Astrophysical Journal

dc.creatorWu, Jingwen
dc.creatorJun, Hyunsung D
dc.creatorAssef, Roberto J
dc.creatorTsai, Chao-Wei
dc.creatorWright, Edward L
dc.creatorEisenhardt, Peter R M
dc.creatorBlain, Andrew
dc.creatorStern, Daniel
dc.creatorDiaz-Santos, Tanio
dc.creatorDenney, Kelly D
dc.date2018-12-07T13:33:30Z
dc.date2022-07-07T21:38:00Z
dc.date2015
dc.date2018-12-07T13:33:30Z
dc.date2022-07-07T21:38:00Z
dc.date2018
dc.date.accessioned2023-08-21T22:48:40Z
dc.date.available2023-08-21T22:48:40Z
dc.identifier1151239
dc.identifier1151239
dc.identifierhttps://hdl.handle.net/10533/232544
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8291928
dc.descriptionHot, dust-obscured galaxies, or "Hot DOGs," are a rare, dusty, hyperluminous galaxy population discovered by the WISE mission. Predominantly at redshifts 2-3, they include the most luminous known galaxies in the universe. Their high luminosities likely c
dc.descriptionRegular
dc.descriptionFONDECYT
dc.descriptionFONDECYT
dc.languageeng
dc.relationhandle/10533/111557
dc.relationhandle/10533/111541
dc.relationhandle/10533/108045
dc.relationhttps://arxiv.org/pdf/1703.06888.pdf
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleEddington-limited accretion in z similar to 2 wise-selected hot, dust-obscured galaxies
dc.titleAstrophysical Journal
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


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