Identification of the brightest Lyα emitters at z = 6.6: implications for the evolution of the luminosity function in the reionization era
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Forming supermassive black hole seeds under the influence of a nearby anisotropic multifrequency source.The MUSE Hubble Ultra Deep Field Survey VI. The faint-end of the Lyα luminosity function at 2.91 < z < 6.64 and implications for reionisationOn the Formation of the First QuasarsDetecting direct collapse black holes: making the case for CR7Lyman continuum escape fraction of faint galaxies at z ~ 3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBC
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Identification of the brightest Lyα emitters at z = 6.6: implications for the evolution of the luminosity function in the reionization era
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im Mai 2015 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована в травні 2015
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name
Identification of the brightes ...... nction in the reionization era
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Identification of the brightes ...... nction in the reionization era
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type
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Identification of the brightes ...... nction in the reionization era
@en
Identification of the brightes ...... nction in the reionization era
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prefLabel
Identification of the brightes ...... nction in the reionization era
@en
Identification of the brightes ...... nction in the reionization era
@nl
P2093
P2860
P356
P1476
Identification of the brightes ...... nction in the reionization era
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P2093
Bahram Mobasher
Behnam Darvish
Huub Röttgering
Jorryt Matthee
Sérgio Santos
P2860
P304
P356
10.1093/MNRAS/STV947
P407
P50
P577
2015-05-27T00:00:00Z
P818
1502.07355
P819
2015MNRAS.451..400M