Related papers: Gamma-Ray Bursts Detected From BATSE DISCLA Data

Analysis of the Swift Gamma-Ray Bursts duration

Two classes of gamma-ray bursts have been identified in the BATSE catalogs characterized by durations shorter and longer than about 2 seconds. There are, however, some indications for the existence of a third type of burst. Swift satellite…

High Energy Astrophysical Phenomena · Physics 2009-07-20 I. Horvath , L. G. Balazs , Z. Bagoly , J. Kelemen , P. Veres , G. Tusnady

Detection of a Millisecond Periodicity in BATSE Short Gamma-Ray Bursts

Coherent oscillations at kilohertz frequencies have recently been detected in a small number of gamma-ray bursts (GRBs), suggesting quasi-periodic dynamics in their central engines. A prominent example is GRB~230307A, which exhibited a…

High Energy Astrophysical Phenomena · Physics 2026-01-21 Run-Chao Chen , Jun Yang , Yi-Han Iris Yin , Bin-Bin Zhang

Search for gravitational-wave bursts associated with gamma-ray bursts using data from LIGO Science Run 5 and Virgo Science Run 1

We present the results of a search for gravitational-wave bursts associated with 137 gamma-ray bursts (GRBs) that were detected by satellite-based gamma-ray experiments during the fifth LIGO science run and first Virgo science run. The data…

