Modeling cosmic reionization
NY Gnedin, P Madau - Living Reviews in Computational Astrophysics, 2022 - Springer
The transformation of cold neutral intergalactic hydrogen into a highly ionized warm plasma
marks the end of the cosmic dark ages and the beginning of the age of galaxies. The details …
marks the end of the cosmic dark ages and the beginning of the age of galaxies. The details …
Improved upper limits on the 21 cm signal power spectrum of neutral hydrogen at z ≈ 9.1 from LOFAR
ABSTRACT A new upper limit on the 21 cm signal power spectrum at a redshift of z≈ 9.1 is
presented, based on 141 h of data obtained with the Low-Frequency Array (LOFAR). The …
presented, based on 141 h of data obtained with the Low-Frequency Array (LOFAR). The …
HERA phase I limits on the cosmic 21 cm signal: constraints on astrophysics and cosmology during the epoch of reionization
Z Abdurashidova, JE Aguirre, P Alexander… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract Recently, the Hydrogen Epoch of Reionization Array (HERA) has produced the
experiment's first upper limits on the power spectrum of 21 cm fluctuations at z∼ 8 and 10 …
experiment's first upper limits on the power spectrum of 21 cm fluctuations at z∼ 8 and 10 …
Inferring the astrophysics of reionization and cosmic dawn from galaxy luminosity functions and the 21-cm signal
J Park, A Mesinger, B Greig… - Monthly Notices of the …, 2019 - academic.oup.com
The properties of the first galaxies, expected to drive the Cosmic Dawn and the Epoch of
Reionization, are encoded in the 3D structure of the cosmic 21-cm signal. Parameter …
Reionization, are encoded in the 3D structure of the cosmic 21-cm signal. Parameter …
Studying cosmic dawn using redshifted HI 21-cm signal: A brief review
In this review article, we briefly outline our current understanding of the physics associated
with the HI 21-cm signal from cosmic dawn. We discuss different phases of cosmic dawn as …
with the HI 21-cm signal from cosmic dawn. We discuss different phases of cosmic dawn as …
Constraining the intergalactic medium at z ≈ 9.1 using LOFAR Epoch of Reionization observations
We derive constraints on the thermal and ionization states of the intergalactic medium (IGM)
at redshift≈ 9.1 using new upper limits on the 21-cm power spectrum measured by the …
at redshift≈ 9.1 using new upper limits on the 21-cm power spectrum measured by the …
An effective model for the cosmic-dawn 21-cm signal
JB Muñoz - Monthly Notices of the Royal Astronomical Society, 2023 - academic.oup.com
The 21-cm signal holds the key to understanding the first structure formation during cosmic
dawn. Theoretical progress over the last decade has focused on simulations of this signal …
dawn. Theoretical progress over the last decade has focused on simulations of this signal …
Constraining the state of the intergalactic medium during the Epoch of Reionization using MWA 21-cm signal observations
ABSTRACT The Murchison Widefield Array (MWA) team has derived new upper limits on the
spherically averaged power spectrum of the 21-cm signal at six redshifts in the range z≈ 6.5 …
spherically averaged power spectrum of the 21-cm signal at six redshifts in the range z≈ 6.5 …
Emulating simulations of cosmic dawn for 21 cm power spectrum constraints on cosmology, reionization, and x-ray heating
Current and upcoming radio interferometric experiments are aiming to make a statistical
characterization of the high-redshift 21 cm fluctuation signal spanning the hydrogen …
characterization of the high-redshift 21 cm fluctuation signal spanning the hydrogen …
Constraining the X-ray heating and reionization using 21-cm power spectra with Marginal Neural Ratio Estimation
ABSTRACT Cosmic Dawn (CD) and Epoch of Reionization (EoR) are epochs of the
Universe which host invaluable information about the cosmology and astrophysics of X-ray …
Universe which host invaluable information about the cosmology and astrophysics of X-ray …