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19932026
most citedThe Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission

4.1k citations

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astro-ph.IM2026

Scientific performances of the XGIS instrument on-board THESEUS

E. Arrigoni, S. Mereghetti, R. Campana +6

The Transient High Energy Sky and Early Universe Surveyor (THESEUS) satellite, currently undergoing a Phase-A study for the M7 ESA mission selection, will mainly rely on the XGIS (…

astro-ph.IM2026

Multivariate time-series forecasting of ASTRI-Horn monitoring data: A Normal Behavior Model

Federico Incardona, Alessandro Costa, Farida Farsian +8

This study presents a Normal Behavior Model (NBM) developed to forecast monitoring time-series data from the ASTRI-Horn Cherenkov telescope under normal operating conditions. The a…

astro-ph.IM2025★ 4 cited

Conceptual Opto-Mechanical design of SHARP: a near-infrared multi-mode spectrograph conceived for the next-generation telescopes

H. Mahmoodzadeh, P. Saracco, P. Conconi +18

The next generation of Extremely Large Telescopes (ELTs), with their wide apertures and advanced Multi-Conjugate Adaptive Optics (MCAO) systems, will provide unprecedented sharp an…

astro-ph.IM2025★ 7 cited

Unveiling the origin of XMM-Newton soft proton flares: I. Design and validation of a response matrix for proton spectral analysis

Valentina Fioretti, Teresa Mineo, Simone Lotti +8

Low-energy (<300 keV) protons entering the field of view of XMM-Newton are observed in the form of a sudden increase in the background level, the so-called soft proton flares, affe…

astro-ph.IM2024★ 5 cited

Design and development of the HERMES Pathfinder payloads

R. Campana, Y. Evangelista, F. Fiore +22

HERMES (High Energy Rapid Modular Ensemble of Satellites) Pathfinder mission aims to observe and localize Gamma Ray Bursts (GRBs) and other transients using a constellation of nano…

astro-ph.IM2023

GRBAlpha: the smallest astrophysical space observatory -- Part 1: Detector design, system description and satellite operations

András Pál, Masanori Ohno, László Mészáros +42

Aims. Since launched on 2021 March 22, the 1U-sized CubeSat GRBAlpha operates and collects scientific data on high-energy transients, making it the smallest astrophysical space obs…

astro-ph.IM2022★ 19 cited

SIPGI: an interactive pipeline for spectroscopic data reduction

A. Gargiulo, M. Fumana, S. Bisogni +5

We present SIPGI, a spectroscopic pipeline to reduce optical/near-infrared data from slit-based spectrographs. SIPGI is a complete spectroscopic data reduction environment which re…

astro-ph.IM2022

Athena charged particle diverter simulations: effects of micro-roughness on proton scattering using Geant4

Jean-Paul Breuer, Gábor Galgóczi, Valentina Fioretti +12

The last generation of X-ray focusing telescopes operating outside the Earth's radiation belt discovered that optics were able to focus not only astrophysical X-ray photons, but al…

astro-ph.IM2022★ 18 cited

First light of BEaTriX, the new testing facility for the modular X-ray optics of the ATHENA mission

S. Basso, B. Salmaso, D. Spiga +35

The Beam Expander Testing X-ray facility (BEaTriX) is a unique X-ray apparatus now operated at the Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Brera (OAB)…

astro-ph.IM2022★ 59 cited

Sonification and Sound Design for Astronomy Research, Education and Public Engagement

A. Zanella, C. M. Harrison, S. Lenzi +3

Over the last ten years there has been a large increase in the number of projects using sound to represent astronomical data and concepts. Motivation for these projects includes th…

astro-ph.IM2022★ 15 cited

Exploring X-ray variability with unsupervised machine learning I. Self-organizing maps applied to XMM-Newton data

Miloš Kovačević, Mario Pasquato, Martino Marelli +3

XMM-Newton provides unprecedented insight into the X-ray Universe, recording variability information for hundreds of thousands of sources. Manually searching for interesting patter…

astro-ph.IM2022★ 14 cited

Mirror production for the Cherenkov telescopes of the ASTRI Mini-Array and of the MST project for the Cherenkov Telescope Array

