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The HI content of star-forming galaxies at z = 0.24

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dc.contributor.authorLah, Philip
dc.contributor.authorChengalur, Jayaram N
dc.contributor.authorBriggs, Franklin
dc.contributor.authorColless, Matthew
dc.contributor.authorDe Propris, Roberto
dc.contributor.authorPracy, Michael
dc.contributor.authorde Blok, Willem
dc.contributor.authorFujita, Shinobu
dc.contributor.authorAjiki, Masaru
dc.contributor.authorShioya, Yasuhiro
dc.contributor.authorNagao, Tohru
dc.contributor.authorMurayama, Takashi
dc.contributor.authorTaniguchi, Yoshiaki
dc.contributor.authorYagi, Masafumi
dc.contributor.authorOkamura, Sadanori
dc.date.accessioned2015-12-07T22:17:02Z
dc.date.issued2006
dc.date.updated2015-12-07T08:01:25Z
dc.description.abstractWe use observations from the Giant Metrewave Radio Telescope (GMRT) to measure the atomic hydrogen gas content of star-forming galaxies at z = 0.24 (i.e. a look-back time of ∼3 Gyr). The sample of galaxies studied were selected from Hα-emitting fieldga
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/18345
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Galaxies: evolution; Galaxies: ISM; Radio continuum: galaxies; Radio lines: galaxies
dc.titleThe HI content of star-forming galaxies at z = 0.24
dc.typeJournal article
local.bibliographicCitation.issue3
local.bibliographicCitation.lastpage1366
local.bibliographicCitation.startpage1357
local.contributor.affiliationLah, Philip, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationChengalur, Jayaram N, University of Pune
local.contributor.affiliationBriggs, Franklin, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationColless, Matthew, Anglo-Australian Observatory
local.contributor.affiliationDe Propris, Roberto, Cerro Tololo Inter-American Observatory
local.contributor.affiliationPracy, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationde Blok, Willem, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationFujita, Shinobu, Tohoku University
local.contributor.affiliationAjiki, Masaru, Tohoku University
local.contributor.affiliationShioya, Yasuhiro, Ehime University
local.contributor.affiliationNagao, Tohru, National Astronomical Observatory of Japan
local.contributor.affiliationMurayama, Takashi, Tohoku University
local.contributor.affiliationTaniguchi, Yoshiaki, Ehime University
local.contributor.affiliationYagi, Masafumi, National Astronomical Observatory of Japan
local.contributor.affiliationOkamura, Sadanori, University of Tokyo
local.contributor.authoruidLah, Philip, u3173491
local.contributor.authoruidBriggs, Franklin, u4049161
local.contributor.authoruidPracy, Michael, u4016224
local.contributor.authoruidde Blok, Willem, u4191932
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4193696xPUB4
local.identifier.citationvolume376
local.identifier.doi10.1111/j.1365-2966.2007.11540.x
local.identifier.scopusID2-s2.0-34147131320
local.type.statusPublished Version

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