activity
19962025
most citedGeneral physical properties of bright Fermi blazars

593 citations · 6.9k across the 112 of their papers we have counts for

collaborators

112 papers

astro-ph.HE2025★ 1 cited

NVSS J151002+570243: accretion and spin of a z > 4 Fermi detected blazar

Gabriele Alzati, Tullia Sbarrato, Gabriele Ghisellini

Active galactic nuclei formation and evolution is currently an open puzzle. Their enormous mass is not explainable via sub-Eddington accretion and the frequent presence of relativi…

astro-ph.GA2024★ 5 cited

Revealing faint compact radio jets at redshifts above 5 with very long baseline interferometry

Máté Krezinger, Giovanni Baldini, Marcello Giroletti +6

Over the past two decades, our knowledge of the high-redshift (z > 5) radio quasars has expanded, thanks to dedicated high-resolution very long baseline interferometry (VLBI) obser…

astro-ph.HE2020★ 17 cited

The best place and time to live in the Milky Way

R. Spinelli, G. Ghirlanda, F. Haardt +2

Counted among the most powerful cosmic events, supernovae (SNe) and gamma-ray bursts (GRBs) can be highly disruptive for life: Their radiation can be harmful for biota or induce ex…

astro-ph.HE2018★ 28 cited

X-ray absorption towards high-redshift sources: probing the intergalactic medium with blazars

R. Arcodia, S. Campana, R. Salvaterra +1

The role played by the intergalactic medium (IGM) in the X-ray absorption towards high-redshift sources has recently drawn more attention in spectral analysis studies. Here, we stu…

astro-ph.HE2017★ 86 cited

Consistency with synchrotron emission in the bright GRB 160625B observed by Fermi

M. E. Ravasio, G. Oganesyan, G. Ghirlanda +4

We present time resolved spectral analysis of prompt emission from GRB 160625B, one of the brightest bursts ever detected by Fermi in its nine years of operations. Standard empiric…

astro-ph.HE2017★ 6 cited

Bulk Comptonization: new hints from the luminous blazar 4C+25.05

E. S. Kammoun, E. Nardini, G. Risaliti +3

Blazars are often characterized by a spectral break at soft X-rays, whose origin is still debated. While most sources show a flattening, some exhibit a blackbody-like soft excess w…