The Stony Brook Photometric Redshifts of Faint Galaxies in the Hubble Deep Fields

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We report on some aspects of the current status of our efforts to establish properties of faint galaxies by applying our photometric redshift technique to faint galaxies in the HDF and HDF-S WFPC2 and NICMOS fields.
6 pages, 4 figures, to appear in "Photometric Redshifts and High Redshift Galaxies", eds. R. Weymann, L. Storrie-Lombardi, M. Sawicki & R. Brunner

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/14517

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/9907281
 http://arxiv.org/abs/astro-ph/9907281

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arXiv