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Constraining the intergalactic medium at z ≈ 9.1 using LOFAR Epoch of Reionization observations
R. Ghara
, S. K. Giri
, G. Mellema
, B. Ciardi
,
S. Zaroubi
, I. T. Iliev
, L. V.E. Koopmans
, E. Chapman
, S. Gazagnes
, B. K. Gehlot
, A. Ghosh
, V. Jelić
, F. G. Mertens
, R. Mondal
, J. Schaye
, M. B. Silva
, K. M.B. Asad
, R. Kooistra
, M. Mevius
, A. R. Offringa
V. N. Pandey, S. Yatawatta
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Physics
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Keyphrases
Intergalactic Medium
100%
Epoch of Reionization
100%
LOFAR
100%
Cosmic Microwave Background
33%
Spin Temperature
33%
Full Width at Half Maximum
33%
Radio Telescope
16%
Parameter Space
16%
Tight
16%
Power Spectrum
16%
Reionization
16%
Large Fluctuations
16%
Ionization State
16%
Thermal State
16%
Large Region
16%
Temperature Fluctuation
16%
Gas Temperature
16%
Physical State
16%
Volume Fraction
16%
Bayesian Inference Method
16%
Credible Interval
16%
Background Observation
16%
Simulation Code
16%
Gas Heating
16%
Engineering
Upper Limit
100%
Constrains
50%
Parameter Space
50%
Power Spectra
50%
Simulation Code
50%
Gas Temperature
50%
Temperature Fluctuation
50%
Physical State
50%
Physics
Reionization
100%
Intergalactic Medium
100%
LOFAR
100%
Cosmic Microwave Background
33%
Spin Temperature
33%
Radio Telescope
16%
Power Spectra
16%
Gas Temperature
16%