papers

Publications (64)

astro-ph.HE2023

Prospects for -ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array

The Cherenkov Telescope Array Consortium, :, K. Abe +564

Galaxy clusters are expected to be dark matter (DM) reservoirs and storage rooms for the cosmic-ray protons (CRp) that accumulate along the cluster's formation history. Accordingly…

astro-ph.IM2015

Cherenkov Telescope Array Data Management

G. Lamanna, L. A. Antonelli, J. L. Contreras +37

Very High Energy gamma-ray astronomy with the Cherenkov Telescope Array (CTA) is evolving towards the model of a public observatory. Handling, processing and archiving the large am…

astro-ph.HE2021

Multi-messenger and transient astrophysics with the Cherenkov Telescope Array

Ž. Bošnjak, A. M. Brown, A. Carosi +142

The discovery of gravitational waves, high-energy neutrinos or the very-high-energy counterpart of gamma-ray bursts has revolutionized the high-energy and transient astrophysics co…

astro-ph.IM2025

The Real-Time Data Processor Framework for Data Handling and Analysis of High-Energy Instruments

A. Bulgarelli, N. Parmiggiani, L. Castaldini +5

We implemented a real-time data processor (rta-dp) framework that can be used to develop real-time analysis pipelines and data handling systems to manage high-throughput data strea…

astro-ph.IM2018

Science with the Cherenkov Telescope Array

The Cherenkov Telescope Array Consortium, :, B. S. Acharya +580

The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. The scientific potential of CTA i…

astro-ph.IM2023

The RTApipe framework for the gamma-ray real-time analysis software development

N. Parmiggiani, A. Bulgarelli, D. Beneventano +7

In the multi-messenger era, coordinating observations between astronomical facilities is mandatory to study transient phenomena (e.g. Gamma-ray bursts) and is achieved by sharing i…

astro-ph.HE2021

A Deep Learning Method for AGILE-GRID GRB Detection

N. Parmiggiani, A. Bulgarelli, V. Fioretti +7

The follow-up of external science alerts received from Gamma-Ray Bursts (GRB) and Gravitational Waves (GW) detectors is one of the AGILE Team's current major activities. The AGILE…

astro-ph.IM2015

A magnetic diverter for charged particle background rejection in the SIMBOL-X telescope

D. Spiga, V. Fioretti, A. Bulgarelli +6

Minimization of charged particle background in X-ray telescopes is a well known issue. Charged particles (chiefly protons and electrons) naturally present in the cosmic environment…

astro-ph.HE2018

The e-ASTROGAM gamma-ray space observatory for the multimessenger astronomy of the 2030s

V. Tatischeff, A. De Angelis, M. Tavani +74

e-ASTROGAM is a concept for a breakthrough observatory space mission carrying a gamma-ray telescope dedicated to the study of the non-thermal Universe in the photon energy range fr…

astro-ph.HE2015

On the Angular Resolution of the AGILE gamma-ray imaging detector

S. Sabatini, I. Donnarumma, M. Tavani +16

We present a study of the Angular Resolution of the AGILE gamma-ray imaging detector (GRID) that is operational in space since April 2007. The AGILE instrument is made of an array…

astro-ph.IM2018

Calibration of AGILE-GRID with on-ground data and Monte Carlo simulations

P. W. Cattaneo, A. Rappoldi, A. Argan +41

AGILE is a mission of the Italian Space Agency (ASI) Scientific Program dedicated to gamma-ray astrophysics, operating in a low Earth orbit since April 23, 2007. It is designed to…

astro-ph.HE2018

Science with e-ASTROGAM (A space mission for MeV-GeV gamma-ray astrophysics)

A. De Angelis, V. Tatischeff, I. A. Grenier +248

e-ASTROGAM (enhanced ASTROGAM) is a breakthrough Observatory space mission, with a detector composed by a Silicon tracker, a calorimeter, and an anticoincidence system, dedicated t…

astro-ph.HE2020

Gamma-Ray and X-Ray Observations of the Periodic-Repeater FRB 180916 During Active Phases

