High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey

In the local Universe, most galaxies are dominated by stars, with less than ten per cent of their visible mass in the form of gas. Determining when most of these stars formed is one of the central issues of observational cosmology. Optical and ultraviolet observations of high-redshift galaxies (part...

Full description

Saved in:
Bibliographic Details
Published in:Nature (London) 1998-07, Vol.394 (6690), p.241-247
Main Authors: Hughes, David H., Serjeant, Stephen, Dunlop, James, Rowan-Robinson, Michael, Blain, Andrew, Mann, Robert G., Ivison, Rob, Peacock, John, Efstathiou, Andreas, Gear, Walter, Oliver, Seb, Lawrence, Andy, Longair, Malcolm, Goldschmidt, Pippa, Jenness, Tim
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics
Characteristics and properties of external galaxies and extragalactic objects
Earth, ocean, space
Exact sciences and technology
Humanities and Social Sciences
multidisciplinary
Origin, formation, evolution, age, and star formation
Science
Science (multidisciplinary)
Space telescopes
Stars
Stars & galaxies
Stellar systems. Galactic and extragalactic objects and systems. The 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-c403t-ed9017db10b8f81f500dbd901289cd5298766abecac144e3f9ba281c21b86e583
cites cdi_FETCH-LOGICAL-c403t-ed9017db10b8f81f500dbd901289cd5298766abecac144e3f9ba281c21b86e583
container_end_page 247
container_issue 6690
container_start_page 241
container_title Nature (London)
container_volume 394
creator Hughes, David H.
Serjeant, Stephen
Dunlop, James
Rowan-Robinson, Michael
Blain, Andrew
Mann, Robert G.
Ivison, Rob
Peacock, John
Efstathiou, Andreas
Gear, Walter
Oliver, Seb
Lawrence, Andy
Longair, Malcolm
Goldschmidt, Pippa
Jenness, Tim
description In the local Universe, most galaxies are dominated by stars, with less than ten per cent of their visible mass in the form of gas. Determining when most of these stars formed is one of the central issues of observational cosmology. Optical and ultraviolet observations of high-redshift galaxies (particularly those in the Hubble Deep Field) have been interpreted as indicating that the peak of star formation occurred between redshifts of 1 and 1.5. But it is known that star formation takes place in dense clouds, and is often hidden at optical wavelengths because of extinction by dust in the clouds. Here we report a deep submillimetre-wavelength survey of the Hubble Deep Field; these wavelengths trace directly the emission from dust that has been warmed by massive star-formation activity. The combined radiation of the five most significant detections accounts for 30–50 per cent of the previously unresolved background emission in this area. Four of these sources appear to be galaxies in the redshift range 2< z < 4, which, assuming these objects have properties comparable to local dust-enshrouded starburst galaxies, implies a star-formation rate during that period about a factor of five higher than that inferred from the optical and ultraviolet observations.
doi_str_mv 10.1038/28328
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_27537087</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>27537087</sourcerecordid><originalsourceid>FETCH-LOGICAL-c403t-ed9017db10b8f81f500dbd901289cd5298766abecac144e3f9ba281c21b86e583</originalsourceid><addsrcrecordid>eNpdkF9LwzAUxYMoOOe-QxD1rXqT_kn6KNM5QfBFn0uS3m4ZaTuTdrJvb-eGQ58unPPj3MMhZMLgjkEs77mMuTwhI5aILEoyKU7JCIDLCGScnZOLEFYAkDKRjIiZ28Uy8liGpa06GjrladX6WnW2bahtaLdEOu-1dkgfEdd0ZtGV1OMGlcOS6i1VNPS6ts7ZGjuP0ZfaoMNm0S0Hw29we0nOKuUCTg53TD5mT-_TefT69vwyfXiNTAJxF2GZAxOlZqBlJVmVApR6p3GZmzLluRRZpjQaZViSYFzlWnHJDGdaZpjKeExu97lr3372GLqitsGgc6rBtg8FF2ksQIoBvPoHrtreN0O3gkMyrAZ5PkA3e8j4NgSPVbH2tlZ-WzAodjsXPzsP3PUhTAWjXOVVY2z4hXmciDwVx3JhcJoF-uPPv3nf_giIRA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>204476099</pqid></control><display><type>article</type><title>High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey</title><source>Nature Journals</source><creator>Hughes, David H. ; Serjeant, Stephen ; Dunlop, James ; Rowan-Robinson, Michael ; Blain, Andrew ; Mann, Robert G. ; Ivison, Rob ; Peacock, John ; Efstathiou, Andreas ; Gear, Walter ; Oliver, Seb ; Lawrence, Andy ; Longair, Malcolm ; Goldschmidt, Pippa ; Jenness, Tim</creator><creatorcontrib>Hughes, David H. ; Serjeant, Stephen ; Dunlop, James ; Rowan-Robinson, Michael ; Blain, Andrew ; Mann, Robert G. ; Ivison, Rob ; Peacock, John ; Efstathiou, Andreas ; Gear, Walter ; Oliver, Seb ; Lawrence, Andy ; Longair, Malcolm ; Goldschmidt, Pippa ; Jenness, Tim</creatorcontrib><description>In the local Universe, most galaxies are dominated by stars, with less than ten per cent of their visible mass in the form of gas. Determining when most of these stars formed is one of the central issues of observational cosmology. Optical and ultraviolet observations of high-redshift galaxies (particularly those in the Hubble Deep Field) have been interpreted as indicating that the peak of star formation occurred between redshifts of 1 and 1.5. But it is known that star formation takes place in dense clouds, and is often hidden at optical wavelengths because of extinction by dust in the clouds. Here we report a deep submillimetre-wavelength survey of the Hubble Deep Field; these wavelengths trace directly the emission from dust that has been warmed by massive star-formation activity. The combined radiation of the five most significant detections accounts for 30–50 per cent of the previously unresolved background emission in this area. Four of these sources appear to be galaxies in the redshift range 2&lt; z &lt; 4, which, assuming these objects have properties comparable to local dust-enshrouded starburst galaxies, implies a star-formation rate during that period about a factor of five higher than that inferred from the optical and ultraviolet observations.</description><identifier>ISSN: 0028-0836</identifier><identifier>EISSN: 1476-4687</identifier><identifier>DOI: 10.1038/28328</identifier><identifier>CODEN: NATUAS</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>Astronomy ; Astrophysics ; Characteristics and properties of external galaxies and extragalactic objects ; Earth, ocean, space ; Exact sciences and technology ; Humanities and Social Sciences ; multidisciplinary ; Origin, formation, evolution, age, and star formation ; Science ; Science (multidisciplinary) ; Space telescopes ; Stars ; Stars &amp; galaxies ; Stellar systems. Galactic and extragalactic objects and systems. The universe</subject><ispartof>Nature (London), 1998-07, Vol.394 (6690), p.241-247</ispartof><rights>Macmillan Magazines Ltd. 1998</rights><rights>1998 INIST-CNRS</rights><rights>Copyright Macmillan Journals Ltd. Jul 16, 1998</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c403t-ed9017db10b8f81f500dbd901289cd5298766abecac144e3f9ba281c21b86e583</citedby><cites>FETCH-LOGICAL-c403t-ed9017db10b8f81f500dbd901289cd5298766abecac144e3f9ba281c21b86e583</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27901,27902</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=2347957$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Hughes, David H.</creatorcontrib><creatorcontrib>Serjeant, Stephen</creatorcontrib><creatorcontrib>Dunlop, James</creatorcontrib><creatorcontrib>Rowan-Robinson, Michael</creatorcontrib><creatorcontrib>Blain, Andrew</creatorcontrib><creatorcontrib>Mann, Robert G.</creatorcontrib><creatorcontrib>Ivison, Rob</creatorcontrib><creatorcontrib>Peacock, John</creatorcontrib><creatorcontrib>Efstathiou, Andreas</creatorcontrib><creatorcontrib>Gear, Walter</creatorcontrib><creatorcontrib>Oliver, Seb</creatorcontrib><creatorcontrib>Lawrence, Andy</creatorcontrib><creatorcontrib>Longair, Malcolm</creatorcontrib><creatorcontrib>Goldschmidt, Pippa</creatorcontrib><creatorcontrib>Jenness, Tim</creatorcontrib><title>High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey</title><title>Nature (London)</title><addtitle>Nature</addtitle><description>In the local Universe, most galaxies are dominated by stars, with less than ten per cent of their visible mass in the form of gas. Determining when most of these stars formed is one of the central issues of observational cosmology. Optical and ultraviolet observations of high-redshift galaxies (particularly those in the Hubble Deep Field) have been interpreted as indicating that the peak of star formation occurred between redshifts of 1 and 1.5. But it is known that star formation takes place in dense clouds, and is often hidden at optical wavelengths because of extinction by dust in the clouds. Here we report a deep submillimetre-wavelength survey of the Hubble Deep Field; these wavelengths trace directly the emission from dust that has been warmed by massive star-formation activity. The combined radiation of the five most significant detections accounts for 30–50 per cent of the previously unresolved background emission in this area. Four of these sources appear to be galaxies in the redshift range 2&lt; z &lt; 4, which, assuming these objects have properties comparable to local dust-enshrouded starburst galaxies, implies a star-formation rate during that period about a factor of five higher than that inferred from the optical and ultraviolet observations.