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THESEUS is one of the three missions selected by ESA as fifth medium class mission (M5) candidates in its Cosmic Vision science program, currently under assessment in a phase A study with a planned launch date in 2032. THESEUS is designed…

Building on the success of the French-Chinese SVOM mission, our consortium proposes CATCH (Chasing All Transients Constellation of Hunters), targeting Gamma-Ray Bursts and X-ray transients. Its first step, CATCH-PM (Precursor Mission),…

Instrumentation and Methods for Astrophysics · Physics 2026-05-26 Stéphane Schanne

The HERMES (High Energy Rapid Modular Ensemble of Satellites) Pathfinder mission aims to develop a constellation of nanosatellites to study astronomical transient sources, such as gamma-ray bursts, in the X and soft $\gamma$ energy range,…

The multi-wavelength detection of GW170817 has inaugurated multi-messenger astronomy. The next step consists in interpreting observations coming from population of gravitational wave sources. We introduce saprEMo, a tool aimed at predicting…

Instrumentation and Methods for Astrophysics · Physics 2018-12-24 Serena Vinciguerra , Marica Branchesi , Riccardo Ciolfi , Ilya Mandel , Coenraad Neijssel , Giulia Stratta

Hard X-/soft gamma-ray astronomy is a crucial field for transient, nuclear and multimessenger astrophysics. However, the spatial localization, imaging capabilities and sensitivity of the measurements are strongly limited for the energy…

The High Energy Cosmic-Radiation Detection (HERD) facility has been proposed as a leading experiment on China's Space Station (CSS). Scheduled for installation around 2027, HERD is expected to operate for at least a decade. The main…

High Energy Astrophysical Phenomena · Physics 2025-04-18 Keerthana Rajan Lathika

THESEUS is a space mission concept, currently under Phase A study by ESA as candidate M5 mission, aiming at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and…

Instrumentation and Methods for Astrophysics · Physics 2021-02-18 Lorenzo Amati , Paul T. O'Brien , Diego Götz , Enrico Bozzo , Andrea Santangelo

The measurement of cosmic rays at energies exceeding 100 TeV per nucleon is crucial for enhancing the understanding of high-energy particle propagation and acceleration models in the Galaxy. HERD is a space-borne calorimetric experiment…

GrailQuest (Gamma-ray Astronomy International Laboratory for Quantum Exploration of Space-Time) is an ambitious astrophysical mission concept that uses a fleet of small satellites whose main objective is to search for a dispersion law for…

High Energy Astrophysical Phenomena · Physics 2021-01-19 L. Burderi , T. Di Salvo , A. Sanna , F. Fiore , A. Riggio , A. F. Gambino , the HERMES-TP , HERMES-SP Collaborations

As a new member of GECAM mission, the GECAM-C (also called High Energy Burst Searcher, HEBS) is a gamma-ray all-sky monitor onboard SATech-01 satellite, which was launched on July 27th, 2022 to detect gamma-ray transients from 6 keV to 6…

HERMES, a fibre-fed high-resolution (R=85000) echelle spectrograph with good stability and excellent throughput, is the work-horse instrument of the 1.2-m Mercator telescope on La Palma. HERMES targets building up time series of…

Instrumentation and Methods for Astrophysics · Physics 2015-06-17 Gert Raskin , Hans Van Winckel

The High Energy cosmic-Radiation Detector (HERD) facility is planned to go onboard China's Space Station, planned to be operational starting in around 2025 for about 10 years. The main scientific objectives of HERD are the search for…

Instrumentation and Detectors · Physics 2020-08-26 P. W. Cattaneo , M. Pullia , M. C. Prata , A. Rappoldi , M. Rossella

The High-Energy Particle Detector (HEPD) is one of the payloads of the CSES space mission. The CSES (China Seismo-Electromagnetic Satellite) mission will investigate the structure and the dynamic of the topside ionosphere, will monitor…

Instrumentation and Methods for Astrophysics · Physics 2017-02-01 Beatrice Panico , Francesco Palma , Alessandro Sotgiu

