about
sameAs
The MUSE Hubble Ultra Deep Field Survey I. Survey description, data reduction, and source detectionThe MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxiesThe MUSE Hubble Ultra Deep Field Survey. VIII. Extended Lyman-{alpha} haloes around high-z star-forming galaxiesNearly all the sky is covered by Lyman-α emission around high-redshift galaxiesGreat Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV luminosity functions at z ∼ 4–7 derived with the half-million dropouts on the 100 deg2 sky†Stacking the Cosmic Web in fluorescent Ly α emission with MUSE
P50
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P50
description
Iraani astronoom
@et
Iranian astronomer
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Iranian astronomer
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Iranian astronomer
@en-gb
astronom iranian
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astronom iranian
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astronome iranien
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astronomo irandarra
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astronomo iraniano
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astrònom iranià
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name
Mohammad Akhlaghi
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Mohammad Akhlaghi
@en
Mohammad Akhlaghi
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Mohammad Akhlaghi
@fr
Mohammad Akhlaghi
@nl
Mohammad Akhlaghi
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type
label
Mohammad Akhlaghi
@ast
Mohammad Akhlaghi
@en
Mohammad Akhlaghi
@es
Mohammad Akhlaghi
@fr
Mohammad Akhlaghi
@nl
Mohammad Akhlaghi
@sq
prefLabel
Mohammad Akhlaghi
@ast
Mohammad Akhlaghi
@en
Mohammad Akhlaghi
@es
Mohammad Akhlaghi
@fr
Mohammad Akhlaghi
@nl
Mohammad Akhlaghi
@sq
P39
P551
P106
P21
P27
P31
P4594
akhlaghi_m_1
P496
0000-0003-1710-6613