</description><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Characteristics and properties of external galaxies and extragalactic objects</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Humanities and Social Sciences</subject><subject>multidisciplinary</subject><subject>Origin, formation, evolution, age, and star formation</subject><subject>Science</subject><subject>Science (multidisciplinary)</subject><subject>Space telescopes</subject><subject>Stars</subject><subject>Stars &amp; galaxies</subject><subject>Stellar systems. Galactic and extragalactic objects and systems. The universe</subject><issn>0028-0836</issn><issn>1476-4687</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1998</creationdate><recordtype>article</recordtype><recordid>eNpdkF9LwzAUxYMoOOe-QxD1rXqT_kn6KNM5QfBFn0uS3m4ZaTuTdrJvb-eGQ58unPPj3MMhZMLgjkEs77mMuTwhI5aILEoyKU7JCIDLCGScnZOLEFYAkDKRjIiZ28Uy8liGpa06GjrladX6WnW2bahtaLdEOu-1dkgfEdd0ZtGV1OMGlcOS6i1VNPS6ts7ZGjuP0ZfaoMNm0S0Hw29we0nOKuUCTg53TD5mT-_TefT69vwyfXiNTAJxF2GZAxOlZqBlJVmVApR6p3GZmzLluRRZpjQaZViSYFzlWnHJDGdaZpjKeExu97lr3372GLqitsGgc6rBtg8FF2ksQIoBvPoHrtreN0O3gkMyrAZ5PkA3e8j4NgSPVbH2tlZ-WzAodjsXPzsP3PUhTAWjXOVVY2z4hXmciDwVx3JhcJoF-uPPv3nf_giIRA</recordid><startdate>19980716</startdate><enddate>19980716</enddate><creator>Hughes, David H.</creator><creator>Serjeant, Stephen</creator><creator>Dunlop, James</creator><creator>Rowan-Robinson, Michael</creator><creator>Blain, Andrew</creator><creator>Mann, Robert G.</creator><creator>Ivison, Rob</creator><creator>Peacock, John</creator><creator>Efstathiou, Andreas</creator><creator>Gear, Walter</creator><creator>Oliver, Seb</creator><creator>Lawrence, Andy</creator><creator>Longair, Malcolm</creator><creator>Goldschmidt, Pippa</creator><creator>Jenness, Tim</creator><general>Nature Publishing Group UK</general><general>Nature Publishing</general><general>Nature Publishing Group</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7QG</scope><scope>7QL</scope><scope>7QP</scope><scope>7QR</scope><scope>7RV</scope><scope>7SN</scope><scope>7SS</scope><scope>7ST</scope><scope>7T5</scope><scope>7TG</scope><scope>7TK</scope><scope>7TM</scope><scope>7TO</scope><scope>7U9</scope><scope>7X2</scope><scope>7X7</scope><scope>7XB</scope><scope>88A</scope><scope>88E</scope><scope>88G</scope><scope>88I</scope><scope>8AF</scope><scope>8AO</scope><scope>8C1</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FH</scope><scope>8FI</scope><scope>8FJ</scope><scope>8FK</scope><scope>8G5</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>ATCPS</scope><scope>AZQEC</scope><scope>BBNVY</scope><scope>BEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>D1I</scope><scope>DWQXO</scope><scope>FR3</scope><scope>FYUFA</scope><scope>GHDGH</scope><scope>GNUQQ</scope><scope>GUQSH</scope><scope>H94</scope><scope>HCIFZ</scope><scope>K9.</scope><scope>KB.</scope><scope>KB0</scope><scope>KL.</scope><scope>L6V</scope><scope>LK8</scope><scope>M0K</scope><scope>M0S</scope><scope>M1P</scope><scope>M2M</scope><scope>M2O</scope><scope>M2P</scope><scope>M7N</scope><scope>M7P</scope><scope>M7S</scope><scope>MBDVC</scope><scope>NAPCQ</scope><scope>P5Z</scope><scope>P62</scope><scope>P64</scope><scope>PATMY</scope><scope>PCBAR</scope><scope>PDBOC</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PSYQQ</scope><scope>PTHSS</scope><scope>PYCSY</scope><scope>Q9U</scope><scope>R05</scope><scope>RC3</scope><scope>S0X</scope><scope>SOI</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>19980716</creationdate><title>High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey</title><author>Hughes, David H. ; Serjeant, Stephen ; Dunlop, James ; Rowan-Robinson, Michael ; Blain, Andrew ; Mann, Robert G. ; Ivison, Rob ; Peacock, John ; Efstathiou, Andreas ; Gear, Walter ; Oliver, Seb ; Lawrence, Andy ; Longair, Malcolm ; Goldschmidt, Pippa ; Jenness, Tim</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c403t-ed9017db10b8f81f500dbd901289cd5298766abecac144e3f9ba281c21b86e583</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1998</creationdate><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Characteristics and properties of external galaxies and extragalactic objects</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Humanities and Social Sciences</topic><topic>multidisciplinary</topic><topic>Origin, formation, evolution, age, and star formation</topic><topic>Science</topic><topic>Science (multidisciplinary)</topic><topic>Space telescopes</topic><topic>Stars</topic><topic>Stars &amp; galaxies</topic><topic>Stellar systems. Galactic and extragalactic objects and systems. The universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hughes, David H.