An array of large observational programs using ground-based and space-borne telescopes
is planned in the next decade. The forthcoming wide-field sky surveys are expected to …

Modern radio telescopes will generate, on a daily basis, data sets on the scale of exabytes
for systems like the Square Kilometre Array (SKA). Massive data sets are a source of …

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 …

Imaging the cosmic 21 cm signal will map out the first billion years of our Universe. The
resulting 3D lightcone (LC) will encode the properties of the unseen first galaxies and …

Detecting the cosmic 21-cm signal during the Epoch of Reionization and Cosmic Dawn will
reveal insights into the properties of the first galaxies and advance cosmological parameter …

The 21-cm power spectrum of reionization is a promising probe for cosmology and
fundamental physics. Exploiting this new observable, however, requires fast predictors …

Enlightening our understanding of the first galaxies responsible for driving reionization
requires detecting the 21-cm signal from neutral hydrogen. Interpreting the wealth of …

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 …

The presence of dust in spiral galaxies affects the ability of photometric decompositions to
retrieve the parameters of their main structural components. For galaxies in an edge-on …

We study the topology of the network of ionized and neutral regions that characterized the
intergalactic medium during the Epoch of Reionization. Our analysis uses the formalism of …