ABSTRACT The Experiment to Detect the Global Epoch of Reionization Signature (EDGES)
recently reported a strong 21-cm absorption signal relative to the cosmic microwave …

Using the global 21-cm signal measurement by the EDGES collaboration, we derive
constraints on the fraction of the dark matter that is in the form of primordial black holes …

Cosmic Dawn (CD), when the first stars and proto-galaxies began to form, is commonly
expected to be accompanied by an absorption signature at radio frequencies. This feature …

We investigate the nebular emission produced by young stellar populations using the new
galsevn model based on the combination of the sevn population-synthesis code including …

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 …

Any particle dark matter (DM) scenario featuring a suppressed power spectrum of
astrophysical relevance results in a delay of galaxy formation. As a consequence, such …

The birth of the first luminous sources and the ensuing epoch of reionization are best studied
via the redshifted 21-cm emission line, the signature of the first two imprinting the last. In this …

The distribution of matter fluctuations in our universe is key for understanding the nature of
dark matter and the physics of the early cosmos. Different observables have been able to …

Observations of the 21-cm line from primordial hydrogen promise to be one of the best tools
to study the early epochs of the Universe: the dark ages, the cosmic dawn and the …

We build a new model for the global 21-cm signal that is calibrated to measurements of the
high-z galaxy luminosity function (LF) and further tuned to match the Thomson scattering …