</creatorcontrib><creatorcontrib>Serjeant, Stephen</creatorcontrib><creatorcontrib>Dunlop, James</creatorcontrib><creatorcontrib>Rowan-Robinson, Michael</creatorcontrib><creatorcontrib>Blain, Andrew</creatorcontrib><creatorcontrib>Mann, Robert G.</creatorcontrib><creatorcontrib>Ivison, Rob</creatorcontrib><creatorcontrib>Peacock, John</creatorcontrib><creatorcontrib>Efstathiou, Andreas</creatorcontrib><creatorcontrib>Gear, Walter</creatorcontrib><creatorcontrib>Oliver, Seb</creatorcontrib><creatorcontrib>Lawrence, Andy</creatorcontrib><creatorcontrib>Longair, Malcolm</creatorcontrib><creatorcontrib>Goldschmidt, Pippa</creatorcontrib><creatorcontrib>Jenness, Tim</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Animal Behavior Abstracts</collection><collection>Bacteriology Abstracts (Microbiology B)</collection><collection>Calcium &amp; Calcified Tissue Abstracts</collection><collection>Chemoreception Abstracts</collection><collection>ProQuest Nursing and Allied Health Journals</collection><collection>Ecology Abstracts</collection><collection>Entomology Abstracts (Full archive)</collection><collection>Environment Abstracts</collection><collection>Immunology Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Neurosciences Abstracts</collection><collection>Nucleic Acids Abstracts</collection><collection>Oncogenes and Growth Factors Abstracts</collection><collection>Virology and AIDS Abstracts</collection><collection>Agricultural Science Collection</collection><collection>Health &amp; Medical Collection (Proquest)</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Biology Database (Alumni Edition)</collection><collection>Medical Database (Alumni Edition)</collection><collection>Psychology Database (Alumni)</collection><collection>Science Database (Alumni Edition)</collection><collection>STEM Database</collection><collection>ProQuest Pharma Collection</collection><collection>Public Health Database (Proquest)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Natural Science Collection</collection><collection>Hospital Premium Collection</collection><collection>Hospital Premium Collection (Alumni Edition)</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>Research Library (Alumni Edition)</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central</collection><collection>Advanced Technologies &amp; Aerospace Database‎ (1962 - current)</collection><collection>Agricultural &amp; Environmental Science Collection</collection><collection>ProQuest Central Essentials</collection><collection>Biological Science Collection</collection><collection>eLibrary</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric &amp; Aquatic Science Collection</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ProQuest One Community College</collection><collection>ProQuest Materials Science Collection</collection><collection>ProQuest Central</collection><collection>Engineering Research Database</collection><collection>Health Research Premium Collection</collection><collection>Health Research Premium Collection (Alumni)</collection><collection>ProQuest Central Student</collection><collection>Research Library Prep</collection><collection>AIDS and Cancer Research Abstracts</collection><collection>SciTech Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>ProQuest Health &amp; Medical Complete (Alumni)</collection><collection>Materials Science Database</collection><collection>Nursing &amp; Allied Health Database (Alumni Edition)</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>ProQuest Engineering Collection</collection><collection>Biological Sciences</collection><collection>Agricultural Science Database</collection><collection>Health &amp; Medical Collection (Alumni Edition)</collection><collection>PML(ProQuest Medical Library)</collection><collection>Psychology Database</collection><collection>ProQuest research library</collection><collection>ProQuest Science Journals</collection><collection>Algology Mycology and Protozoology Abstracts (Microbiology C)</collection><collection>Biological Science Database</collection><collection>Engineering