ANGULAR-CORRELATION FUNCTION OF FAINT GALAXIES

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dc.contributor.authorPRITCHET, CJ
dc.contributor.authorINFANTE, L
dc.date.accessioned2025-01-23T19:22:00Z
dc.date.available2025-01-23T19:22:00Z
dc.date.issued1992
dc.description.abstractThe angular correlation function has been computed for a two-color survey Of faint galaxies (J < 24, F < 23) covering a approximately 2.4 deg2 area near the North Galactic Pole. Faint galaxies are found to belong to a population that is more weakly clustered than luminous nearby galaxies, by a factor greater than or similar to 2 at J = 22 and greater than or similar to 4 at J = 24. Objects selected in the F (red) band are closer to model predictions than those observed in the J band. These observations are interpreted in terms of models in which (weakly clustered) bursting dwarf galaxies comprise the bulk of the number counts at faint magnitudes.
dc.fuente.origenWOS
dc.identifier.eissn1538-4357
dc.identifier.issn0004-637X
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/98932
dc.identifier.wosidWOS:A1992JV04800010
dc.issue.numero1
dc.language.isoen
dc.pagina.finalL38
dc.pagina.inicioL35
dc.revistaAstrophysical journal
dc.rightsacceso restringido
dc.subjectCOSMOLOGY, OBSERVATIONS
dc.subjectGALAXIES, CLUSTERING
dc.subjectGALAXIES, EVOLUTION
dc.titleANGULAR-CORRELATION FUNCTION OF FAINT GALAXIES
dc.typeartículo
dc.volumen399
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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