Photometric Redshifts in Hubble Deep Field South

Simple item page
dc.creatorClements, D. L.
dc.date1999-09-02
dc.date.accessioned2026-07-07T02:33:02Z
dc.date.available2026-07-07T02:33:02Z
dc.descriptionWe apply both a traditional `dropout' approach and a photometric redshift estimation technique to the Hubble Deep Field South data. We give a list of dropout selected z$\sim$3 objects, and show their images. We then discuss our photometric redshift estimation technique, demonstrate both its effectiveness and the role played by near-IR data, and then apply it to HDF-S to obtain an estimated redshift distribution.
dc.descriptionTo appear in "Photometric Redshifts and High Redshift Galaxies", eds. R. Weymann, L. Storrie-Lombardi, M. Sawicki & R. Brunner
dc.identifierhttps://arxiv.org/abs/astro-ph/9909045
dc.identifierhttp://arxiv.org/abs/astro-ph/9909045
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14684
dc.subjectAstrophysics
dc.titlePhotometric Redshifts in Hubble Deep Field South
dc.typetext

Files

Collections

arXiv