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The discovery of six Ly{alpha} emitters near a radio galaxy at z {approx} 5.2

Journal Article · · Astronomy & Astrophysics
OSTI ID:15011562
The authors present the results of narrow-band and broad-band imaging with the Very Large Telescope of the field surrounding the radio galaxy TN J0924-2201 at z = 5.2. 14 candidate Ly{alpha} emitters with an observed equivalent width of at least 124 {angstrom} were detected. Spectroscopy of 8 of these objects revealed 6 having redshifts similar to that of the radio galaxy. The density of emitters near the radio galaxy is a factor 3-4 higher than in the field, and comparable to the density of Ly{alpha} emitters in the protocluster 1338-1942 at z = 4.1. The Ly{alpha} emitters near TN J0924-2201 could therefore be part of a structure that will evolve into a 10{sup 15} M{sub {circle_dot}} cluster. These observations confirm that substantial clustering of Ly{alpha} emitters occur at z > 5 and strengthen the idea that radio galaxies in the early Universe pinpoint regions of high density.
Research Organization:
Lawrence Livermore National Lab., Livermore, CA (US)
Sponsoring Organization:
US Department of Energy (US)
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
15011562
Report Number(s):
UCRL-JRNL-206783
Journal Information:
Astronomy & Astrophysics, Journal Name: Astronomy & Astrophysics Vol. 430
Country of Publication:
United States
Language:
English

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