Current best limits on the 21-cm signal during reionization are provided at large scales ($\gtrsim$100 Mpc). To model these scales, enormous simulation volumes are required which are computationally expensive. We find that the primary source of uncertainty at these large scales is sample variance, which decides the minimum size of simulations required to analyse current and upcoming observations. In large-scale structure simulations, the method of `fixing' the initial conditions (ICs) to exactly follow the initial power spectrum and `pairing' two simulations with exactly out-of-phase ICs has been shown to significantly reduce sample variance. Here we apply this `fixing and pairing' (F\&P) approach to reionization simulations whose clusterin...
Upper limits from the current generation of interferometers targeting the 21-cm signal from high red...
We apply Bayesian statistics to perform model selection on different reionization scenarios via the ...
abstract: One of the most fundamental questions in astronomy is how the Universe evolved to become t...
Current best limits on the 21 cm signal during reionization are provided at large scales (≳100 Mpc)....
The optical depth $\tau$ is the least well determined parameter in the standard model of cosmology, ...
The 21-cm probability distribution function (PDF; i.e. distribution of pixel brightness temperatures...
Weintroduce 21CMMC: a parallelized, Monte Carlo Markov Chain analysis tool, incorporating the epoch ...
In the coming decade, low-frequency radio arrays will begin to probe the epoch of reionization via t...
Cosmic 21cm interferometry is set to revolutionize our understanding of the Epoch of Reionization (E...
Radio interferometric experiments aim to constrain the reionization model parameters by measuring th...
Redshifted 21-cm measurements of the structure of ionized regions that grow during reionization prom...
Cosmic Dawn (CD) and Epoch of Reionization (EoR) are epochs of the Universe which host invaluable in...
We explore the ability of measurements of the 21-cm power spectrum during reionization to enable the...
Accurate simulations of the 21-cm signal from the Epoch of Reionization require the generation of ma...
Measurement of the global 21-cm signal during Cosmic Dawn (CD) and the Epoch of Reionization (EoR) i...
Upper limits from the current generation of interferometers targeting the 21-cm signal from high red...
We apply Bayesian statistics to perform model selection on different reionization scenarios via the ...
abstract: One of the most fundamental questions in astronomy is how the Universe evolved to become t...
Current best limits on the 21 cm signal during reionization are provided at large scales (≳100 Mpc)....
The optical depth $\tau$ is the least well determined parameter in the standard model of cosmology, ...
The 21-cm probability distribution function (PDF; i.e. distribution of pixel brightness temperatures...
Weintroduce 21CMMC: a parallelized, Monte Carlo Markov Chain analysis tool, incorporating the epoch ...
In the coming decade, low-frequency radio arrays will begin to probe the epoch of reionization via t...
Cosmic 21cm interferometry is set to revolutionize our understanding of the Epoch of Reionization (E...
Radio interferometric experiments aim to constrain the reionization model parameters by measuring th...
Redshifted 21-cm measurements of the structure of ionized regions that grow during reionization prom...
Cosmic Dawn (CD) and Epoch of Reionization (EoR) are epochs of the Universe which host invaluable in...
We explore the ability of measurements of the 21-cm power spectrum during reionization to enable the...
Accurate simulations of the 21-cm signal from the Epoch of Reionization require the generation of ma...
Measurement of the global 21-cm signal during Cosmic Dawn (CD) and the Epoch of Reionization (EoR) i...
Upper limits from the current generation of interferometers targeting the 21-cm signal from high red...
We apply Bayesian statistics to perform model selection on different reionization scenarios via the ...
abstract: One of the most fundamental questions in astronomy is how the Universe evolved to become t...