activity
20022026
most citedLow-Mass Relics of Early Star Formation

250 citations · 1.8k across the 31 of their papers we have counts for

collaborators

32 papers

astro-ph.GA2026★ 1 cited

Multiphase images of a powerful supernova-driven wind in the early Universe

Rebecca L. Davies, D. B. Fisher, R. Herrera-Camus +38

Galactic winds are considered a likely driver of rapid quenching in early massive galaxies, but until now there has been no direct evidence that such systems drive winds powerful e…

hep-ex2026

Testing Heavy Dark Matter Decay as the Origin of KM3-230213A

KM3NeT Collaboration, O. Adriani, J. A. Aguilar +287

This work explores the hypothesis that the ultra-high-energy neutrino event KM3-230213A originates from the decay of a heavy dark matter particle with a mass above PeV scale. The a…

astro-ph.GA2026

Possible evidence for a pair-instability supernova nature of ultra-early JWST sources

Andrea Ferrara, Stefano Carniani, Takahiro Morishita +1

Recent JWST observations have revealed a population of unexpectedly bright sources at ultra-high redshift (), challenging current models of early galaxy formation. One extr…

astro-ph.CO2022★ 33 cited

Cosmic radiation backgrounds from primordial black holes

Francesco Ziparo, Simona Gallerani, Andrea Ferrara +1

Recent measurements of the cosmic X-ray and radio backgrounds (CXB/CRB, respectively) obtained with Chandra and ARCADE2 report signals in excess of those expected from known source…

astro-ph.GA2019★ 38 cited

Lyα emission from galaxies in the Epoch of Reionization

Christoph Behrens, Andrea Pallottini, Andrea Ferrara +2

The intrinsic strength of the Ly line in young, star-forming systems makes it a special tool for studying high-redshift galaxies. However, interpreting observations remains chal…

astro-ph.GA2016★ 41 cited

On the Formation of Molecular Clumps in QSO Outflows

Andrea Ferrara, Evan Scannapieco

We study the origin of the cold molecular clumps in quasar outflows, recently detected in CO and HCN emission. We first describe the physical properties of such radiation-driven ou…