A massive protocluster of galaxies at a redshift of z ≈ 5.3.
about
A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34.Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission.A millimetre-wave redshift search for the unlensed HyLIRG, HS1700.850.1The environments of Ly α blobs – I. Wide-field Ly α imaging of TN J1338−1942, a powerful radio galaxy at z ≃ 4.1 associated with a giant Ly α nebula★An extendedHerscheldrop-out source in the center of AS1063: a normal dusty galaxy atz= 6.1 or SZ substructures?AzTEC half square degree survey of the SHADES fields - II. Identifications, redshifts and evidence for large-scale structureThe most luminous quasars do not live in the most massive dark matter haloes at any redshiftEnhanced [CII] emission in az = 4.76 submillimetre galaxyPlanck intermediate results XXVII. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel-SPIREPlanck intermediate results XXXIX. The Planck list of high-redshift source candidatesTracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICAVIMOS Ultra-Deep Survey (VUDS): Witnessing the assembly of a massive cluster atz~ 3.3Discovery of a rich proto-cluster atz= 2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)Physical properties ofz> 4 submillimeter galaxies in the COSMOS field(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. II. The spatial extent of the radio-emitting regionsDust and gas in luminous proto-cluster galaxies at z = 4.05: the case for different cosmic dust evolution in normal and starburst galaxiesThe intense starburst HDF 850.1 in a galaxy overdensity at z ≈ 5.2 in the Hubble Deep Field(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxiesMillimeter imaging of submillimeter galaxies in the COSMOS field: redshift distributionThe source counts of submillimetre galaxies detected at λ= 1.1 mmGalaxy clusters and groups in the ALHAMBRA surveyA massive, quiescent galaxy at a redshift of 3.717The ALMA Redshift 4 Survey (AR4S)
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P2860
A massive protocluster of galaxies at a redshift of z ≈ 5.3.
description
2011 nî lūn-bûn
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2011年の論文
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2011年学术文章
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2011年学术文章
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2011年学术文章
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2011年学术文章
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name
A massive protocluster of galaxies at a redshift of z ≈ 5.3.
@en
A massive protocluster of galaxies at a redshift of z ≈ 5.3.
@nl
type
label
A massive protocluster of galaxies at a redshift of z ≈ 5.3.
@en
A massive protocluster of galaxies at a redshift of z ≈ 5.3.
@nl
prefLabel
A massive protocluster of galaxies at a redshift of z ≈ 5.3.
@en
A massive protocluster of galaxies at a redshift of z ≈ 5.3.
@nl
P2093
P2860
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A massive protocluster of galaxies at a redshift of z ≈ 5.3.
@en
P2093
Alexander Karim
Bahram Mobasher
Brant Robertson
Chris Carilli
Grant W Wilson
Johannes G Staguhn
Nick Z Scoville
Roberto Neri
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P2888
P304
P356
10.1038/NATURE09681
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P50
P577
2011-01-12T00:00:00Z
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P6179
1001540905
P698
P818
P819
2011Natur.470..233C