N. La Palombara, G. Sironi, E. Giro +14

The Cherenkov Telescope Array (CTA) is the next ground-based -ray observatory in the TeV -ray spectral region operating with the Imaging Atmospheric Cherenkov Technique. It i…

astro-ph.IM2021★ 9 cited

The Fluorescence Telescope on board EUSO-SPB2 for the detection of Ultra High Energy Cosmic Rays

G. Osteria, J. Adams, M. Battisti +37

The Fluorescence Telescope is one of the two telescopes on board the Extreme Universe Space Observatory on a Super Pressure Balloon II (EUSO-SPB2). EUSO-SPB2 is an ultra-long-durat…

astro-ph.IM2021★ 2 cited

The Aperture Array Verification System 1: System overview and early commissioning results

P. Benthem, R. Wayth, E. de Lera Acedo +51

The design and development process for the Square Kilometre Array (SKA) radio telescope, the Low Frequency Aperture Array component, was progressed during the SKA pre-construction…

astro-ph.IM2021★ 68 cited

Fermi Large Area Telescope Performance After 10 Years Of Operation

The Fermi LAT Collaboration, M. Ajello, W. B. Atwood +126

The Large Area Telescope (LAT), the primary instrument for the Fermi Gamma-ray Space Telescope (Fermi) mission, is an imaging, wide field-of-view, high-energy gamma-ray telescope,…

astro-ph.IM2021★ 10 cited

Synergies of THESEUS with the large facilities of the 2030s and guest observer opportunities

P. Rosati, S. Basa, A. W. Blain +37

The proposed THESEUS mission will vastly expand the capabilities to monitor the high-energy sky, and will exploit large samples of gamma-ray bursts to probe the early Universe back…

astro-ph.IM2021★ 20 cited

Gamma Ray Burst studies with THESEUS

G. Ghirlanda, R. Salvaterra, M. Toffano +30

Gamma-ray Bursts (GRBs) are the most powerful transients in the Universe, over-shining for a few seconds all other -ray sky sources. Their emission is produced within narrowly c…

astro-ph.IM2021★ 2 cited

Multi-Messenger Astrophysics with THESEUS in the 2030s

Riccardo Ciolfi, Giulia Stratta, Marica Branchesi +63

Multi-messenger astrophysics is becoming a major avenue to explore the Universe, with the potential to span a vast range of redshifts. The growing synergies between different probe…

astro-ph.IM2021★ 1 cited

Exploration of the high-redshift universe enabled by THESEUS

N. R. Tanvir, E. Le Floc'h, L. Christensen +36

At peak, long-duration gamma-ray bursts are the most luminous sources of electromagnetic radiation known. Since their progenitors are massive stars, they provide a tracer of star f…

astro-ph.IM2021★ 3 cited

The THESEUS space mission: science goals, requirements and mission concept

L. Amati, P. T. O'Brien, D. Götz +31

THESEUS, one of the two space mission concepts being studied by ESA as candidates for next M5 mission within its Comsic Vision programme, aims at fully exploiting Gamma-Ray Bursts…

astro-ph.IM2021

The XGIS instrument on-board THESEUS: Monte Carlo simulations for response, background, and sensitivity

Riccardo Campana, Fabio Fuschino, Claudio Labanti +6

The response of the X and Gamma Imaging Spectrometer (XGIS) instrument onboard the Transient High Energy Sky and Early Universe Surveyor (THESEUS) mission, selected by ESA for an a…

astro-ph.IM2021★ 22 cited

Review of the particle background of the Athena X-IFU instrument

Simone Lotti, Matteo D'Andrea, Silvano Molendi +6

X-ray observations are limited by the background, due to intrinsic faintness or diffuse nature of the sources. The future Athena X-ray observatory has among its goals the character…

astro-ph.IM2020★ 16 cited

Analysis of the unconcentrated background of the EPIC-pn camera on board XMM-Newton

Martino Marelli, Silvano Molendi, Mariachiara Rossetti +8

Our understanding of the background of the EPIC/pn camera onboard XMM-Newton is incomplete. This affects the study of extended sources and can influence the predictions of the back…

astro-ph.IM2020★ 16 cited

Prediction and understanding of soft proton contamination in XMM-Newton: a machine learning approach

E. A. Kronberg, F. Gastaldello, S. Haaland +10

One of the major and unfortunately unforeseen sources of background for the current generation of X-ray telescopes are few tens to hundreds of keV (soft) protons concentrated by th…