The ALMA Spectroscopic Survey in the HUDF : A Model to Explain Observed 1.1 and 0.85 mm Dust Continuum Number Counts
dc.contributor.author | Popping, G. | |
dc.contributor.author | Walter, F. | |
dc.contributor.author | Behroozi, P. | |
dc.contributor.author | Gozález López, José Ignacio | |
dc.contributor.author | Hayward, C. C. | |
dc.contributor.author | Somerville, R. S. | |
dc.contributor.author | van der Werf, P. | |
dc.contributor.author | Aravena, M. | |
dc.contributor.author | Assef, R. J. | |
dc.contributor.author | Boogaard, L. | |
dc.contributor.author | Bauer, Franz Erik | |
dc.contributor.author | Cortes, P. C. | |
dc.contributor.author | Cox, P. | |
dc.contributor.author | Díaz Santos, T. | |
dc.contributor.author | Decarli, R. | |
dc.contributor.author | Franco, M. | |
dc.contributor.author | Ivison, R. | |
dc.contributor.author | Riechers, D. | |
dc.contributor.author | Rix, H. W. | |
dc.contributor.author | Weiss, A. | |
dc.date.accessioned | 2022-03-16T19:39:42Z | |
dc.date.available | 2022-03-16T19:39:42Z | |
dc.date.issued | 2020 | |
dc.format.extent | 15 páginas | |
dc.fuente.origen | Converis | |
dc.identifier.doi | 10.3847/1538-4357/ab76c0 | |
dc.identifier.eissn | 1538-4357 | |
dc.identifier.issn | 0004-637X | |
dc.identifier.uri | https://doi.org/10.3847/1538-4357/ab76c0 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/63476 | |
dc.identifier.wosid | WOS:000521436700001 | |
dc.information.autoruc | Instituto de astrofísica ; Gozález López, José Ignacio ; 0000-0003-3926-1411 ; 154597 | |
dc.issue.numero | No. 2 | |
dc.language.iso | en | |
dc.pagina.final | 15 | |
dc.pagina.inicio | 1 | |
dc.revista | ASTROPHYS J | es_ES |
dc.rights | acceso abierto | |
dc.title | The ALMA Spectroscopic Survey in the HUDF : A Model to Explain Observed 1.1 and 0.85 mm Dust Continuum Number Counts | es_ES |
dc.type | artículo | |
dc.volumen | Vol. 891 | |
sipa.codpersvinculados | 154597 |
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