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タイトルA Lyman Break Galaxy in the Epoch of Reionization from Hubble Space Telescope (HST) Grism Spectroscopy
本文(外部サイト)http://hdl.handle.net/2060/20130014397
著者(英)Haiman, Zoltan; Rhoads, James E.; Gronwall, Caryl; Hathi, Nimish; Ferreras, Ignacio; Gardner, Jonathan P.; Grogin, Norman; Meurer, Gernhardt; Budavari, Tamas; Stern, Daniel K.; Cohen, Seth; Koekemoer, Anton; Spinrad, Hyron; Pirzkal, Norbert; Dey, Arjun; Reddy, Naveen; Dickinson, Mark; Straughn, Amber N.; Malhotra, Sangeeta; Peth, Michael A.
著者所属(英)NASA Goddard Space Flight Center
発行日2013-03-22
言語eng
内容記述Slitless grism spectroscopy from space offers dramatic advantages for studying high redshift galaxies: high spatial resolution to match the compact sizes of the targets, a dark and uniform sky background, and simultaneous observation over fields ranging from five square arcminutes (HST) to over 1000 square arcminutes (Euclid). Here we present observations of a galaxy at z = 6.57 the end of the reioinization epoch identified using slitless HST grism spectra from the PEARS survey (Probing Evolution And Reionization Spectroscopically) and reconfirmed with Keck + DEIMOS. This high redshift identification is enabled by the depth of the PEARS survey. Substantially higher redshifts are precluded for PEARS data by the declining sensitivity of the ACS grism at greater than lambda 0.95 micrometers. Spectra of Lyman breaks at yet higher redshifts will be possible using comparably deep observations with IR-sensitive grisms.
NASA分類Astrophysics
レポートNOGSFC-E-DAA-TN8215
権利Copyright, Distribution as joint owner in the copyright


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