Photometric Redshift Techniques: Reliability and Applications

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dc.creatorYee, H. K. C.
dc.date1998-09-27
dc.date.accessioned2026-07-07T02:28:05Z
dc.date.available2026-07-07T02:28:05Z
dc.descriptionThis article describes the various photometric techniques currently being used, including some preliminary results from the large CNOC2 redshift survey. It also presents a critical look at the reliability of the photometric redshift technique, in part using the HDF results from various groups as a case study.
dc.description11 pages, Latex, 3 postscript figures. A review article to appear in the proceedings of the Xth Recontres de Blois: Birth of Galaxies; Blois, France, July 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9809347
dc.identifierhttp://arxiv.org/abs/astro-ph/9809347
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12968
dc.subjectAstrophysics
dc.titlePhotometric Redshift Techniques: Reliability and Applications
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