Multi-messenger observations of the transient sky to detect cosmic explosions and counterparts of gravitational wave mergers critically rely on orbiting wide-FoV telescopes to cover the wide range of wavelengths where atmospheric absorption…

The China Seismo Electromagnetic Satellite (CSES) aims to contribute to the monitoring of earthquakes from space. This space mission, lead by a Chinese-Italian collaboration, will study phenomena of electromagnetic nature and their…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 V. Scotti , G. Osteria

The third-generation of gravitational wave observatories, such as the Einstein Telescope (ET) and Cosmic Explorer (CE), aim for an improvement in sensitivity of at least a factor of ten over a wide frequency range compared to the current…

Instrumentation and Methods for Astrophysics · Physics 2022-10-05 A. Utina , A. Amato , J. Arends , C. Arina , M. de Baar , M. Baars , P. Baer , N. van Bakel , W. Beaumont , A. Bertolini , M. van Beuzekom , S. Biersteker , A. Binetti , H. J. M. ter Brake , G. Bruno , J. Bryant , H. J. Bulten , L. Busch , P. Cebeci , C. Collette , S. Cooper , R. Cornelissen , P. Cuijpers , M. van Dael , S. Danilishin , D. Dixit , S. van Doesburg , M. Doets , R. Elsinga , V. Erends , J. van Erps , A. Freise , H. Frenaij , R. Garcia , M. Giesberts , S. Grohmann , H. Van Haevermaet , S. Heijnen , J. V. van Heijningen , E. Hennes , J. -S. Hennig , M. Hennig , T. Hertog , S. Hild , H. -D. Hoffmann , G. Hoft , M. Hopman , D. Hoyland , G. A. Iandolo , C. Ietswaard , R. Jamshidi , P. Jansweijer , A. Jones , P. Jones , N. Knust , G. Koekoek , X. Koroveshi , T. Kortekaas , A. N. Koushik , M. Kraan , M. van de Kraats , S. L. Kranzhoff , P. Kuijer , K. A. Kukkadapu , K. Lam , N. Letendre , P. Li , R. Limburg , F. Linde , J. -P. Locquet , P. Loosen , H. Lueck , M. Martınez , A. Masserot , F. Meylahn , M. Molenaar , C. Mow-Lowry , J. Mundet , B. Munneke , L. van Nieuwland , E. Pacaud , D. Pascucci , S. Petit , Z. Van Ranst , G. Raskin , P. M. Recaman , N. van Remortel , L. Rolland , L. de Roo , E. Roose , J. C. Rosier , D. Ryckbosch , K. Schouteden , A. Sevrin , A. Sider , A. Singha , V. Spagnuolo , A. Stahl , J. Steinlechner , S. Steinlechner , B. Swinkels , N. Szilasi , M. Tacca , H. Thienpont , A. Vecchio , H. Verkooijen , C. H. Vermeer , M. Vervaeke , G. Visser , R. Walet , P. Werneke , C. Westhofen , B. Willke , A. Xhahi , T. Zhang

Since their discovery at radio wavelengths pulsars have been persistent targets for widespread multi-wave observations throughout optics, radio, X-rays, and high-energy gamma-rays. Observations with the EGRET gamma-ray telescope, on board…

