contribution at z ~ 4 has a lower limit of 3 x 10 super(-3) M sub([middot in circle]) yr super(-1) h3 Mpc super(-3), [gap]20% of the estimated total SFRD. This highlights the importance of extremely infrared-luminous galaxies with high SFRs to the buildup of stellar mass, even at the earliest epochs.
doi_str_mv 10.1088/0004-637X/761/2/139
format article
fullrecord <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_22139971</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1730064402</sourcerecordid><originalsourceid>FETCH-LOGICAL-c373t-bd9ad75f1af87aaa5e8ef59645801aba32eaecfa143eff9b57cbce83e0b2d7f73</originalsourceid><addsrcrecordid>eNqNkctqg0AUhofSQtO0T9CNUArdWOfiOLopWKuNIDGoge6GcTJDLSamjlm0T18lIeuuDufw_ef2A3CP4DOCvu9ACF3bI-zDYR5ysINIcAFmiBLfdglll2B2Jq7BjTFfU4qDYAbi0Frlq3UWVmm-tPLE-rVeLGwlYWGny6QIi_jNWsRFGS3izC5XaRHbZZzFUTXWyyosXtdFWZW34EqL1qi7U5yDdRJX0cLO8vc0CjNbEkYGu94EYsOoRkL7TAhBla80DTyX-hCJWhCshJJaIJcorYOaMllL5RMFa7xhmpE5eDj27czQcCObQclP2e12Sg4c4_HsgKGRejpS-777Pigz8G1jpGpbsVPdwXDECISe60L8DxRhylyPeSNKjqjsO2N6pfm-b7ai_-EI8skFPj2VTz_mowsc83GdUfV4GiCMFK3uxU425izFHqMYU0T-AAHngIY</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1712574676</pqid></control><display><type>article</type><title>A POPULATION OF z &gt; 2 FAR-INFRARED HERSCHEL-SPIRE-SELECTED STARBURSTS</title><source>EZB Electronic Journals Library</source><creator>CASEY, C. M ; BERTA, S ; CONSELICE, C. J ; COORAY, A ; FARRAH, D ; HATZIMINAOGLOU, E ; IVISON, R. J ; LEFLOC'H, E ; LUTZ, D ; MAGDIS, G ; MAGNELLI, B ; OLIVER, S. J ; BETHERMIN, M ; PAGE, M. J ; POZZI, F ; RIGOPOULOU, D ; RIGUCCINI, L ; ROSEBOOM, I. G ; SANDERS, D. B ; SCOTT, Douglas ; SEYMOUR, N ; VALTCHANOV, I ; VIEIRA, J. D ; BOCK, J ; VIERO, M ; WARDLOW, J ; BRIDGE, C ; BURGARELLA, D ; CHAPIN, E ; CHAPMAN, S. C ; CLEMENTS, D. L ; CONLEY, A</creator><creatorcontrib>CASEY, C. M ; BERTA, S ; CONSELICE, C. J ; COORAY, A ; FARRAH, D ; HATZIMINAOGLOU, E ; IVISON, R. J ; LEFLOC'H, E ; LUTZ, D ; MAGDIS, G ; MAGNELLI, B ; OLIVER, S. J ; BETHERMIN, M ; PAGE, M. J ; POZZI, F ; RIGOPOULOU, D ; RIGUCCINI, L ; ROSEBOOM, I. G ; SANDERS, D. B ; SCOTT, Douglas ; SEYMOUR, N ; VALTCHANOV, I ; VIEIRA, J. D ; BOCK, J ; VIERO, M ; WARDLOW, J ; BRIDGE, C ; BURGARELLA, D ; CHAPIN, E ; CHAPMAN, S. C ; CLEMENTS, D. L ; CONLEY, A</creatorcontrib><description>We present spectroscopic observations for a sample of 36 Herschel-SPIRE 250-500 [mu]m selected galaxies (HSGs) at 2 &gt; z &lt; 5 from the Herschel Multi-tiered Extragalactic Survey. Redshifts are confirmed as part of a large redshift survey of Herschel-SPIRE-selected sources covering ~0.93 deg super(2) in six extragalactic legacy fields. Observations were taken with the Keck I Low Resolution Imaging Speedometer and the Keck II DEep Imaging Multi-Object Spectrograph. Precise astrometry, needed for spectroscopic follow-up, is determined by identification of counterparts at 24 [mu]m or 1.4 GHz using a cross-identification likelihood matching method. We present both individual and composite rest-frame ultraviolet spectra and infrared spectral energy distributions. The contribution at z ~ 4 has a lower limit of 3 x 10 super(-3) M sub([middot in circle]) yr super(-1) h3 Mpc super(-3), [gap]20% of the estimated total SFRD. This highlights the importance of extremely infrared-luminous galaxies with high SFRs to the buildup of stellar mass, even at the earliest epochs.