activity
20012026
most citedScience with e-ASTROGAM (A space mission for MeV-GeV gamma-ray astrophysics)

253 citations · 838 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.GA2026

Milliarcsecond-resolution Radio-imaging Survey of Blazar Candidates at 4 < z < 5.4

Máté Krezinger, Alessandro Caccianiga, Daniele Dallacasa +9

We present a milliarcsecond-resolution radio survey of 17 high-redshift (4 < z < 5.4) blazar candidates observed with the European Very Long Baseline Interferometry (VLBI) Network…

astro-ph.GA2024

Obscuration in high redshift jetted QSO

A. Caccianiga, L. Ighina, A. Moretti +6

Obscuration in high-redshift quasi-stellar objects (QSO) has a profound impact on our understanding of the evolution of supermassive black holes across the cosmic time. An accurate…

astro-ph.HE2022★ 43 cited

A New Sample of Gamma-Ray Emitting Jetted Active Galactic Nuclei

Luigi Foschini, Matthew L. Lister, Heinz Andernach +11

We considered the fourth catalog of gamma-ray point sources produced by the Fermi Large Area Telescope (LAT) and selected only jetted active galactic nuclei (AGN) or sources with n…

astro-ph.HE2021★ 1 cited

A New Sample of Gamma-Ray Emitting Jetted Active Galactic Nuclei -- Preliminary Results

L. Foschini, M. L. Lister, S. Antón +8

We are compiling a new list of gamma-ray jetted active galactic nuclei (AGN), starting from the fourth catalog of point sources of the Fermi Large Area Telescope (LAT). Our aim is…

astro-ph.GA2019★ 39 cited

The space density of z>4 blazars

Alessandro Caccianiga, Alberto Moretti, Silvia Belladitta +9

High redshift blazars are an important class of Active Galactic Nuclei (AGN) that can provide an independent estimate of the supermassive black-hole mass function in high redshift…

astro-ph.IM2018★ 38 cited

Star-galaxy classification in the Dark Energy Survey Y1 dataset

I. Sevilla-Noarbe, B. Hoyle, M. J. Marchã +75

We perform a comparison of different approaches to star-galaxy classification using the broad-band photometric data from Year 1 of the Dark Energy Survey. This is done by performin…