ALMA spectroscopic Survey in the Hubble Ultra Deep Field : The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass

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dc.contributor.authorBouwens, Rychard J.
dc.contributor.authorAravena, Manuel
dc.contributor.authorDecarli, Roberto
dc.contributor.authorWalter, Fabian
dc.contributor.authorCunha, Elisabete da
dc.contributor.authorLabbé, Ivo
dc.contributor.authorBauer, Franz Erik
dc.contributor.authorBertoldi, Frank
dc.contributor.authorCarilli, Chris
dc.contributor.authorChapman, Scott
dc.contributor.authorDaddi, Emanuele
dc.contributor.authorHodge, Jacqueline
dc.contributor.authorIvison, Rob J.
dc.contributor.authorKarim, Alex
dc.contributor.authorLe Fevre, Olivier
dc.contributor.authorMagnelli, Benjamin
dc.contributor.authorOta, Kazuaki
dc.contributor.authorRiechers, Dominik
dc.contributor.authorSmail, Ian R.
dc.contributor.authorWerf, Paul van der
dc.contributor.authorWeiss, Axel
dc.contributor.authorCox, Pierre
dc.contributor.authorElbaz, David
dc.contributor.authorGonzalez-Lopez, Jorge
dc.contributor.authorInfante Lira, Leopoldo
dc.contributor.authorOesch, Pascal
dc.contributor.authorWagg, Jeff
dc.contributor.authorWilkins, Steve
dc.date.accessioned2020-07-22T02:40:15Z
dc.date.available2020-07-22T02:40:15Z
dc.date.issued2016
dc.fechaingreso.objetodigital2024-07-11
dc.format.extent32 páginas
dc.fuente.origenConveris
dc.identifier.doi10.3847/1538-4357/833/1/72
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357
dc.identifier.urihttps://doi.org/10.3847/1538-4357/833/1/72
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/33814
dc.issue.numeroNo. 1
dc.language.isoen
dc.nota.accesoContenido completo
dc.pagina.final32
dc.pagina.inicio1
dc.revistaAstrophysical Journales_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherTelescopio Espacial Hubblees_ES
dc.subject.otherObservaciones astronomicases_ES
dc.subject.otherEstrellas - Formaciónes_ES
dc.subject.otherGalaxiases_ES
dc.titleALMA spectroscopic Survey in the Hubble Ultra Deep Field : The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Masses_ES
dc.typeartículo
dc.volumenVol. 833
sipa.codpersvinculados1007961
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ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD THE INFRARED EXCESS OF UV-SELECTED z = 2–10 GALAXIES AS A FUNCTION OF UV-CONTINUUM SLOPE AND STELLAR MASS.pdf
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