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/761/2/139</identifier><identifier>CODEN: ASJOAB</identifier><language>eng</language><publisher>Bristol: IOP</publisher><subject>Astrometry ; ASTRONOMY ; ASTROPHYSICS ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; Construction ; Earth, ocean, space ; EMISSION SPECTROSCOPY ; ENERGY SPECTRA ; Exact sciences and technology ; GALAXIES ; GHZ RANGE ; Imaging ; Infrared ; INFRARED RADIATION ; INFRARED SPECTRA ; LUMINOSITY ; MASS ; RED SHIFT ; RESOLUTION ; Spectral energy distribution ; Spectroscopy ; STAR EVOLUTION ; STARS ; ULTRAVIOLET SPECTRA ; UNIVERSE</subject><ispartof>The Astrophysical journal, 2012-12, Vol.761 (2), p.1-24</ispartof><rights>2014 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c373t-bd9ad75f1af87aaa5e8ef59645801aba32eaecfa143eff9b57cbce83e0b2d7f73</citedby><cites>FETCH-LOGICAL-c373t-bd9ad75f1af87aaa5e8ef59645801aba32eaecfa143eff9b57cbce83e0b2d7f73</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27924,27925</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=26752251$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/22139971$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>CASEY, C. M</creatorcontrib><creatorcontrib>BERTA, S</creatorcontrib><creatorcontrib>CONSELICE, C. J</creatorcontrib><creatorcontrib>COORAY, A</creatorcontrib><creatorcontrib>FARRAH, D</creatorcontrib><creatorcontrib>HATZIMINAOGLOU, E</creatorcontrib><creatorcontrib>IVISON, R. J</creatorcontrib><creatorcontrib>LEFLOC'H, E</creatorcontrib><creatorcontrib>LUTZ, D</creatorcontrib><creatorcontrib>MAGDIS, G</creatorcontrib><creatorcontrib>MAGNELLI, B</creatorcontrib><creatorcontrib>OLIVER, S. J</creatorcontrib><creatorcontrib>BETHERMIN, M</creatorcontrib><creatorcontrib>PAGE, M. J</creatorcontrib><creatorcontrib>POZZI, F</creatorcontrib><creatorcontrib>RIGOPOULOU, D</creatorcontrib><creatorcontrib>RIGUCCINI, L</creatorcontrib><creatorcontrib>ROSEBOOM, I. G</creatorcontrib><creatorcontrib>SANDERS, D. B</creatorcontrib><creatorcontrib>SCOTT, Douglas</creatorcontrib><creatorcontrib>SEYMOUR, N</creatorcontrib><creatorcontrib>VALTCHANOV, I</creatorcontrib><creatorcontrib>VIEIRA, J. D</creatorcontrib><creatorcontrib>BOCK, J</creatorcontrib><creatorcontrib>VIERO, M</creatorcontrib><creatorcontrib>WARDLOW, J</creatorcontrib><creatorcontrib>BRIDGE, C</creatorcontrib><creatorcontrib>BURGARELLA, D</creatorcontrib><creatorcontrib>CHAPIN, E</creatorcontrib><creatorcontrib>CHAPMAN, S. C</creatorcontrib><creatorcontrib>CLEMENTS, D. L</creatorcontrib><creatorcontrib>CONLEY, A</creatorcontrib><title>A POPULATION OF z &gt; 2 FAR-INFRARED HERSCHEL-SPIRE-SELECTED STARBURSTS</title><title>The Astrophysical journal</title><description>We present spectroscopic observations for a sample of 36 Herschel-SPIRE 250-500 [mu]m selected galaxies (HSGs) at 2 &gt; z &lt; 5 from the Herschel Multi-tiered Extragalactic Survey. Redshifts are confirmed as part of a large redshift survey of Herschel-SPIRE-selected sources covering ~0.93 deg super(2) in six extragalactic legacy fields. Observations were taken with