2.7k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- G. Cusumano2 profiles86 · h 43
- P. Romano3 profiles80 · h 49
- A. Segreto52 · h 55
- V. Mangano3 profiles39 · h 68
- T. Mineo4 profiles37 · h 21
- S. Campana3 profiles36 · h 62
- V. La Parola2 profiles34 · h 12
- F. Frontera2 profiles33 · h 52
- D. Burrows2 profiles31 · h 57
- G. Chincarini2 profiles31 · h 59
- G. Tagliaferri2 profiles30 · h 78
- N. Gehrels2 profiles29 · h 120
- National Institute for AstrophysicsIT232 papers
- Pennsylvania State UniversityUS153 papers
- Brera Astronomical ObservatoryIT149 papers
- Centre National de la Recherche ScientifiqueFR129 papers
- Goddard Space Flight CenterUS112 papers
- Astronomical Observatory of RomeIT105 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di TorinoIT99 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di NapoliIT97 papers
- University of PalermoIT96 papers
- University of Rome Tor VergataIT94 papers
- University of TurinIT93 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di CataniaIT87 papers
41 papers · 1 filter
The Vera C. Rubin Observatory Data Preview 1
Vera C Rubin Observatory Team, Tatiana Acero Cuellar, Emily Acosta +325
We present Rubin Data Preview 1 DP1, the first data from the NSF DOE Vera C Rubin Observatory, comprising raw and calibrated single epoch images, coadds, difference images, detecti…
A simple, flexible method for timing cross-calibration of space missions
Matteo Bachetti, Yukikatsu Terada, Megumi Shidatsu +25
The timing (cross-)calibration of astronomical instruments is often done by comparing pulsar times-of-arrival (TOAs) to a reference timing model. In high-energy astronomy, the choi…
X-ray spectral fitting with Monte Carlo Dropout Neural Networks
A. Tutone, A. Anitra, E. Ambrosi +11
We present a novel approach using neural networks to recover X-ray spectral model parameters and quantify uncertainties, balancing accuracy and computational efficiency against tra…
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…
The EUSO-SPB2 Fluorescence Telescope for the Detection of Ultra-High Energy Cosmic Rays
James H. Adams, Denis Allard, Phillip Alldredge +79
The Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2) flew on May 13 and 14 of 2023. Consisting of two novel optical telescop…
EUSO-SPB1 Mission and Science
EUSO Collaboration, G. Abdellaoui, S. Abe +292
The Extreme Universe Space Observatory on a Super Pressure Balloon 1 (EUSO-SPB1) was launched in 2017 April from Wanaka, New Zealand. The plan of this mission of opportunity on a N…
Developments and results in the context of the JEM-EUSO program obtained with the ESAF Simulation and Analysis Framework
S. Abe, J. H. Adams, D. Allard +172
JEM--EUSO is an international program for the development of space-based Ultra-High Energy Cosmic Ray observatories. The program consists of a series of missions which are either u…
Gain variations as induced by the diffuse night sky background: the ASTRI-Horn experience
D. Impiombato, A. A. Compagnino, T. Mineo +3
ASTRI-Horn is the prototype of the nine telescopes that form the ASTRI Mini-Array, under construction at the Teide Observatory in Tenerife (Spain), devoted to observe the sky in th…
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…
Design and Performance of the Prototype Schwarzschild-Couder Telescope Camera
Colin B. Adams, Giovanni Ambrosi, Michelangelo Ambrosio +86
The prototype Schwarzschild-Couder Telescope (pSCT) is a candidate for a medium-sized telescope in the Cherenkov Telescope Array. The pSCT is based on a novel dual mirror optics de…
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…
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…
Expected Performance of the EUSO-SPB2 Fluorescence Telescope
G. Filippatos, M. Battisti, M. Bertaina +6
The Extreme Universe Space Observatory Supper Pressure Balloon 2 (EUSO-SPB2) is under development, and will prototype instrumentation for future satellite-based missions, including…
Effective pointing of the ASTRI-Horn telescope using the Cherenkov camera with the Variance method
Simone Iovenitti, Giorgia Sironi, Alberto Segreto +2
Cherenkov telescope cameras are not suitable to perform astrometrical pointing calibration since they are not designed to produce images of the sky, but rather to detect nanosecond…
UVscope and its application aboard the ASTRI-Horn telescope
M. C. Maccarone, G. La Rosa, O. Catalano +9
UVscope is an instrument, based on a multi-pixel photon detector, developed to support experimental activities for high-energy astrophysics and cosmic ray research. The instrument,…
The Payload Data Handling Unit (PDHU) on-board the HERMES-TP and HERMES-SP CubeSat Missions
A. Guzman, S. Pliego, J. Bayer +14
The High Energy Rapid Modular Ensemble of Satellites (HERMES) Technological and Scientific pathfinder is a space borne mission based on a constellation of LEO nanosatellites. The p…
Design and implementation of the AMIGA embedded system for data acquisition
The Pierre Auger Collaboration, A. Aab, P. Abreu +383
The Auger Muon Infill Ground Array (AMIGA) is part of the AugerPrime upgrade of the Pierre Auger Observatory. It consists of particle counters buried 2.3 m underground next to the…
The FRAM robotic telescope for atmospheric monitoring at the Pierre Auger Observatory
The Pierre Auger Collaboration, A. Aab, P. Abreu +377
FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stell…
Deep-Learning based Reconstruction of the Shower Maximum using the Water-Cherenkov Detectors of the Pierre Auger Observatory
The Pierre Auger Collaboration, A. Aab, P. Abreu +370
The atmospheric depth of the air shower maximum is an observable commonly used for the determination of the nuclear mass composition of ultra-high energy cosmic…
Calibration of the underground muon detector of the Pierre Auger Observatory
The Pierre Auger Collaboration, A. Aab, P. Abreu +370
To obtain direct measurements of the muon content of extensive air showers with energy above eV, the Pierre Auger Observatory is currently being equipped with an underg…
Using Muon Rings for the Calibration of the Cherenkov Telescope Array: A Systematic Review of the Method and its Potential Accuracy
Markus Gaug, Steven Fegan, Alison Mitchell +3
The analysis of ring images produced by muons in an Imaging Atmospheric Cherenkov Telescope (IACT) provides a powerful and precise method to calibrate the IACT optical throughput a…
First observations of speed of light tracks by a fluorescence detector looking down on the atmosphere
G. Abdellaoui, S. Abe, J. H. Adams +311
EUSO-Balloon is a pathfinder mission for the Extreme Universe Space Observatory onboard the Japanese Experiment Module (JEM-EUSO). It was launched on the moonless night of the 25$^…
The Geant4 mass model of the ATHENA Silicon Pore Optics and its effect on soft proton scattering
Valentina Fioretti, Andrea Bulgarelli, Simone Lotti +6
Given the unprecedented effective area, the new ATHENA Silicon Pore Optics (SPO) focusing technology, the dynamic and variable L2 environment, where no X-ray mission has flown up t…
Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory
The Pierre Auger Collaboration, A. Aab, P. Abreu +392
With the Auger Engineering Radio Array (AERA) of the Pierre Auger Observatory, we have observed the radio emission from 561 extensive air showers with zenith angles between 60$^\ci…