M. Tavani, F. Verrecchia, C. Casentini +33

FRB 180916 is a most intriguing source at 150 Mpc distance capable of producing repeating fast radio bursts with a periodic 16.35 day temporal pattern. We report on the X-ray and $…

astro-ph.IM2021

The AGILE real-time analysis pipelines in the multi-messenger era

N. Parmiggiani, A. Bulgarelli, A. Ursi +9

In the multi-messenger era, space and ground-based observatories usually develop real-time analysis (RTA) pipelines to rapidly detect transient events and promptly share informatio…

astro-ph.IM2020

AGILESim: Monte Carlo simulation of the AGILE gamma-ray telescope

V. Fioretti, A. Bulgarelli, M. Tavani +12

The accuracy of Monte Carlo simulations in reproducing the scientific performance of space telescopes (e.g. angular resolution) is mandatory for a correct design of the mission. A…

astro-ph.HE2022

Extragalactic Observatory Science with the ASTRI Mini-Array at the Observatorio del Teide

F. G. Saturni, C. H. E. Arcaro, B. Balmaverde +47

The ASTRI Mini-Array is a next-generation system of nine imaging atmospheric Cherenkov telescopes that is going to be built at the Observatorio del Teide site. After a first phase,…

astro-ph.IM2023

Preliminary Results of a Deep Learning Anomaly Detection Method to Identify Gamma-Ray Bursts in the AGILE Anticoincidence System

N. Parmiggiani, A. Bulgarelli, A. Ursi +7

AGILE is a space mission launched in 2007 to study X-ray and gamma-ray astronomy. The AGILE team developed real-time analysis pipelines to detect transient phenomena such as Gamma-…

astro-ph.IM2025

The New Architecture of the Online Observation Quality System for the ASTRI Mini-Array Project

N. Parmiggiani, A. Bulgarelli, L. Castaldini +23

The ASTRI Mini-Array is an international collaboration led by the Italian National Institute for Astrophysics. The project aims to construct and operate an array of nine Imaging At…

astro-ph.IM2013

The Real-Time Analysis of the Cherenkov Telescope Array Observatory

A. Bulgarelli, V. Fioretti, J. L. Contreras +31

The Cherenkov Telescope Array (CTA) Observatory must be capable of issuing fast alerts on variable and transient sources to maximize the scientific return. This will be accomplishe…

astro-ph.IM2013

Calibration of AGILE-GRID with In-Flight Data and Monte Carlo Simulations

Andrew W. Chen, A. Argan, A. Bulgarelli +57

Context: AGILE is a gamma-ray astrophysics mission which has been in orbit since 23 April 2007 and continues to operate reliably. The gamma-ray detector, AGILE-GRID, has observed G…

astro-ph.HE2017

Prospects for CTA observations of the young SNR RX J1713.7-3946

The CTA Consortium, :, F. Acero +381

We perform simulations for future Cherenkov Telescope Array (CTA) observations of RX~J1713.73946, a young supernova remnant (SNR) and one of the brightest sources ever discovere…

astro-ph.IM2024

The Online Observation Quality System Implementation for the ASTRI Mini-Array Project

L. Castaldini, N. Parmiggiani, A. Bulgarelli +20

The ASTRI Mini-Array project, led by the Italian National Institute for Astrophysics, aims to construct and operate nine Imaging Atmospheric Cherenkov Telescopes for high-energy ga…

astro-ph.HE2017

Cherenkov Telescope Array Contributions to the 35th International Cosmic Ray Conference (ICRC2017)

F. Acero, B. S. Acharya, V. Acín Portella +1137

List of contributions from the Cherenkov Telescope Array Consortium presented at the 35th International Cosmic Ray Conference, July 12-20 2017, Busan, Korea.

astro-ph.IM2015

Study of the Gamma-ray performance of the GAMMA-400 Calorimeter

P. Cumani, A. M. Galper, V. Bonvicini +73

GAMMA-400 is a new space mission, designed as a dual experiment, capable to study both high energy gamma rays (from 100 MeV to few TeV) and cosmic rays (electrons up to 20 Te…

astro-ph.IM2020

First detection of the Crab Nebula at TeV energies with a Cherenkov telescope in a dual-mirror Schwarzschild-Couder configuration: the ASTRI-Horn telescope

