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Three Ly Emitters at z 6: Early GMOS/Gemini Data from the GLARE Project
Author(s) -
E. R. Stanway,
Karl Glazebrook,
Andrew J. Bunker,
Roberto Abraham,
I. Hook,
James E. Rhoads,
Patrick J. McCarthy,
Brian Boyle,
Matthew Colless,
D. Crampton,
W. J. Couch,
Inger Jrgensen,
Sangeeta Malhotra,
Rick Murowinski,
Kathy Roth,
S. Savaglio,
Z. Tsvetanov
Publication year - 2004
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/383523
Subject(s) - physics , redshift , galaxy , astrophysics , hubble ultra deep field , emission spectrum , spectroscopy , astronomy , spectral line , hubble deep field
We report spectroscopic detection of three z~6 Lyman-alpha emitting galaxies,in the vicinity of the Hubble Ultra Deep Field, from the early data of theGemini Lyman-$\alpha$ at Reionisation Era (GLARE) project. Two objects,GLARE#3001 (z =5.79) and GLARE#3011 (z =5.94), are new detections and arefainter in $z'$ (z'_{AB} =26.37 and 27.15) than any Lyman break galaxypreviously detected in Lyman-alpha. A third object, GLARE#1042 (z =5.83) haspreviously been detected in line emission from the ground; we report here a newspectroscopic continuum detection. Gemini/GMOS-S spectra of these objects,obtained using nod & shuffle, are presented together with a discussion of theirphotometric properties. All three objects were selected for spectroscopy viathe i-drop Lyman Break technique, the two new detections from the GOODS v1.0imaging data. The red i'-z' colors and high equivalent widths of these objectssuggest a high-confidence z>5 Lyman-alpha identification of the emission lines.This brings the total number of known z>5 galaxies within 9 arcmin of theHubble Ultra Deep Field to four, of which three are at the same redshift (z=5.8within 2000 km/s suggesting the existence of a large-scale structure at thisredshift.Comment: 5 pages, 2 figures. Revised to match accepted versio

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