the Keck I Low Resolution Imaging Speedometer and the Keck II DEep Imaging Multi-Object Spectrograph. Precise astrometry, needed for spectroscopic follow-up, is determined by identification of counterparts at 24 [mu]m or 1.4 GHz using a cross-identification likelihood matching method. We present both individual and composite rest-frame ultraviolet spectra and infrared spectral energy distributions. The contribution at z ~ 4 has a lower limit of 3 x 10 super(-3) M sub([middot in circle]) yr super(-1) h3 Mpc super(-3), [gap]20% of the estimated total SFRD. This highlights the importance of extremely infrared-luminous galaxies with high SFRs to the buildup of stellar mass, even at the earliest epochs.</description><subject>Astrometry</subject><subject>ASTRONOMY</subject><subject>ASTROPHYSICS</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>Construction</subject><subject>Earth, ocean, space</subject><subject>EMISSION SPECTROSCOPY</subject><subject>ENERGY SPECTRA</subject><subject>Exact sciences and technology</subject><subject>GALAXIES</subject><subject>GHZ RANGE</subject><subject>Imaging</subject><subject>Infrared</subject><subject>INFRARED RADIATION</subject><subject>INFRARED SPECTRA</subject><subject>LUMINOSITY</subject><subject>MASS</subject><subject>RED SHIFT</subject><subject>RESOLUTION</subject><subject>Spectral energy distribution</subject><subject>Spectroscopy</subject><subject>STAR EVOLUTION</subject><subject>STARS</subject><subject>ULTRAVIOLET SPECTRA</subject><subject>UNIVERSE</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><recordid>eNqNkctqg0AUhofSQtO0T9CNUArdWOfiOLopWKuNIDGoge6GcTJDLSamjlm0T18lIeuuDufw_ef2A3CP4DOCvu9ACF3bI-zDYR5ysINIcAFmiBLfdglll2B2Jq7BjTFfU4qDYAbi0Frlq3UWVmm-tPLE-rVeLGwlYWGny6QIi_jNWsRFGS3izC5XaRHbZZzFUTXWyyosXtdFWZW34EqL1qi7U5yDdRJX0cLO8vc0CjNbEkYGu94EYsOoRkL7TAhBla80DTyX-hCJWhCshJJaIJcorYOaMllL5RMFa7xhmpE5eDj27czQcCObQclP2e12Sg4c4_HsgKGRejpS-777Pigz8G1jpGpbsVPdwXDECISe60L8DxRhylyPeSNKjqjsO2N6pfm-b7ai_-EI8skFPj2VTz_mowsc83GdUfV4GiCMFK3uxU425izFHqMYU0T-AAHngIY</recordid><startdate>20121220</startdate><enddate>20121220</enddate><creator>CASEY, C. M</creator><creator>BERTA, S</creator><creator>CONSELICE, C. J</creator><creator>COORAY, A</creator><creator>FARRAH, D</creator><creator>HATZIMINAOGLOU, E</creator><creator>IVISON, R. J</creator><creator>LEFLOC'H, E</creator><creator>LUTZ, D</creator><creator>MAGDIS, G</creator><creator>MAGNELLI, B</creator><creator>OLIVER, S. J</creator><creator>BETHERMIN, M</creator><creator>PAGE, M. J</creator><creator>POZZI, F</creator><creator>RIGOPOULOU, D</creator><creator>RIGUCCINI, L</creator><creator>ROSEBOOM, I. G</creator><creator>SANDERS, D. B</creator><creator>SCOTT, Douglas</creator><creator>SEYMOUR, N</creator><creator>VALTCHANOV, I</creator><creator>VIEIRA, J. D</creator><creator>BOCK, J</creator><creator>VIERO, M</creator><creator>WARDLOW, J</creator><creator>BRIDGE, C</creator><creator>BURGARELLA, D</creator><creator>CHAPIN, E</creator><creator>CHAPMAN, S. C</creator><creator>CLEMENTS, D. L</creator><creator>CONLEY, A</creator><general>IOP</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20121220</creationdate><title>A POPULATION OF z &gt; 2 FAR-INFRARED HERSCHEL-SPIRE-SELECTED