S. Lombardi, O. Catalano, S. Scuderi +89

We report on the first detection of very high-energy (VHE) gamma-ray emission from the Crab Nebula by a Cherenkov telescope in dual-mirror Schwarzschild-Couder (SC) configuration.…

astro-ph.HE2024

AGILE gamma-ray detection of the exceptional GRB 221009A

M. Tavani, G. Piano, A. Bulgarelli +47

Gamma-ray emission in the MeV-GeV range from explosive cosmic events is of invaluable relevance to understanding physical processes related to the formation of neutron stars and bl…

astro-ph.IM2018

Simulating Modulated X-ray calibration Sources for future X-ray missions, using GEANT4

C. P. de Vries, V. Fioretti, J. W. den Herder +2

The XIFU X-ray spectrometer instrument on the future Athena mission needs X-ray calibration sources to calibrate the gains of the individual detector pixels. For this purpose, elec…

astro-ph.HE2022

Galactic Observatory Science with the ASTRI Mini-Array at the Observatorio del Teide

A. D'Aì, E. Amato, A. Burtovoi +52

The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Mini-Array will be composed of nine imaging atmospheric Cherenkov telescopes at the Observatorio del Teide site…

astro-ph.IM2021

The Online Observation Quality System for the ASTRI Mini-Array

N. Parmiggiani, A. Bulgarelli, L. Baroncelli +18

The ASTRI Mini-Array is an international collaboration led by the Italian National Institute for Astrophysics (INAF), aiming to construct and operate an array of nine Imaging Atmos…

astro-ph.HE2021

AGILE Observations of Fast Radio Bursts

F. Verrecchia, C. Casentini, M. Tavani +22

We report on a systematic search for hard X-ray and gamma-ray emission in coincidence with fast radio bursts (FRBs) observed by the AGILE satellite. We used 13 years of AGILE archi…

astro-ph.HE2017

AGILE Observations of the Gravitational-wave Source GW170817: Constraining Gamma-Ray Emission from a NS-NS Coalescence

F. Verrecchia, M. Tavani, I. Donnarumma +39

The LIGO-Virgo Collaboration (LVC) detected, on 2017 August 17, an exceptional gravitational-wave (GW) event temporally consistent within with the GRB 1708117A…

astro-ph.HE2026

Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies

S. Abe, J. Abhir, A. Abhishek +457

The detection of gravitational waves (GWs) from a binary neutron star (BNS) merger by Advanced LIGO and Advanced Virgo (GW170817), together with its electromagnetic counterpart, th…

astro-ph.HE2017

AGILE Observations of the Gravitational Wave Source GW170104

F. Verrecchia, M. Tavani, A. Ursi +36

The LIGO/Virgo Collaboration (LVC) detected on 2017 January 4, a significant gravitational-wave (GW) event (now named GW170104). We report in this Letter the main results obtained…

astro-ph.IM2026

The Array Control and Data Acquisition software of the Cherenkov Telescope Array Observatory

I. Oya, B. López, P. Aubert +61

The Cherenkov Telescope Array Observatory (CTAO) aims to advance knowledge of the gamma-ray sky as the largest gamma-ray observatory ever built. The CTAO will be deployed at two si…

astro-ph.HE2018

AGILE detection of gamma-ray sources coincident with cosmic neutrino events

F. Lucarelli, M. Tavani, G. Piano +34

The origin of cosmic neutrinos is still largely unknown. Using data obtained by the gamma-ray imager on board of the AGILE satellite, we systematically searched for transient gamma…

astro-ph.HE2025

Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array Observatory

K. Abe, S. Abe, J. Abhir +491

The dwarf spheroidal galaxies (dSphs) orbiting the Milky Way are widely regarded as systems supported by velocity dispersion against self-gravity, and as prime targets for the sear…

astro-ph.HE2020

An X-Ray Burst from a Magnetar Enlightening the Mechanism of Fast Radio Bursts

M. Tavani, C. Casentini, A. Ursi +60

Fast radio bursts (FRBs) are short (millisecond) radio pulses originating from enigmatic sources at extragalactic distances so far lacking a detection in other energy bands. Magnet…

astro-ph.HE2015

CTA Contributions to the 34th International Cosmic Ray Conference (ICRC2015)

The CTA Consortium, :, A. Abchiche +1305

List of contributions from the CTA Consortium presented at the 34th International Cosmic Ray Conference, 30 July - 6 August 2015, The Hague, The Netherlands.

astro-ph.HE2013

X-ray view of four high-luminosity Swift/BAT AGN: Unveiling obscuration and reflection with Suzaku

