Photometric Redshifts in lensing clusters: Identification and Calibration of faint high-z galaxies

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dc.creatorPello, Roser
dc.creatorKneib, Jean-Paul
dc.creatorBolzonella, Micol
dc.creatorMiralles, Joan-Marc
dc.date1999-07-05
dc.date.accessioned2026-07-07T02:32:17Z
dc.date.available2026-07-07T02:32:17Z
dc.descriptionWe discuss a method aiming to use photometric redshifts in lensing clusters to access the population of distant background sources. The amplification provided by gravitational lensing allows to calibrate photometric redshifts 1 to 3 magnitudes deeper with respect to field studies. We present and discuss some results obtained with this procedure on extensively studied clusters, as well as the future issues of this project.
dc.description6 pages, 4 figures, Conference Proceedings of the "Photometric Redshifts and High Redshift Galaxies", April 28-30, 1999, Pasadena
dc.identifierhttps://arxiv.org/abs/astro-ph/9907054
dc.identifierhttp://arxiv.org/abs/astro-ph/9907054
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14451
dc.subjectAstrophysics
dc.titlePhotometric Redshifts in lensing clusters: Identification and Calibration of faint high-z galaxies
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