Astrophysics · Physics 2007-05-23 A. Konopelko

THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a…

Instrumentation and Methods for Astrophysics · Physics 2018-06-13 L. Amati , P. O'Brien , D. Goetz , E. Bozzo , C. Tenzer , F. Frontera , G. Ghirlanda , C. Labanti , J. P. Osborne , G. Stratta , N. Tanvir , R. Willingale , P. Attina , R. Campana , A. J. Castro-Tirado , C. Contini , F. Fuschino , A. Gomboc , R. Hudec , P. Orleanski , E. Renotte , T. Rodic , Z. Bagoly , A. Blain , P. Callanan , S. Covino , A. Ferrara , E. Le Floch , M. Marisaldi , S. Mereghetti , P. Rosati , A. Vacchi , P. D'Avanzo , P. Giommi , A. Gomboc , S. Piranomonte , L. Piro , V. Reglero , A. Rossi , A. Santangelo , R. Salvaterra , G. Tagliaferri , S. Vergani , S. Vinciguerra , M. Briggs , E. Campolongo , R. Ciolfi , V. Connaughton , B. Cordier , B. Morelli , M. Orlandini , C. Adami , A. Argan , J. -L. Atteia , N. Auricchio , L. Balazs , G. Baldazzi , S. Basa , R. Basak , P. Bellutti , M. G. Bernardini , G. Bertuccio , J. Braga , M. Branchesi , S. Brandt , E. Brocato , C. Budtz-Jorgensen , A. Bulgarelli , L. Burderi , J. Camp , S. Capozziello , J. Caruana , P. Casella , B. Cenko , P. Chardonnet , B. Ciardi , S. Colafrancesco , M. G. Dainotti , V. D'Elia , D. De Martino , M. De Pasquale , E. Del Monte , M. Della Valle , A. Drago , Y. Evangelista , M. Feroci , F. Finelli , M. Fiorini , J. Fynbo , A. Gal-Yam , B. Gendre , G. Ghisellini , A. Grado , C. Guidorzi , M. Hafizi , L. Hanlon , J. Hjorth , L. Izzo , L. Kiss , P. Kumar , I. Kuvvetli , M. Lavagna , T. Li , F. Longo , M. Lyutikov , U. Maio , E. Maiorano , P. Malcovati , D. Malesani , R. Margutti , A. Martin-Carrillo , N. Masetti , S. McBreen , R. Mignani , G. Morgante , C. Mundell , H. U. Nargaard-Nielsen , L. Nicastro , E. Palazzi , S. Paltani , F. Panessa , G. Pareschi , A. Pe'er , A. V. Penacchioni , E. Pian , E. Piedipalumbo , T. Piran , G. Rauw , M. Razzano , A. Read , L. Rezzolla , P. Romano , R. Ruffini , S. Savaglio , V. Sguera , P. Schady , W. Skidmore , L. Song , E. Stanway , R. Starling , M. Topinka , E. Troja , M. van Putten , E. Vanzella , S. Vercellone , C. Wilson-Hodge , D. Yonetoku , G. Zampa , N. Zampa , B. Zhang , B. B. Zhang , S. Zhang , S. -N. Zhang , A. Antonelli , F. Bianco , S. Boci , M. Boer , M. T. Botticella , O. Boulade , C. Butler , S. Campana , F. Capitanio , A. Celotti , Y. Chen , M. Colpi , A. Comastri , J. -G. Cuby , M. Dadina , A. De Luca , Y. -W. Dong , S. Ettori , P. Gandhi , E. Geza , J. Greiner , S. Guiriec , J. Harms , M. Hernanz , A. Hornstrup , I. Hutchinson , G. Israel , P. Jonker , Y. Kaneko , N. Kawai , K. Wiersema , S. Korpela , V. Lebrun , F. Lu , A. MacFadyen , G. Malaguti , L. Maraschi , A. Melandri , M. Modjaz , D. Morris , N. Omodei , A. Paizis , P. Pata , V. Petrosian , A. Rachevski , J. Rhoads , F. Ryde , L. Sabau-Graziati , N. Shigehiro , M. Sims , J. Soomin , D. Szecsi , Y. Urata , M. Uslenghi , L. Valenziano , G. Vianello , S. Vojtech , D. Watson , J. Zicha

JEM-EUSO is an international collaboration for the development of space--based Ultra High Energy Cosmic Ray (UHECR) detectors. The instrument consists of a wide Field Of View (FOV) camera for the detection of the UV light emitted by…

High Energy Astrophysical Phenomena · Physics 2017-03-07 Francesco Fenu

As a new member of GECAM mission, GECAM-C (also named High Energy Burst Searcher, HEBS) was launched onboard the SATech-01 satellite on July 27th, 2022, which is capable to monitor gamma-ray transients from $\sim$ 6 keV to 6 MeV. As the…