V. Fioretti, L. Angelini, R. F. Mushotzky +2

The Swift/BAT nine-month survey observed 153 AGN, all with ultra-hard X-ray BAT fluxes in excess of 10^-11 erg cm^-2 s^-1 and an average redshift of 0.03. Among them, four of the m…

astro-ph.IM2021

Agilepy: A Python framework for scientific analysis of AGILE data

A. Bulgarelli, L. Baroncelli, A. Addis +8

The Italian AGILE space mission, with its Gamma-Ray Imaging Detector (GRID) instrument sensitive in the 30 MeV-50 GeV gamma-ray energy band, has been operating since 2007. Agilepy…

astro-ph.IM2021

The Science Alert Generation system of the Cherenkov Telescope Array Observatory

A. Bulgarelli, S. Caroff, A. Addis +11

The Cherenkov Telescope Array (CTA) Observatory, with dozens of telescopes located in both the Northern and Southern Hemispheres, will be the largest ground-based gamma-ray observa…

astro-ph.HE2019

All-Sky-ASTROGAM: The MeV Gamma-Ray Companion to Multimessenger Astronomy

V. Tatischeff, A. De Angelis, M. Tavani +33

All-Sky-ASTROGAM is a gamma-ray observatory operating in a broad energy range, 100 keV to a few hundred MeV, recently proposed as the "Fast" (F) mission of the European Space Agenc…

astro-ph.HE2021

Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

The Cherenkov Telescope Array Consortium, :, A. Acharyya +449

We provide an updated assessment of the power of the Cherenkov Telescope Array (CTA) to search for thermally produced dark matter at the TeV scale, via the associated gamma-ray sig…

astro-ph.IM2017

The e-ASTROGAM gamma-ray space mission

V. Tatischeff, M. Tavani, P. von Ballmoos +48

The e-ASTROGAM is a gamma-ray space mission to be proposed as the M5 Medium-size mission of the European Space Agency. It is dedicated to the observation of the Universe with unpre…

astro-ph.HE2021

Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation

The Cherenkov Telescope Array Consortium, :, H. Abdalla +496

The Cherenkov Telescope Array (CTA), the new-generation ground-based observatory for -ray astronomy, provides unique capabilities to address significant open questions in astro…

astro-ph.HE2025

Unveiling the origin of XMM-Newton soft proton flares II. Systematics in the proton spectral analysis

T. Mineo, V. Fioretti, S. Lotti +7

Low-energy protons entering the field of view of the XMM-Newton telescope scatter with the X-ray mirror surface and might reach the X-ray detectors on the focal plane. They manifes…

astro-ph.HE2016

Contributions of the Cherenkov Telescope Array (CTA) to the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016)

The CTA Consortium, :, A. Abchiche +1387

List of contributions from the Cherenkov Telescope Array (CTA) Consortium presented at the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016), July 11-15,…

astro-ph.IM2009

Simbol-X Background Minimization: Mirror Spacecraft Passive Shielding Trade-Off Study

V. Fioretti, G. Malaguti, A. Bulgarelli +3

The present work shows a quantitative trade-off analysis of the Simbol-X Mirror Spacecraft (MSC) passive shielding, in the phase space of the various parameters: mass budget, dimen…

astro-ph.HE2024

Quantum Convolutional Neural Networks for the detection of Gamma-Ray Bursts in the AGILE space mission data

A. Rizzo, N. Parmiggiani, A. Bulgarelli +17

Quantum computing represents a cutting-edge frontier in artificial intelligence. It makes use of hybrid quantum-classical computation which tries to leverage quantum mechanic princ…

astro-ph.HE2018

AGILE, Fermi, Swift, and GASP-WEBT multi-wavelength observations of the high-redshift blazar 4C 71.07 in outburst