High Energy Astrophysical Phenomena · Physics 2015-03-13 LIGO Scientific Collaboration , Virgo Collaboration , B. P. Abbott , R. Abbott , F. Acernese , R. Adhikari , P. Ajith , B. Allen , G. Allen , M. Alshourbagy , R. S. Amin , S. B. Anderson , W. G. Anderson , F. Antonucci , S. Aoudia , M. A. Arain , M. Araya , H. Armandula , P. Armor , K. G. Arun , Y. Aso , S. Aston , P. Astone , P. Aufmuth , C. Aulbert , S. Babak , P. Baker , G. Ballardin , S. Ballmer , C. Barker , D. Barker , F. Barone , B. Barr , P. Barriga , L. Barsotti , M. Barsuglia , M. A. Barton , I. Bartos , R. Bassiri , M. Bastarrika , Th. S. Bauer , B. Behnke , M. Beker , M. Benacquista , J. Betzwieser , P. T. Beyersdorf , S. Bigotta , I. A. Bilenko , G. Billingsley , S. Birindelli , R. Biswas , M. A. Bizouard , E. Black , J. K. Blackburn , L. Blackburn , D. Blair , B. Bland , C. Boccara , T. P. Bodiya , L. Bogue , F. Bondu , L. Bonelli , R. Bork , V. Boschi , S. Bose , L. Bosi , S. Braccini , C. Bradaschia , P. R. Brady , V. B. Braginsky , J. E. Brau , D. O. Bridges , A. Brillet , M. Brinkmann , V. Brisson , C. Van Den Broeck , A. F. Brooks , D. A. Brown , A. Brummit , G. Brunet , R. Budzyński , T. Bulik , A. Bullington , H. J. Bulten , A. Buonanno , O. Burmeister , D. Buskulic , R. L. Byer , L. Cadonati , G. Cagnoli , E. Calloni , J. B. Camp , E. Campagna , J. Cannizzo , K. C. Cannon , B. Canuel , J. Cao , F. Carbognani , L. Cardenas , S. Caride , G. Castaldi , S. Caudill , M. Cavaglià , F. Cavalier , R. Cavalieri , G. Cella , C. Cepeda , E. Cesarini , T. Chalermsongsak , E. Chalkley , P. Charlton , E. Chassande-Mottin , S. Chatterji , S. Chelkowski , Y. Chen , A. Chincarini , N. Christensen , C. T. Y. Chung , D. Clark , J. Clark , J. H. Clayton , F. Cleva , E. Coccia , T. Cokelaer , C. N. Colacino , J. Colas , A. Colla , M. Colombini , R. Conte , D. Cook , T. R. C. Corbitt , C. Corda , N. Cornish , A. Corsi , J. -P. Coulon , D. Coward , D. C. Coyne , J. D. E. Creighton , T. D. Creighton , A. M. Cruise , R. M. Culter , A. Cumming , L. Cunningham , E. Cuoco , S. L. Danilishin , S. D'Antonio , K. Danzmann , A. Dari , V. Dattilo , B. Daudert , M. Davier , G. Davies , E. J. Daw , R. Day , R. De Rosa , D. DeBra , J. Degallaix , M. del Prete , V. Dergachev , S. Desai , R. DeSalvo , S. Dhurandhar , L. Di Fiore , A. Di Lieto , M. Di Paolo Emilio , A. Di Virgilio , M. Díaz , A. Dietz , F. Donovan , K. L. Dooley , E. E. Doomes , M. Drago , R. W. P. Drever , J. Dueck , I. Duke , J. -C. Dumas , J. G. Dwyer , C. Echols , M. Edgar , M. Edwards , A. Effler , P. Ehrens , E. Espinoza , T. Etzel , M. Evans , T. Evans , V. Fafone , S. Fairhurst , Y. Faltas , Y. Fan , D. Fazi , H. Fehrmann , I. Ferrante , F. Fidecaro , L. S. Finn , I. Fiori , R. Flaminio , K. Flasch , S. Foley , C. Forrest , N. Fotopoulos , J. -D. Fournier , J. Franc , A. Franzen , S. Frasca , F. Frasconi , M. Frede , M. Frei , Z. Frei , A. Freise , R. Frey , T. Fricke , P. Fritschel , V. V. Frolov , M. Fyffe , V. Galdi , L. Gammaitoni , J. A. Garofoli , F. Garufi , G. Gemme , E. Genin , A. Gennai , I. Gholami , J. A. Giaime , S. Giampanis , K. D. Giardina , A. Giazotto , K. Goda , E. Goetz , L. M. Goggin , G. González , M. L. Gorodetsky , S. Goeßzetler , S. Goßler , R. Gouaty , M. Granata , V. Granata , A. Grant , S. Gras , C. Gray , M. Gray , R. J. S. Greenhalgh , A. M. Gretarsson , C. Greverie , F. Grimaldi , R. Grosso , H. Grote , S. Grunewald , M. Guenther , G. Guidi , E. K. Gustafson , R. Gustafson , B. Hage , J. M. Hallam , D. Hammer , G. D. Hammond , C. Hanna , J. Hanson , J. Harms , G. M. Harry , I. W. Harry , E. D. Harstad , K. Haughian , K. Hayama , J. Heefner , H. Heitmann , P. Hello , I. S. Heng , A. Heptonstall , M. Hewitson , S. Hild , E. Hirose , D. Hoak , K. A. Hodge , K. Holt , D. J. Hosken , J. Hough , D. Hoyland , D. Huet , B. Hughey , S. H. Huttner , D. R. Ingram , T. Isogai , M. Ito , A. Ivanov , P. Jaranowski , B. Johnson , W. W. Johnson , D. I. Jones , G. Jones , R. Jones , L. Sancho de la Jordana , L. Ju , P. Kalmus , V. Kalogera , S. Kandhasamy , J. Kanner , D. Kasprzyk , E. Katsavounidis , K. Kawabe , S. Kawamura , F. Kawazoe , W. Kells , D. G. Keppel , A. Khalaidovski , F. Y. Khalili , R. Khan , E. Khazanov , P. King , J. S. Kissel , S. Klimenko , K. Kokeyama , V. Kondrashov , R. Kopparapu , S. Koranda , I. Kowalska , D. Kozak , B. Krishnan , A. Królak , R. Kumar , P. Kwee , P. La Penna , P. K. Lam , M. Landry , B. Lantz , A. Lazzarini , H. Lei , M. Lei , N. Leindecker , I. Leonor , N. Leroy , N. Letendre , C. Li , H. Lin , P. E. Lindquist , T. B. Littenberg , N. A. Lockerbie , D. Lodhia , M. Longo , M. Lorenzini , V. Loriette , M. Lormand , G. Losurdo , P. Lu , M. Lubinski , A. Lucianetti , H. Lück , B. Machenschalk , M. MacInnis , J. -M. Mackowski , M. Mageswaran , K. Mailand , E. Majorana , N. Man , I. Mandel , V. Mandic , M. Mantovani , F. Marchesoni , F. Marion , S. Márka , Z. Márka , A. Markosyan , J. Markowitz , E. Maros , J. Marque , F. Martelli , I. W. Martin , R. M. Martin , J. N. Marx , K. Mason , A. Masserot , F. Matichard , L. Matone , R. A. Matzner , N. Mavalvala , R. McCarthy , D. E. McClelland , S. C. McGuire , M. McHugh , G. McIntyre , D. J. A. McKechan , K. McKenzie , M. Mehmet , A. Melatos , A. C. Melissinos , G. Mendell , D. F. Menéndez , F. Menzinger , R. A. Mercer , S. Meshkov , C. Messenger , M. S. Meyer , C. Michel , L. Milano , J. Miller , J. Minelli , Y. Minenkov , Y. Mino , V. P. Mitrofanov , G. Mitselmakher , R. Mittleman , O. Miyakawa , B. Moe , M. Mohan , S. D. Mohanty , S. R. P. Mohapatra , J. Moreau , G. Moreno , N. Morgado , A. Morgia , T. Morioka , K. Mors , S. Mosca , V. Moscatelli , K. Mossavi , B. Mours , C. MowLowry , G. Mueller , D. Muhammad , H. zur Mühlen , S. Mukherjee , H. Mukhopadhyay , A. Mullavey , H. Müller-Ebhardt , J. Munch , P. G. Murray , E. Myers , J. Myers , T. Nash , J. Nelson , I. Neri , G. Newton , A. Nishizawa , F. Nocera , K. Numata , E. Ochsner , J. O'Dell , G. H. Ogin , B. O'Reilly , R. O'Shaughnessy , D. J. Ottaway , R. S. Ottens , H. Overmier , B. J. Owen , G. Pagliaroli , C. Palomba , Y. Pan , C. Pankow , F. Paoletti , M. A. Papa , V. Parameshwaraiah , S. Pardi , A. Pasqualetti , R. Passaquieti , D. Passuello , P. Patel , M. Pedraza , S. Penn , A. Perreca , G. Persichetti , M. Pichot , F. Piergiovanni , V. Pierro , M. Pietka , L. Pinard , I. M. Pinto , M. Pitkin , H. J. Pletsch , M. V. Plissi , R. Poggiani , F. Postiglione , M. Prato , M. Principe , R. Prix , G. A. Prodi , L. Prokhorov , O. Punken , M. Punturo , P. Puppo , V. Quetschke , F. J. Raab , O. Rabaste , D. S. Rabeling , H. Radkins , P. Raffai , Z. Raics , N. Rainer , M. Rakhmanov , P. Rapagnani , V. Raymond , V. Re , C. M. Reed , T. Reed , T. Regimbau , H. Rehbein , S. Reid , D. H. Reitze , F. Ricci , R. Riesen , K. Riles , B. Rivera , P. Roberts , N. A. Robertson , F. Robinet , C. Robinson , E. L. Robinson , A. Rocchi , S. Roddy , L. Rolland , J. Rollins , J. D. Romano , R. Romano , J. H. Romie , D. Rosińska , C. Röver , S. Rowan , A. Rüdiger , P. Ruggi , P. Russell , K. Ryan , S. Sakata , F. Salemi , V. Sandberg , V. Sannibale , L. Santamaría , S. Saraf , P. Sarin , B. Sassolas , B. S. Sathyaprakash , S. Sato , M. Satterthwaite , P. R. Saulson , R. Savage , P. Savov , M. Scanlan , R. Schilling , R. Schnabel , R. Schofield , B. Schulz , B. F. Schutz , P. Schwinberg , J. Scott , S. M. Scott , A. C. Searle , B. Sears , F. Seifert , D. Sellers , A. S. Sengupta , D. Sentenac , A. Sergeev , B. Shapiro , P. Shawhan , D. H. Shoemaker , A. Sibley , X. Siemens , D. Sigg , S. Sinha , A. M. Sintes , B. J. J. Slagmolen , J. Slutsky , M. V. van der Sluys , J. R. Smith , M. R. Smith , N. D. Smith , K. Somiya , B. Sorazu , A. Stein , L. C. Stein , S. Steplewski , A. Stochino , R. Stone , K. A. Strain , S. Strigin , A. Stroeer , R. Sturani , A. L. Stuver , T. Z. Summerscales , K. -X. Sun , M. Sung , Patrick J. Sutton , B. Swinkels , G. P. Szokoly , D. Talukder , L. Tang , D. B. Tanner , S. P. Tarabrin , J. R. Taylor , R. Taylor , R. Terenzi , J. Thacker , K. A. Thorne , K. S. Thorne , A. Thüring , K. V. Tokmakov , A. Toncelli , M. Tonelli , C. Torres , C. Torrie , E. Tournefier , F. Travasso , G. Traylor , M. Trias , J. Trummer , D. Ugolini , J. Ulmen , K. Urbanek , H. Vahlbruch , G. Vajente , M. Vallisneri , J. F. J. van den Brand , S. van der Putten , S. Vass , R. Vaulin , M. Vavoulidis , A. Vecchio , G. Vedovato , A. A. van Veggel , J. Veitch , P. Veitch , C. Veltkamp , D. Verkindt , F. Vetrano , A. Viceré , A. Villar , J. -Y. Vinet , H. Vocca , C. Vorvick , S. P. Vyachanin , S. J. Waldman , L. Wallace , R. L. Ward , M. Was , A. Weidner , M. Weinert , A. J. Weinstein , R. Weiss , L. Wen , S. Wen , K. Wette , J. T. Whelan , S. E. Whitcomb , B. F. Whiting , C. Wilkinson , P. A. Willems , H. R. Williams , L. Williams , B. Willke , I. Wilmut , L. Winkelmann , W. Winkler , C. C. Wipf , A. G. Wiseman , G. Woan , R. Wooley , J. Worden , W. Wu , I. Yakushin , H. Yamamoto , Z. Yan , S. Yoshida , M. Yvert , M. Zanolin , J. Zhang , L. Zhang , C. Zhao , N. Zotov , M. E. Zucker , J. Zweizig

