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Astronomical transients, such as supernovae and other rare stellar explosions, have been instrumental in some of the most significant discoveries in astronomy. New astronomical sky surveys will soon record unprecedented numbers of…

Instrumentation and Methods for Astrophysics · Physics 2023-11-30 Hali Huang , Daniel Muthukrishna , Prajna Nair , Zimi Zhang , Michael Fausnaugh , Torsha Majumder , Ryan J. Foley , George R. Ricker

The Swift Gamma-ray Burst (GRB) observatory responds to GRB triggers with optical observations in ~ 100 s, but cannot respond faster than ~ 60 s. While some ground-based telescopes respond quickly, the number of sub-60 s detections remains…

A new ground-based wide-field extensive air shower array known as the High-Altitude Water Cherenkov (HAWC) Observatory promises a new window to monitoring the $\sim$100 GeV gamma-ray sky with the potential for detecting a high energy…

High Energy Astrophysical Phenomena · Physics 2018-01-08 Joshua Wood

The primary challenge in the study of explosive astrophysical transients is their detection and characterisation using multiple messengers. For this purpose, we have developed a new data-driven discovery framework, based on deep learning.…

High Energy Astrophysical Phenomena · Physics 2020-05-14 Iftach Sadeh

In the context of time domain astronomy, we present an offline detection search of gamma-ray transients using a wild binary segmentation analysis called FWBSB targeting both short and long gamma-ray bursts (GRBs) and covering the soft and…

Instrumentation and Methods for Astrophysics · Physics 2020-02-05 Sarah Antier , Kateryna Barynova , Piotr Fryzlewicz , Cyril Lachaud , Gerard Marchal-Duval

This paper is an extended summary of the talk I gave at IAU Symposium "New Horizons in Time Domain Astronomy" (Oxford, 2011). I first review the history of transients (which is intimately related to the advent of wide-field telescopic…

High Energy Astrophysical Phenomena · Physics 2012-02-14 S. R. Kulkarni

We explore the possibility of very long-lived gravitational-wave transients (and detector artifacts) lasting hours to weeks. Such very long signals are both interesting in their own right and as a potential source of systematic error in…

Instrumentation and Methods for Astrophysics · Physics 2015-06-03 Eric Thrane , Vuk Mandic , Nelson Christensen

The rise of multi-messenger astronomy has brought with it the need to exploit all available data streams and learn more about the astrophysical objects that fall within its breadth. One possible avenue is the search for serendipitous…

Fast radio burst (FRBs) are an exciting class of bright, extragalactic, millisecond radio transients. The recent development of large field-of-view (FOV) radio telescopes has caused a rapid rise in the number of identified single burst and…

High Energy Astrophysical Phenomena · Physics 2021-08-24 Matthew Lundy

Gamma-ray bursts (GRBs) are intense, short-lived bursts of gamma-ray radiation observed up to a high redshift ($z \sim 10$) due to their luminosities. Thus, they can serve as cosmological tools to probe the early Universe. However, we need…

NASA's Swift satellite has completed ten years of amazing discoveries in time domain astronomy. Its primary mission is to chase gamma-ray bursts (GRBs), but due to its scheduling flexibility it has subsequently become a prime discovery…

High Energy Astrophysical Phenomena · Physics 2015-03-24 Neil Gehrels , John K. Cannizzo

The era of time domain multi-messenger (MM) astrophysics requires sensitive, large field-of-view (FoV) observatories that are able to quickly react in order to respond to alerts from gravitational wave (GW) triggers, neutrino detections,…

High Energy Astrophysical Phenomena · Physics 2025-04-08 James Rodi , Lorenzo Natalucci

The discovery of gravitational waves, high-energy neutrinos or the very-high-energy counterpart of gamma-ray bursts has revolutionized the high-energy and transient astrophysics community. The development of new instruments and analysis…

