Informace o publikaci

GRINTA: a new probe of the dynamic universe

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NATALUCCI Lorenzo LAURENT Philippe BRANCHESI Marica FIOCCHI Mariateresa HANLON Lorraine MAS-HESSE J. Miguel MEURIS Aline O'BRIEN Paul RODI James C. SCARINGI Simone SKUP Konrad WERNER Norbert ZANE Silvia ALFONSO-GARZON Julia BANERJEE Biswajit BARRIA Patrizia BIRD Anthony J. BRANDT Soren BRUNI Gabriele CANGEMI Floriane CASTIGNANI Gianluca CHASSANDE-MOTTIN Eric CHATY Sylvain CHENEVEZ Jerome COLEIRO Alexis DAZZI Francesco DE SANTIS Alessio L. EVANS Phil GODET Olivier GOTZ Diego HUDEC Rene KUIPER Lucien MALIZIA Angela MCBREEN Sheila MEREGHETTI Sandro MOLINA Manuela MÜNZ Filip MURPHY David OGANESYAN Gor PANESSA Francesca PIAN Elena ŘÍPA Jakub ROBERTS Oliver J. RONCHINI Samuele SCHUSSLER Fabian ŠIMON Vojtěch TANVIR Nial ULIYANOV Alexey VERTOLLI Nello VITEK Stanislav ZANNONI Ugo

Rok publikování 2026
Druh Stať ve sborníku
Konference Proc. SPIE 14146, Space Telescopes and Instrumentation 2026: Ultraviolet to Gamma Ray
Fakulta / Pracoviště MU

Přírodovědecká fakulta

Citace
www https://www.spiedigitallibrary.org/conference-proceedings-of-spie/14146/3105908/GRINTA-a-new-probe-of-the-dynamic-universe/10.1117/12.3105908.full
Doi https://doi.org/10.1117/12.3105908
Klíčová slova Multi-messenger astronomy; High energy surveys; AGNs and their evolution; Physics of Compact objects; Non-thermal phenomena; cosmic-ray and astroparticle; Technologies for high energy astrophysics
Popis Recent observations of the transient sky at all wavelengths are increasingly revealing the importance of the multi-messenger and multi-wavelength approach. The GRINTA (Gamma-Ray INternational Transient Array Observatory) mission, proposed for launch around the middle of the next decade, is conceived as a small mission with good sensitivity, excellent angular resolution and fast follow-up capability for studying transient sources at timescales from ms to hours, at the same time ensuring optimal integration with multi-messenger networks. The GRINTA mission will carry two complementary payloads to cover in total the 5 keV-10 MeV band, that will detect and localise gamma-ray bursts covering ~ half of the sky and will be able to perform imaging surveys with sub-arcmin resolution. GRINTA will operate in synergy with the most powerful electromagnetic, gravitational wave and neutrino observatories foreseen to be operational after ~ 2035.
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