A large population of 'Lyman-break' galaxies in a protocluster at redshift z approximately 4.1.
The most massive galaxies and the richest clusters are believed to have emerged from regions with the largest enhancements of mass density relative to the surrounding space. Distant radio galaxies may pinpoint the locations of the ancestors of rich clusters, because they are massive systems associated with 'overdensities' of galaxies that are bright in the Lyman-alpha line of hydrogen. A powerful technique for detecting high-redshift galaxies is to search for the characteristic 'Lyman break' feature in the galaxy colour, at wavelengths just shortwards of Lyalpha, which is due to absorption of radiation from the galaxy by the intervening intergalactic medium. Here we report multicolour imaging of the most distant candidate protocluster, TN J1338-1942 at a redshift z approximately 4.1. We find a large number of objects with the characteristic colours of galaxies at that redshift, and we show that this excess is concentrated around the targeted dominant radio galaxy. Our data therefore indicate that TN J1338-1942 is indeed the most distant cluster progenitor of a rich local cluster, and that galaxy clusters began forming when the Universe was only ten per cent of its present age.
Miley
George K
GK
Leiden Observatory, University of Leiden, PO Box 9513, Leiden, 2300 RA, The Netherlands. miley@strw.leidenuniv.nl
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Roderik A
RA
Tsvetanov
Zlatan I
ZI
Bouwens
Rychard J
RJ
Benítez
Narciso
N
Blakeslee
John P
JP
Ford
Holland C
HC
Illingworth
Garth D
GD
Postman
Marc
M
Rosati
Piero
P
Clampin
Mark
M
Hartig
George F
GF
Zirm
Andrew W
AW
Röttgering
Huub J A
HJ
Venemans
Bram P
BP
Ardila
David R
DR
Bartko
Frank
F
Broadhurst
Tom J
TJ
Brown
Robert A
RA
Burrows
Chris J
CJ
Cheng
E S
ES
Cross
Nicholas J G
NJ
De Breuck
Carlos
C
Feldman
Paul D
PD
Franx
Marijn
M
Golimowski
David A
DA
Gronwall
Caryl
C
Infante
Leopoldo
L
Martel
André R
AR
Menanteau
Felipe
F
Meurer
Gerhardt R
GR
Sirianni
Marco
M
Kimble
Randy A
RA
Krist
John E
JE
Sparks
William B
WB
Tran
Hien D
HD
White
Richard L
RL
Zheng
Wei
W