U-band study of the z=2.38 Filament

dc.contributor.authorColbert, Jamesen_AU
dc.contributor.authorTeplitz, Harryen_AU
dc.contributor.authorSiana, Brianen_AU
dc.contributor.authorFrancis, Paulen_AU
dc.contributor.authorWoodgate, Bruceen_AU
dc.contributor.authorPalunas, Povilasen_AU
dc.contributor.authorWilliger, Gerarden_AU
dc.date.accessioned2018-09-12T06:17:44Z
dc.date.available2018-09-12T06:17:44Z
dc.date.created2006en_AU
dc.description.abstractWe request 3 nights on the CTIO Blanco 4m with the MOSAIC camera to image the z=2.38 Filament in U-band. The primary goal is to achieve depths in the U filter (26.5 AB) necessary to identify further members of this high redshift structure, using the "BX" method of Steidel et al. (2004) and photometric redshifts. Combined with deep Spitzer (IRAC and MIPS 24(mu)m) and near-IR data, we will measure mass, ages, dust content, and SFR throughout this region of early galaxy assembly. Further structure members will also facilitate a robust determination of the weakly-detected filament and void distribution. We will also obtain z'-band imaging in order to provide a full data set for photometric redshifts.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.urihttp://hdl.handle.net/1885/147380en_AU
dc.language.isoen_AUen_AU
dc.publisherNOAOen_AU
dc.rights© The Author(s)en_AU
dc.source.urihttps://www.noao.edu/perl/abstract?2006A-0427en_AU
dc.titleU-band study of the z=2.38 Filamenten_AU
dc.typeDataseten_AU
dcterms.accessRightsOpen Accessen_AU
local.contributor.affiliationFrancis, P., Mount Stromlo Observatory, Research School of Astronomy and Astrophysics, The Australian National Universityen_AU
local.contributor.authoremailPaul.Francis@anu.edu.auen_AU
local.contributor.authoruidu9710753en_AU
local.description.notesNOAO Proposal ID 2006A-0427en_AU
local.identifier.uidSubmittedByu1005913en_AU
local.type.statusPublished Versionen_AU

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