activity
20152026
most citedOn the Angular Resolution of the AGILE gamma-ray imaging detector

23 citations · 56 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2026

Twenty-five years of XMM-Newton EPIC-MOS2 Unfocused Particle Background: Solar Cycle Modulation, Galactic Cosmic-Ray Correlation, and Implications for NewAthena

B. Vaia, F. Gastaldello, S. Molendi +13

We present a study of the unfocused particle-induced background measured by the XMM-Newton EPIC-MOS2 detector, extending previous analyses to the end of 2025 and covering approxima…

astro-ph.IM2025★ 2 cited

Pre-flight Background Estimates for COSI

Savitri Gallego, Uwe Oberlack, Jan Lommler +14

The Compton Spectrometer and Imager (COSI) is a Compton telescope designed to survey the 0.2 - 5 MeV sky, consisting of a compact array of cross-strip germanium detectors. It is pl…

astro-ph.IM2025

Using the XMM-Newton small window mode to investigate systematic uncertainties in the particle background of X-ray charge-coupled device detectors

Gerrit Schellenberger, Ralph Kraft, Paul Nulsen +17

The level and uncertainty of the particle induced background in CCD detectors plays a crucial role for future X-ray instruments, such as the Wide Field Imager (WFI) onboard Athena.…

astro-ph.IM2025

The X-ray Integral Field Unit at the end of the Athena reformulation phase

Philippe Peille, Didier Barret, Edoardo Cucchetti +279

The Athena mission entered a redefinition phase in July 2022, driven by the imperative to reduce the mission cost at completion for the European Space Agency below an acceptable ta…

astro-ph.HE2025★ 4 cited

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.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.IM2017★ 8 cited

Updates on the background estimates for the X-IFU instrument onboard of the ATHENA mission

Simone Lotti, Claudio Macculi, Matteo D'Andrea +10

ATHENA, with a launch foreseen in 2028 towards the L2 orbit, addresses the science theme "The Hot and Energetic Universe", coupling a high-performance X-ray Telescope with two comp…

astro-ph.IM2015★ 12 cited

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.HE2015★ 23 cited

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…