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 …

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 …

Cosmic dawn (CD) and the epoch of reionization (EoR) are the most important parts of
cosmic history during which the first luminous structures emerged. These first objects heated …

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 …

In this study, we introduce beorn (Bubbles during the Epoch of Reionization Numerical
Simulator), a publicly available python code that generates three-dimensional maps of the …

The 21-cm signal from the epoch of cosmic dawn prior to reionization consists of a promising
observable to gain new insights into the dark matter (DM) sector. In this paper, we …

We present simulations of cosmic reionization and reheating from z= 18 to z= 5,
investigating the role of stars (emitting soft UV-photons), nuclear black holes (BHs, with …

During the epoch of reionization (EoR), the 21-cm signal allows direct observation of the
neutral hydrogen (H i) in the intergalactic medium (IGM). In the post-reionization era, this …

We explore the possibility of constraining model parameters of the Epoch of Reionization
(EoR) from 21cm brightness temperature maps, using a combination of morphological …

ABSTRACT The upcoming Square Kilometre Array (SKA-Low) will map the distribution of
neutral hydrogen during reionization and produce a tremendous amount of three …