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Informace o publikaci
GRINTA: a new probe of the dynamic universe
| Autoři | |
|---|---|
| Rok publikování | 2026 |
| Druh | Stať ve sborníku |
| Konference | Proc. SPIE 14146, Space Telescopes and Instrumentation 2026: Ultraviolet to Gamma Ray |
| Fakulta / Pracoviště MU | |
| 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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