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Impact of the [C II]_158 μm luminosity scatter on the line-intensity mapping power spectrum from the EoR
[article]
2021
arXiv
pre-print
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., the power spectrum of the LIM signal to be detectable by these experiments, which will help us understand the large-scale distribution and astrophysical properties of the [C II]_158 μm line emitters ...
which arises from various ongoing astrophysical processes under varied environments inside individual galaxies, from a hydrodynamic and radiative transfer simulation of galaxies, to interpret its impact on ...
F., et al., 2020, Journal of Low Temperature Physics, 199, 898 ference on Intelligent Data Understanding (CIDU). pp 47 –54,
Crites A. T., et al., 2014, in Holland W. ...
arXiv:2110.10687v2
fatcat:h4g2ne7vqbfwxog2lcwmlrivm4
The Atacama Cosmology Telescope: dynamical masses for 44 SZ-selected galaxy clusters over 755 square degrees
2016
Monthly notices of the Royal Astronomical Society
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2015 pre-print arXiv:1512.00910v1 fatcat:rfcd3jtulraojh3csezi5bvztaOther Versions
., 2012, Proceedings of Conference on Intelligent Data Understanding (CIDU), 47 van Dokkum, P. G., 2001, PASP, 113, 1420 Vikhlinin, A., Burenin, R. ...
The Bolshoi and MultiDark simulations were run on the NASA's Pleiades supercomputer at the NASA Ames Research Center. ...
doi:10.1093/mnras/stw1284
fatcat:zber2oum5fbaldwofarzx2mpue
Nadir Shah
1935
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When describing important events, I have endeavoured to draw my facts from more than one source; in fact, I have, throughout, sought to coordinate the Iranian and other authorities available. ...
Nadir went on to say that, after the cIdu! ...
is is proof of his sound understanding of the
situation. ...
doi:10.25501/soas.00033980
fatcat:u3x2im6obzcjxiumshrv2hnwka