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Authordc.contributor.authorHuertas Company, M. 
Authordc.contributor.authorGravet, R. 
Authordc.contributor.authorCabrera Vives, Guillermo 
Authordc.contributor.authorPérez González, P. G. 
Authordc.contributor.authorKartaltepe, J. S. 
Authordc.contributor.authorBarro, G. 
Authordc.contributor.authorBernardi, M. 
Authordc.contributor.authorMei, S. 
Authordc.contributor.authorShankar, F. 
Authordc.contributor.authorDimauro, P. 
Authordc.contributor.authorBell, E. F. 
Authordc.contributor.authorKocevski, D. 
Authordc.contributor.authorKoo, D. C. 
Authordc.contributor.authorFaber, S. M. 
Authordc.contributor.authorMcintosh, D. H. 
Admission datedc.date.accessioned2016-01-12T14:32:13Z
Available datedc.date.available2016-01-12T14:32:13Z
Publication datedc.date.issued2015
Cita de ítemdc.identifier.citationAstrophysical Journal Supplement Series Volumen: 221 Número: 1 Número de artículo: 8 Nov. 2015en_US
Identifierdc.identifier.otherDOI: 10.1088/0067-0049/221/1/8
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/136386
General notedc.descriptionArtículo de publicación ISIen_US
Abstractdc.description.abstractWe present a catalog of visual-like H-band morphologies of similar to 50.000 galaxies (H-f160w < 24.5) in the 5 CANDELS fields (GOODS-N, GOODS-S, UDS, EGS, and COSMOS). Morphologies are estimated using Convolutional Neural Networks (ConvNets). The median redshift of the sample is < z > similar to 1.25. The algorithm is trained on GOODS-S, for which visual classifications are publicly available, and then applied to the other 4 fields. Following the CANDELS main morphology classification scheme, our model retrieves for each galaxy the probabilities of having a spheroid or a disk, presenting an irregularity, being compact or a point source, and being unclassifiable. ConvNets are able to predict the fractions of votes given to a galaxy image with zero bias and similar to 10% scatter. The fraction of mis-classifications is less than 1%. Our classification scheme represents a major improvement with respect to Concentration-Asymmetry-Smoothness-based methods, which hit a 20%-30% contamination limit at high z.en_US
Patrocinadordc.description.sponsorshipCONICYT-Chile DPI20140090 Institut Universitaire de France (IUF) NSF AST-08-08133 NASA HST-GO-12060.10Aen_US
Lenguagedc.language.isoenen_US
Publisherdc.publisherIOP Publishingen_US
Type of licensedc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Keywordsdc.subjectCatalogsen_US
Keywordsdc.subjectGalaxies: high-redshiften_US
Keywordsdc.subjectGalaxies: structureen_US
Keywordsdc.subjectSurveysen_US
Títulodc.titleA catalog of visual-like morphologies in the 5 candels fields using deep-learningen_US
Document typedc.typeArtículo de revista


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Atribución-NoComercial-SinDerivadas 3.0 Chile
Except where otherwise noted, this item's license is described as Atribución-NoComercial-SinDerivadas 3.0 Chile