High Energy Astrophysical Phenomena · Physics 2021-06-09 Ž. Bošnjak , A. M. Brown , A. Carosi , M. Chernyakova , P. Cristofari , F. Longo , A. López-Oramas , M. Santander , K. Satalecka , F. Schüssler , O. Sergijenko , A. Stamerra , I. Agudo , R. Alves Batista , E. Amato , E. O. Anguner , L. A. Antonelli , M. Backes , Csaba Balazs , L. Baroncelli , J. Becker Tjus , C. Bigongiari , E. Bissaldi , C. Boisson , J. Bolmont , M. Böttcher , P. Bordas , C. Braiding , J. Bregeon , N. Bucciantini , A. Bulgarelli , M. Burton , F. Cangemi , P. Caraveo , M. Cardillo , S. Caroff , S. Casanova , S. Chaty , J. G. Coelho , G. Cotter , A. D'Aì , F. D'Ammando , E. M. de Gouveia Dal Pino , D. della Volpe , D. de Martino , T. Di Girolamo , A. Di Piano , A. Djannati-Ataï , V. Dwarkadas , E. de Ona Wilhelmi , R. C. Dos Anjos , G. Emery , E. Fedorova , S. Fegan , A. Fiasson , V. Fioretti , M. D. Filipovic , D. Gaggero , G. Galanti , D. Gasparrini , G. Ghirlanda , P. Goldoni , J. Granot , J. G. Green , M. Heller , B. Hnatyk , R. Hnatyk , D. Horan , T. Hovatta , S. Inoue , M. Jamrozy , D. Kantzas , B. Khélifi , N. Komin , A. Lamastra , N. La Palombara , J. P. Lenain , E. Lindfors , I. Liodakis , S. Lombardi , F. Lucarelli , P. L. Luque-Escamilla , P. Majumdar , A. Marcowith , S. Markoff , J. Marti , M. Martinez , D. Mazin , S. McKeague , S. Mereghetti , E. Mestre , T. Montaruli , G. Morlino , A. Morselli , C. Mundell , T. Murach , L. Nava , A. Nayerhoda , L. Nicastro , J. Niemiec , M. Nikolajuk , B. Olmi , R. Ong , M. Orienti , J. P. Osborne , Josep M. Paredes , G. Pareschi , N. Parmiggiani , B. Patricelli , A. Pe'er , G. Piano , G. Pühlhofer , M. Punch , O. Reimer , M. Ribó , G. Rodriguez , J. Rodriguez , P. Romano , G. Romeo , M. Roncadelli , G. Rowell , B. Rudak , I. Sadeh , F. Salesa Greus , F. G. Saturni , U. Sawangwit , M. Seglar-Arroyo , R. C. Shellard , H. Sol , R. Starling , T. Stolarczyk , G. Tagliaferri , F. Tavecchio , L. Tibaldo , V. Testa , S. Vercellone , A. Viana , J. Vink , V. Vitale , S. D. Vergani , S. Vorobiov , A. Wierzcholska , L. Yang , D. Zavrtanik , V. Zhdanov

The Large Area Telescope on the Fermi gamma-ray Space Telescope (FGST, ex-GLAST) provides unprecedented sensitivity for all-sky monitoring of gamma-ray activity. It is an adequate telescope to detect transient sources, since the observatory…

High Energy Astrophysical Phenomena · Physics 2010-08-25 Sylvain Chaty

Several classes of sources are known to emit different messengers. Among them, transient sources are a special case, due to their serendipitous occurrence, time variability and duration on different timescales. They are associated with…

There are the results of gamma-ray bursts observations obtained using the MASTER robotic telescope in 2007 - 2009. We observed 20 error-boxes of gamma-ray bursts this period.The limits on their optical brightnesses have been derived. There…

Gamma-ray Bursts (GRBs) are relativistic cosmological beacons of transient high energy radiation whose afterglows span the electromagnetic spectrum. Theoretical expectations of correlated neutrino emission position GRBs at an astrophysical…

High Energy Astrophysical Phenomena · Physics 2009-11-05 Michael Stamatikos

The High Altitude Water Cherenkov (HAWC) Observatory is a ground-based TeV gamma-ray observatory in the state of Puebla, Mexico at an altitude of 4100 m. Its 22,000 m$^2$ instrumented area, wide field of view ($\sim$2 sr), and >95% uptime…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Joshua Wood
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