S. Vercellone, P. Romano, G. Piano +56

The flat-spectrum radio quasar 4C 71.07 is a high-redshift (), -loud blazar whose optical emission is dominated by the thermal radiation from accretion disc. 4C

astro-ph.IM2014

The Agile Alert System For Gamma-Ray Transients

A. Bulgarelli, M. Trifoglio, F. Gianotti +26

In recent years, a new generation of space missions offered great opportunities of discovery in high-energy astrophysics. In this article we focus on the scientific operations of t…

astro-ph.IM2019

Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout

A. Acharyya, I. Agudo, E. O. Angüner +467

The Cherenkov Telescope Array (CTA) is the major next-generation observatory for ground-based very-high-energy gamma-ray astronomy. It will improve the sensitivity of current groun…

astro-ph.HE2019

The Second AGILE Catalog of Gamma-Ray Sources

A. Bulgarelli, V. Fioretti, N. Parmiggiani +25

Aims. We present the second AGILE-GRID Catalog (2AGL) of γ-ray sources in the 100 MeV-10 GeV energy range. Methods. With respect to previous AGILE-GRID catalogs, the current 2AGL…

astro-ph.HE2024

Deep Learning for AGILE Anticoincidence System's Background Prediction from Orbital and Attitude Parameters

N. Parmiggiani, A. Bulgarelli, A. Macaluso +8

AGILE is an Italian Space Agency (ASI) space mission launched in 2007 to study X-ray and gamma-ray phenomena in the energy range from 20 keV to 10 GeV. The AGILE AntiCo…

astro-ph.HE2022

ASTRI Mini-Array Core Science at the Observatorio del Teide

S. Vercellone, C. Bigongiari, A. Burtovoi +84

The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Project led by the Italian National Institute for Astrophysics (INAF) is developing and will deploy at the Obse…

astro-ph.IM2015

Data model issues in the Cherenkov Telescope Array project

J. L. Contreras, K. Satalecka, K. Bernlöhr +16

The planned Cherenkov Telescope Array (CTA), a future ground-based Very-High-Energy (VHE) gamma-ray observatory, will be the largest project of its kind. It aims to provide an orde…

hep-ph2024

Dark Matter Line Searches with the Cherenkov Telescope Array

S. Abe, J. Abhir, A. Abhishek +562

Monochromatic gamma-ray signals constitute a potential smoking gun signature for annihilating or decaying dark matter particles that could relatively easily be distinguished from a…

astro-ph.IM2020

Soft proton scattering at grazing incidence from X-ray mirrors: analysis of experimental data in the framework of the non-elastic approximation

R. Amato, T. Mineo, A. D'Aì +9

Astronomical X-ray observatories with grazing incidence optics face the problem of pseudo-focusing of low energy protons from the mirrors towards the focal plane. Those protons con…

astro-ph.HE2023

Preliminary Results of a New Deep Learning Method to Detect and Localize GRBs in the AGILE/GRID Sky Maps

N. Parmiggiani, A. Bulgarelli, A. Macaluso +12

AGILE is an ASI space mission launched in 2007 to study X-ray and gamma-ray phenomena in the energy range from keV to GeV. The AGILE Team developed a real-time an…

astro-ph.IM2023

The Online Observation Quality System Software Architecture for the ASTRI Mini-Array Project

N. Parmiggiani, A. Bulgarelli, L. Baroncelli +21

The ASTRI Mini-Array is an international collaboration led by the Italian National Institute for Astrophysics. This project aims to construct and operate an array of nine Imaging A…

astro-ph.HE2026

Localization and Confidence Region Estimation of Short GRBs with the COSI BGO Shield Using a HEALPix-Based Deep Learning Approach

N. Parmiggiani, A. Bulgarelli, G. Panebianco +17

The Compton Spectrometer and Imager is a NASA satellite mission under development that will survey the entire sky in the 0.2-5 MeV range using a wide-field germanium detector array…

astro-ph.HE2023

Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants

The Cherenkov Telescope Array Consortium, F. Acero, A. Acharyya +356

The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3~PeV. Sources which are capable of accelerating hadrons to such energies are called hadr…

astro-ph.HE2016

AGILE Observations of the Gravitational Wave Event GW150914

M. Tavani, C. Pittori, F. Verrecchia +35

We report the results of an extensive search in the AGILE data for a gamma-ray counterpart of the LIGO gravitational wave event GW150914. Currently in spinning mode, AGILE has the…

astro-ph.IM2021

RTApipe, a framework to develop astronomical pipelines for the real-time analysis of scientific data

N. Parmiggiani, A. Bulgarelli, D. Beneventano +4

In the multi-messenger era, astronomical projects share information about transients phenomena issuing science alerts to the Scientific Community through different communications n…