Galaxy evolution from a microJansky radio survey

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dc.contributor.authorAfonso, J
dc.contributor.authorMobasher, Bahram
dc.contributor.authorHopkins, Andrew M
dc.contributor.authorGeorgakakis, Antonis
dc.contributor.authorCram, Lawrence
dc.contributor.authorChan, B
dc.date.accessioned2015-12-08T22:42:10Z
dc.date.issued2003
dc.date.updated2015-12-08T10:33:32Z
dc.description.abstractA strong evolution of galaxies is observed for 0 < z < 1, as evidenced by an increase of almost an order of magnitude in the galaxy star-formation rate density. However, it is known that dust obscuration has affected our understanding of galaxy evolution
dc.identifier.issn0004-640X
dc.identifier.urihttp://hdl.handle.net/1885/36972
dc.publisherKluwer Academic Publishers
dc.sourceAstrophysics and Space Science
dc.subjectKeywords: Radio continuum: galaxies - galaxies: evolution - galaxies: starburst
dc.titleGalaxy evolution from a microJansky radio survey
dc.typeJournal article
local.bibliographicCitation.lastpage153
local.bibliographicCitation.startpage149
local.contributor.affiliationAfonso, J, Universidade de Lisboa
local.contributor.affiliationMobasher, Bahram, Space Telescope Science Institute
local.contributor.affiliationHopkins, Andrew M, University of Pittsburgh / ATNF / AAO/ Sydney University
local.contributor.affiliationGeorgakakis, Antonis, National Observatory of Athens
local.contributor.affiliationCram, Lawrence, Administrative Division, ANU
local.contributor.affiliationChan, B, University of Sydney
local.contributor.authoremailu4139921@anu.edu.au
local.contributor.authoruidCram, Lawrence, u4139921
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu3379551xPUB143
local.identifier.citationvolume285
local.identifier.doi10.1023/A:1024686431681
local.identifier.scopusID2-s2.0-1642502267
local.identifier.uidSubmittedByu3379551
local.type.statusPublished Version

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