EVIDENCE FOR UBIQUITOUS HIGH-EQUIVALENT-WIDTH NEBULAR EMISSION IN z similar to 7 GALAXIES : TOWARD A CLEAN MEASUREMENT OF THE SPECIFIC STAR-FORMATION RATE USING A SAMPLE OF BRIGHT, MAGNIFIED GALAXIES

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dc.contributor.authorSmit, R.
dc.contributor.authorBouwens, R. J.
dc.contributor.authorLabbé, I.
dc.contributor.authorZheng, W.
dc.contributor.authorLemze, D.
dc.contributor.authorFord, H.
dc.contributor.authorBradley, L.
dc.contributor.authorCoe, D.
dc.contributor.authorPostman, M.
dc.contributor.authorInfante Lira, Leopoldo
dc.date.accessioned2021-05-31T03:41:37Z
dc.date.available2021-05-31T03:41:37Z
dc.date.issued2014
dc.format.extent8 páginas
dc.fuente.origenConveris
dc.identifier.doi10.1088/0004-637X/784/1/58
dc.identifier.eissn1538-4357
dc.identifier.issn0004-637X
dc.identifier.urihttps://doi.org/10.1088/0004-637X/784/1/58
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/59573
dc.identifier.wosidWOS:000335457000058
dc.issue.numeroNo. 1
dc.language.isoen
dc.nota.accesoContenido completo
dc.pagina.final8
dc.pagina.inicio1
dc.revistaAstrophysical Journales_ES
dc.rightsacceso abierto
dc.titleEVIDENCE FOR UBIQUITOUS HIGH-EQUIVALENT-WIDTH NEBULAR EMISSION IN z similar to 7 GALAXIES : TOWARD A CLEAN MEASUREMENT OF THE SPECIFIC STAR-FORMATION RATE USING A SAMPLE OF BRIGHT, MAGNIFIED GALAXIESes_ES
dc.typeartículo
dc.volumenVol. 784
sipa.codpersvinculados55248
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