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

  • Elizabeth R. Stanway*
  • , Karl Glazebrook
  • , Andrew J. Bunker
  • , Roberto G. Abraham
  • , Isobel Hook
  • , James Rhoads
  • , Patrick J. McCarthy
  • , Brian Boyle
  • , Matthew Colless
  • , David Crampton
  • , Warrick Couch
  • , Inger Jørgensen
  • , Sangeeta Malhotra
  • , Rick Murowinski
  • , Kathy Roth
  • , Sandra Savaglio
  • , Zlatan Tsvetanov
  • *Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

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.

Original languageEnglish
Pages (from-to)L13-L16
JournalAstrophysical Journal
Volume604
Issue number1 II
DOIs
Publication statusPublished - 20 Mar 2004
Externally publishedYes

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