TY - JOUR
T1 - Three Lyα emitters at z ≈ 6
T2 - Early GMOS/gemini data from the GLARE project
AU - Stanway, Elizabeth R.
AU - Glazebrook, Karl
AU - Bunker, Andrew J.
AU - Abraham, Roberto G.
AU - Hook, Isobel
AU - Rhoads, James
AU - McCarthy, Patrick J.
AU - Boyle, Brian
AU - Colless, Matthew
AU - Crampton, David
AU - Couch, Warrick
AU - Jørgensen, Inger
AU - Malhotra, Sangeeta
AU - Murowinski, Rick
AU - Roth, Kathy
AU - Savaglio, Sandra
AU - Tsvetanov, Zlatan
PY - 2004/3/20
Y1 - 2004/3/20
N2 - We report spectroscopic detection of three z ∼ 6 Lyα-emitting galaxies, in the vicinity of the Hubble Ultra Deep Field, from the early data of the Gemini Lyman Alpha at Reionisation Era (GLARE) project. Two objects, GLARE 3001 (z = 5.79) and GLARE 3011 (z = 5.94), are new detections and are fainter in z′ (z′AB = 26.37 and 27.15) than any Lyman break galaxy previously detected in Lyα. A third object, GLARE 1042 (z = 5.83), has previously been detected in line emission from the ground; we report here a new spectroscopic continuum detection. Gemini/GMOS-South spectra of these objects, obtained using nod and shuffle, are presented together with a discussion of their photometric properties. All three objects were selected for spectroscopy via the i-drop Lyman break technique, the two new detections from the GOODS version 1.0 imaging data. The red i′-z′ colors and high equivalent widths of these objects suggest a high-confidence z > 5 Lyα identification of the emission lines. This brings the total number of known z > 5 galaxies within 9′ of the Hubble Ultra Deep Field to four, of which three are at the same redshift (z = 5.8 within 2000 km s-1), suggesting the existence of a large-scale structure at this redshift.
AB - We report spectroscopic detection of three z ∼ 6 Lyα-emitting galaxies, in the vicinity of the Hubble Ultra Deep Field, from the early data of the Gemini Lyman Alpha at Reionisation Era (GLARE) project. Two objects, GLARE 3001 (z = 5.79) and GLARE 3011 (z = 5.94), are new detections and are fainter in z′ (z′AB = 26.37 and 27.15) than any Lyman break galaxy previously detected in Lyα. A third object, GLARE 1042 (z = 5.83), has previously been detected in line emission from the ground; we report here a new spectroscopic continuum detection. Gemini/GMOS-South spectra of these objects, obtained using nod and shuffle, are presented together with a discussion of their photometric properties. All three objects were selected for spectroscopy via the i-drop Lyman break technique, the two new detections from the GOODS version 1.0 imaging data. The red i′-z′ colors and high equivalent widths of these objects suggest a high-confidence z > 5 Lyα identification of the emission lines. This brings the total number of known z > 5 galaxies within 9′ of the Hubble Ultra Deep Field to four, of which three are at the same redshift (z = 5.8 within 2000 km s-1), suggesting the existence of a large-scale structure at this redshift.
UR - https://www.scopus.com/pages/publications/2442502681
U2 - 10.1086/383523
DO - 10.1086/383523
M3 - Article
AN - SCOPUS:2442502681
SN - 0004-637X
VL - 604
SP - L13-L16
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1 II
ER -