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Authordc.contributor.authorGawiser, Eric 
Authordc.contributor.authorvan Dokkum, Pieter es_CL
Authordc.contributor.authorHerrera, David es_CL
Authordc.contributor.authorMaza Sancho, José es_CL
Authordc.contributor.authorCastander, Francisco es_CL
Authordc.contributor.authorInfante, Leopoldo es_CL
Authordc.contributor.authorLira Teillery, Paulina es_CL
Authordc.contributor.authorQuadri, Ryan es_CL
Authordc.contributor.authorToner, Ruth es_CL
Authordc.contributor.authorTreister, Ezequiel es_CL
Authordc.contributor.authorUrry, C. Megan es_CL
Authordc.contributor.authorAltmann, Martín es_CL
Authordc.contributor.authorAssef, Roberto es_CL
Authordc.contributor.authorChristlein, Daniel es_CL
Authordc.contributor.authorCoppi, Paolo es_CL
Authordc.contributor.authorDurán, María Fernanda es_CL
Authordc.contributor.authorMarijn, Franx es_CL
Authordc.contributor.authorGalaz, Gaspar, 1967- es_CL
Authordc.contributor.authorHuerta, Leonor es_CL
Authordc.contributor.authorCharles, Liu es_CL
Authordc.contributor.authorLópez Morales, Sebastián es_CL
Authordc.contributor.authorMéndez Bussard, René Alejandro es_CL
Authordc.contributor.authorMoore, David C. es_CL
Authordc.contributor.authorRubio López, Mónica es_CL
Authordc.contributor.authorRuiz González, María Teresa es_CL
Authordc.contributor.authorSune, Toft es_CL
Authordc.contributor.authorSukyoung K., Yi es_CL
Admission datedc.date.accessioned2012-10-18T15:32:57Z
Available datedc.date.available2012-10-18T15:32:57Z
Publication datedc.date.issued2006-01
Cita de ítemdc.identifier.citationThe Astrophysical Journal Supplement Series, 162:1–19, 2006 Januaryes_CL
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/125680
General notedc.descriptionArtículo de publicación ISI
Abstractdc.description.abstractWe present UBVRIz0 optical images taken with MOSAIC on the CTIO 4 m telescope of the 0.32 deg2 Extended Hubble Deep Field–South. This is one of four fields comprising the MUSYC survey, which is optimized for the study of galaxies at z ¼ 3, active galactic nucleus (AGN) demographics, and Galactic structure. Our methods used for astrometric calibration, weighted image combination, and photometric calibration in ABmagnitudes are described. We calculate corrected aperture photometry and its uncertainties and find through tests that these provide a significant improvement upon standard techniques. Our photometric catalog of 62,968 objects is complete to a total magnitude of RAB ¼ 25, with R-band counts consistent with results from the literature.We select z ’ 3 Lyman break galaxy (LBG) candidates from their UVR colors and find a sky surface density of 1.4 arcmin 2 and an angular correlation function w( ) ¼ (2:3 1:0) 0:8, consistent with previous findings that high-redshift Lyman break galaxies reside in massive dark matter halos. Our images and catalogs are available onlinees_CL
Lenguagedc.language.isoen_USes_CL
Publisherdc.publisherIOP Publishing.es_CL
Keywordsdc.subjectgalaxies: high-redshiftes_CL
Títulodc.titleTHE MULTIWAVELENGTH SURVEY BY YALE-CHILE (MUSYC): SURVEY DESIGN AND DEEP PUBLIC UBVRIz0 IMAGES AND CATALOGS OF THE EXTENDED HUBBLE DEEP FIELD–SOUTHes_CL
Document typedc.typeArtículo de revista


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