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Просмотр по теме "Gamma-ray bursts"

Просмотр по теме "Gamma-ray bursts"

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  • Exploration of the high-redshift universe enabled by THESEUS 
    Tanvir N.R.; Le Floc’h E.; Christensen L.; Caruana J.; Salvaterra R.; Ghirlanda G.; Ciardi B.; Maio U.; D’Odorico V.; Piedipalumbo E.; Campana S.; Noterdaeme P.; Graziani L.; Amati L.; Bagoly Z.; Balázs L.G.; Basa S.; Behar E.; De Cia A.; Valle M.D.; De Pasquale M.; Frontera F.; Gomboc A.; Götz D.; Horvath I.; Hudec R.; Mereghetti S.; O’Brien P.T.; Osborne J.P.; Paltani S.; Rosati P.; Sergijenko O.; Stanway E.R.; Szécsi D.; Tot́h L.V.; Urata Y.; Vergani S.; Zane S. (2021)
    At peak, long-duration gamma-ray bursts are the most luminous sources of electromagnetic radiation known. Since their progenitors are massive stars, they provide a tracer of star formation and star-forming galaxies over ...
  • Statistical properties of GRB afterglow parameters as evidence of cosmological evolution of their host galaxies 
    Beskin G.; Oganesyan G.; Greco G.; Karpov S. (2014)
    The results of a study of 43 peaked R-band light curves of optical counterparts of gamma-ray bursts with known redshifts are presented. The parameters of optical transients were calculated in the comoving frame, and then ...
  • Status and perspectives of the Mini-MegaTORTORA wide-field monitoring system with high temporal resolution 
    Karpov S.; Beskin G.; Bondar S.; Perkov A.; Ivanov E.; Guarnieri A.; Bartolini C.; Greco G.; Shearer A.; Sasyuk V. (2013)
    Here we briefly summarize our long-term experience of constructing and operating wide-field monitoring cameras with sub-second temporal resolution to look for optical components of GRBs, fast-moving satellites and meteors. ...
  • THESEUS: A key space mission concept for Multi-Messenger Astrophysics 
    Stratta G.; Ciolfi R.; Amati L.; Bozzo E.; Ghirlanda G.; Maiorano E.; Nicastro L.; Rossi A.; Vinciguerra S.; Frontera F.; Götz D.; Guidorzi C.; O'Brien P.; Osborne J.; Tanvir N.; Branchesi M.; Brocato E.; Dainotti M.; De Pasquale M.; Grado A.; Greiner J.; Longo F.; Maio U.; Mereghetti D.; Mignani R.; Piranomonte S.; Rezzolla L.; Salvaterra R.; Starling R.; Willingale R.; Böer M.; Bulgarelli A.; Caruana J.; Colafrancesco S.; Colpi M.; Covino S.; D'Avanzo P.; D'Elia V.; Drago A.; Fuschino F.; Gendre B.; Hudec R.; Jonker P.; Labanti C.; Malesani D.; Mundell C.; Palazzi E.; Patricelli B.; Razzano M.; Campana R.; Rosati P.; Rodic T.; Szécsi D.; Stamerra A.; van Putten M.; Vergani S.; Zhang B.; Bernardini M. (2018)
    © 2018 COSPAR The recent discovery of the electromagnetic counterpart of the gravitational wave source GW170817, has demonstrated the huge informative power of multi-messenger observations. During the next decade the nascent ...

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