STARBURSTS</title><author>CASEY, C. M ; BERTA, S ; CONSELICE, C. J ; COORAY, A ; FARRAH, D ; HATZIMINAOGLOU, E ; IVISON, R. J ; LEFLOC'H, E ; LUTZ, D ; MAGDIS, G ; MAGNELLI, B ; OLIVER, S. J ; BETHERMIN, M ; PAGE, M. J ; POZZI, F ; RIGOPOULOU, D ; RIGUCCINI, L ; ROSEBOOM, I. G ; SANDERS, D. B ; SCOTT, Douglas ; SEYMOUR, N ; VALTCHANOV, I ; VIEIRA, J. D ; BOCK, J ; VIERO, M ; WARDLOW, J ; BRIDGE, C ; BURGARELLA, D ; CHAPIN, E ; CHAPMAN, S. C ; CLEMENTS, D. L ; CONLEY, A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c373t-bd9ad75f1af87aaa5e8ef59645801aba32eaecfa143eff9b57cbce83e0b2d7f73</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Astrometry</topic><topic>ASTRONOMY</topic><topic>ASTROPHYSICS</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>Construction</topic><topic>Earth, ocean, space</topic><topic>EMISSION SPECTROSCOPY</topic><topic>ENERGY SPECTRA</topic><topic>Exact sciences and technology</topic><topic>GALAXIES</topic><topic>GHZ RANGE</topic><topic>Imaging</topic><topic>Infrared</topic><topic>INFRARED RADIATION</topic><topic>INFRARED SPECTRA</topic><topic>LUMINOSITY</topic><topic>MASS</topic><topic>RED SHIFT</topic><topic>RESOLUTION</topic><topic>Spectral energy distribution</topic><topic>Spectroscopy</topic><topic>STAR EVOLUTION</topic><topic>STARS</topic><topic>ULTRAVIOLET SPECTRA</topic><topic>UNIVERSE</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>CASEY, C. M</creatorcontrib><creatorcontrib>BERTA, S</creatorcontrib><creatorcontrib>CONSELICE, C. J</creatorcontrib><creatorcontrib>COORAY, A</creatorcontrib><creatorcontrib>FARRAH, D</creatorcontrib><creatorcontrib>HATZIMINAOGLOU, E</creatorcontrib><creatorcontrib>IVISON, R. J</creatorcontrib><creatorcontrib>LEFLOC'H, E</creatorcontrib><creatorcontrib>LUTZ, D</creatorcontrib><creatorcontrib>MAGDIS, G</creatorcontrib><creatorcontrib>MAGNELLI, B</creatorcontrib><creatorcontrib>OLIVER, S. J</creatorcontrib><creatorcontrib>BETHERMIN, M</creatorcontrib><creatorcontrib>PAGE, M. J</creatorcontrib><creatorcontrib>POZZI, F</creatorcontrib><creatorcontrib>RIGOPOULOU, D</creatorcontrib><creatorcontrib>RIGUCCINI, L</creatorcontrib><creatorcontrib>ROSEBOOM, I. G</creatorcontrib><creatorcontrib>SANDERS, D. B</creatorcontrib><creatorcontrib>SCOTT, Douglas</creatorcontrib><creatorcontrib>SEYMOUR, N</creatorcontrib><creatorcontrib>VALTCHANOV, I</creatorcontrib><creatorcontrib>VIEIRA, J. D</creatorcontrib><creatorcontrib>BOCK, J</creatorcontrib><creatorcontrib>VIERO, M</creatorcontrib><creatorcontrib>WARDLOW, J</creatorcontrib><creatorcontrib>BRIDGE, C</creatorcontrib><creatorcontrib>BURGARELLA, D</creatorcontrib><creatorcontrib>CHAPIN, E</creatorcontrib><creatorcontrib>CHAPMAN, S. C</creatorcontrib><creatorcontrib>CLEMENTS, D. L</creatorcontrib><creatorcontrib>CONLEY, A</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>CASEY, C. M</au><au>BERTA, S</au><au>CONSELICE, C. J</au><au>COORAY, A</au><au>FARRAH, D</au><au>HATZIMINAOGLOU, E</au><au>IVISON, R. J</au><au>LEFLOC'H, E</au><au>LUTZ, D</au><au>MAGDIS, G</au><au>MAGNELLI, B</au><au>OLIVER, S. J</au><au>BETHERMIN, M</au><au>PAGE, M. J</au><au>POZZI, F</au><au>RIGOPOULOU, D</au><au>RIGUCCINI, L</au><au>ROSEBOOM, I. G</au><au>SANDERS, D. B</au><au>SCOTT, Douglas</au><au>SEYMOUR, N</au><au>VALTCHANOV, I</au><au>VIEIRA, J. D</au><au>BOCK, J</au><au>VIERO, M</au><au>WARDLOW, J</au><au>BRIDGE, C</au><au>BURGARELLA, D</au><au>CHAPIN, E</au><au>CHAPMAN, S. C</au><au>CLEMENTS, D. L</au><au>CONLEY, A</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A