Photometric Redshifts in the Hubble Deep Field

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dc.creatorSawicki, M. J.
dc.creatorLin, H.
dc.creatorYee, H. K. C.
dc.date1996-10-03
dc.date.accessioned2026-07-07T02:22:00Z
dc.date.available2026-07-07T02:22:00Z
dc.descriptionPhotometric redshifts for galaxies in the Hubble Deep Field are measured. Luminosity functions show steepening of the faint-end slope and mild brightening of M* out to z~3, followed by a decline at higher z; an excess of faint, star-forming galaxies is seen at low z. Our results are consistent with the formation of large galaxies at z=2-3, followed by that of dwarfs at z<1.
dc.description2 pages. To appear in the proceedings of the 37th Herstmonceux conference, "HST and the High Redshift Universe"
dc.identifierhttps://arxiv.org/abs/astro-ph/9610027
dc.identifierhttp://arxiv.org/abs/astro-ph/9610027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10718
dc.subjectAstrophysics
dc.titlePhotometric Redshifts in the Hubble Deep Field
dc.typetext

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