Three Lyα emitters at z ≈ 6:: Early GMOS/Gemini data from the GLARE project

被引:102
作者
Stanway, ER
Glazebrook, K
Bunker, AJ
Abraham, RG
Hook, I
Rhoads, J
McCarthy, PJ
Boyle, B
Colless, M
Crampton, D
Couch, W
Jorgensen, I
Malhotra, S
Murowinski, R
Roth, K
Savaglio, S
Tsvetanov, Z
机构
[1] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[2] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[3] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 3H8, Canada
[4] Univ Oxford, Dept Astrophys, Nucl & Astrophys Lab, Oxford OX1 3RH, England
[5] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[6] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA
[7] Australia Telescope Natl Facil, Epping, NSW 1710, Australia
[8] Anglo Australian Observ, Epping, NSW 1710, Australia
[9] Natl Res Council Canada, Herzberg Inst Astrophys, Victoria, BC V9E 2E7, Canada
[10] Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia
[11] Gemini Observ, Hilo, HI 96720 USA
关键词
galaxies : evolution; galaxies : formation; galaxies : high-redshift; galaxies : starburst;
D O I
10.1086/383523
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report spectroscopic detection of three z similar to 6 Lyalpha-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 Lyalpha. 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 Lyalpha 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.
引用
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页码:L13 / L16
页数:4
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