POPULATION OF z &gt; 2 FAR-INFRARED HERSCHEL-SPIRE-SELECTED STARBURSTS</atitle><jtitle>The Astrophysical journal</jtitle><date>2012-12-20</date><risdate>2012</risdate><volume>761</volume><issue>2</issue><spage>1</spage><epage>24</epage><pages>1-24</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><coden>ASJOAB</coden><abstract>We present spectroscopic observations for a sample of 36 Herschel-SPIRE 250-500 [mu]m selected galaxies (HSGs) at 2 &gt; z &lt; 5 from the Herschel Multi-tiered Extragalactic Survey. Redshifts are confirmed as part of a large redshift survey of Herschel-SPIRE-selected sources covering ~0.93 deg super(2) in six extragalactic legacy fields. Observations were taken with the Keck I Low Resolution Imaging Speedometer and the Keck II DEep Imaging Multi-Object Spectrograph. Precise astrometry, needed for spectroscopic follow-up, is determined by identification of counterparts at 24 [mu]m or 1.4 GHz using a cross-identification likelihood matching method. We present both individual and composite rest-frame ultraviolet spectra and infrared spectral energy distributions. The contribution at z ~ 4 has a lower limit of 3 x 10 super(-3) M sub([middot in circle]) yr super(-1) h3 Mpc super(-3), [gap]20% of the estimated total SFRD. This highlights the importance of extremely infrared-luminous galaxies with high SFRs to the buildup of stellar mass, even at the earliest epochs.</abstract><cop>Bristol</cop><pub>IOP</pub><doi>10.1088/0004-637X/761/2/139</doi><tpages>24</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0004-637X
ispartof The Astrophysical journal, 2012-12, Vol.761 (2), p.1-24
issn 0004-637X
1538-4357
language eng
recordid cdi_osti_scitechconnect_22139971
source EZB Electronic Journals Library
subjects Astrometry
ASTRONOMY
ASTROPHYSICS
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Construction
Earth, ocean, space
EMISSION SPECTROSCOPY
ENERGY SPECTRA
Exact sciences and technology
GALAXIES
GHZ RANGE
Imaging
Infrared
INFRARED RADIATION
INFRARED SPECTRA
LUMINOSITY
MASS
RED SHIFT
RESOLUTION
Spectral energy distribution
Spectroscopy
STAR EVOLUTION
STARS
ULTRAVIOLET SPECTRA
UNIVERSE
title A POPULATION OF z > 2 FAR-INFRARED HERSCHEL-SPIRE-SELECTED STARBURSTS
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-02T01%3A40%3A46IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=A%20POPULATION%20OF%20z%20%3E%202%20FAR-INFRARED%20HERSCHEL-SPIRE-SELECTED%20STARBURSTS&rft.jtitle=The%20Astrophysical%20journal&rft.au=CASEY,%20C.%20M&rft.date=2012-12-20&rft.volume=761&rft.issue=2&rft.spage=1&rft.epage=24&rft.pages=1-24&rft.issn=0004-637X&rft.eissn=1538-4357&rft.coden=ASJOAB&rft_id=info:doi/10.1088/0004-637X/761/2/139&rft_dat=%3Cproquest_osti_%3E1730064402%3C/proquest_osti_%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c373t-bd9ad75f1af87aaa5e8ef59645801aba32eaecfa143eff9b57cbce83e0b2d7f73%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1712574676&rft_id=info:pmid/&rfr_iscdi=true