Database</collection><collection>Research Library (Corporate)</collection><collection>Nursing &amp; Allied Health Premium</collection><collection>ProQuest advanced technologies &amp; aerospace journals</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>Biotechnology and BioEngineering Abstracts</collection><collection>Environmental Science Database</collection><collection>Earth, Atmospheric &amp; Aquatic Science Database</collection><collection>Materials Science Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest One Psychology</collection><collection>Engineering collection</collection><collection>Environmental Science Collection</collection><collection>ProQuest Central Basic</collection><collection>University of Michigan</collection><collection>Genetics Abstracts</collection><collection>SIRS Editorial</collection><collection>Environment Abstracts</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Nature (London)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hughes, David H.</au><au>Serjeant, Stephen</au><au>Dunlop, James</au><au>Rowan-Robinson, Michael</au><au>Blain, Andrew</au><au>Mann, Robert G.</au><au>Ivison, Rob</au><au>Peacock, John</au><au>Efstathiou, Andreas</au><au>Gear, Walter</au><au>Oliver, Seb</au><au>Lawrence, Andy</au><au>Longair, Malcolm</au><au>Goldschmidt, Pippa</au><au>Jenness, Tim</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey</atitle><jtitle>Nature (London)</jtitle><stitle>Nature</stitle><date>1998-07-16</date><risdate>1998</risdate><volume>394</volume><issue>6690</issue><spage>241</spage><epage>247</epage><pages>241-247</pages><issn>0028-0836</issn><eissn>1476-4687</eissn><coden>NATUAS</coden><abstract>In the local Universe, most galaxies are dominated by stars, with less than ten per cent of their visible mass in the form of gas. Determining when most of these stars formed is one of the central issues of observational cosmology. Optical and ultraviolet observations of high-redshift galaxies (particularly those in the Hubble Deep Field) have been interpreted as indicating that the peak of star formation occurred between redshifts of 1 and 1.5. But it is known that star formation takes place in dense clouds, and is often hidden at optical wavelengths because of extinction by dust in the clouds. Here we report a deep submillimetre-wavelength survey of the Hubble Deep Field; these wavelengths trace directly the emission from dust that has been warmed by massive star-formation activity. The combined radiation of the five most significant detections accounts for 30–50 per cent of the previously unresolved background emission in this area. Four of these sources appear to be galaxies in the redshift range 2&lt; z &lt; 4, which, assuming these objects have properties comparable to local dust-enshrouded starburst galaxies, implies a star-formation rate during that period about a factor of five higher than that inferred from the optical and ultraviolet observations.</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><doi>10.1038/28328</doi><tpages>7</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0028-0836
ispartof Nature (London), 1998-07, Vol.394 (6690), p.241-247
issn 0028-0836
1476-4687
language eng
recordid cdi_proquest_miscellaneous_27537087
source Nature Journals
subjects Astronomy
Astrophysics
Characteristics and properties of external galaxies and extragalactic objects
Earth, ocean, space
Exact sciences and technology
Humanities and Social Sciences
multidisciplinary
Origin, formation, evolution, age, and star formation
Science
Science (multidisciplinary)
Space telescopes
Stars
Stars & galaxies
Stellar systems. Galactic and extragalactic objects and systems. The universe
title High-redshift star formation in the Hubble Deep Field revealed by a submillimetre-wavelength survey
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-06T15%3A50%3A19IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=High-redshift%20star%20formation%20in%20the%20Hubble%20Deep%20Field%20revealed%20by%20a%20submillimetre-wavelength%20survey&rft.jtitle=Nature%20(London)&rft.au=Hughes,%20David%20H.&rft.date=1998-07-16&rft.volume=394&rft.issue=6690&rft.spage=241&rft.epage=247&rft.pages=241-247&rft.issn=0028-0836&rft.eissn=1476-4687&rft.coden=NATUAS&rft_id=info:doi/10.1038/28328&rft_dat=%3Cproquest_cross%3E27537087%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c403t-ed9017db10b8f81f500dbd901289cd5298766abecac144e3f9ba281c21b86e583%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=204476099&rft_id=info:pmid/&rfr_iscdi=true