Investigation of Redshift- and Duration-Dependent Clustering of Gamma-ray Bursts

Gamma-ray bursts (GRBs) are detectable out to very large distances and as such are potentially powerful cosmological probes. Historically, the angular distribution of GRBs provided important information about their origin and physical…

High Energy Astrophysical Phenomena · Physics 2015-11-11 T. N. Ukwatta , P. R. Wozniak

Gamma Ray Bursts

Gamma-ray bursts (GRBs) are bright flashes of gamma-rays coming from the cosmos. They occur roughly once per day, last typically 10s of seconds and are the most luminous events in the universe. More than three decades after their discovery,…

High Energy Astrophysical Phenomena · Physics 2012-09-03 Neil Gehrels , Peter Meszaros

GRB010921: Localization and Observations by the HETE Satellite

On September 21 at 18950.56 SOD (05:15:50.56) UT the FREGATE gamma-ray instrument on the High Energy Transient Explorer (HETE) detected a bright gamma-ray burst (GRB). The burst was also seen by the X-detector on the WXM X-ray instrument…

Astrophysics · Physics 2007-05-23 G. Ricker , K. Hurley , D. Lamb , S. Woosley , J-L Atteia , N. Kawai , R. Vanderspek , G. Crew , J. Doty , J. Villasenor , G. Prigozhin , G. Monnelly , N. Butler , M. Matsuoka , Y. Shirasaki , T. Tamagawa , K. Torii , T. Sakamoto , A. Yoshida , E. Fenimore , M. Galassi , T. Tavenner , T. Donaghy , C. Graziani , M. Boer , J-P Dezalay , M. Niel , J-F Olive , G. Vedrenne , T. Cline , J. G. Jernigan , A. Levine , F. Martel , E. Morgan , J. Braga , R. Manchanda , G. Pizzichini , K. Takagishi , M. Yamauchi

A Search for Ultra-High Energy Counterparts to Gamma-Ray Bursts

A small air shower array operating over many years has been used to search for ultra-high energy (UHE) gamma radiation ($\geq 50$ TeV) associated with gamma-ray bursts (GRBs) detected by the BATSE instrument on the Compton Gamma-Ray…

Astrophysics · Physics 2009-10-28 S. P. Plunkett , M. Delaney , B. McBreen , K. J. Hurley , C. T. O'Sullivan

The Statistics of Gamma Ray Burst Lensing

Possibly the only unambiguous verification that gamma-ray bursts (GRBs) are at cosmological distances would be the observation of multiple images of a gravitationally lensed burst. Each images would arrive at a different time, but exhibit…

Astrophysics · Physics 2009-10-22 S. A. Grossman , M. A. Nowak

BATSE Observations of the Large-Scale Isotropy of Gamma-Ray Bursts

We use dipole and quadrupole statistics to test the large-scale isotropy of the first 1005 gamma-ray bursts observed by the Burst and Transient Source Experiment (BATSE). In addition to the entire sample of 1005 gamma-ray bursts, many…

Astrophysics · Physics 2009-10-28 Michael S. Briggs , William S. Paciesas , Geoffrey N. Pendleton , Charles A. Meegan , Gerald J. Fishman , John M. Horack , Martin Brock , Chryssa Kouveliotou , Dieter H. Hartmann , Jon Hakkila

The Fermi GBM Gamma-Ray Burst Spectral Catalog: 10 Years of Data

We present the systematic spectral analyses of gamma-ray bursts (GRBs) detected by the Fermi Gamma-Ray Burst Monitor (GBM) during its first ten years of operation. This catalog contains two types of spectra; time-integrated spectral fits…

High Energy Astrophysical Phenomena · Physics 2021-06-02 S. Poolakkil , R. Preece , C. Fletcher , A. Goldstein , P. N. Bhat , E. Bissaldi , M. S. Briggs , E. Burns , W. H. Cleveland , M. M. Giles , C. M. Hui , D. Kocevski , S. Lesage , B. Mailyan , C. Malacaria , W. S. Paciesas , O. J. Roberts , P. Veres , A. von Kienlin , C. A. Wilson-Hodge

High energy gamma-ray emission from Gamma-Ray Bursts -- before GLAST

Gamma-ray bursts (GRBs) are short and intense emission of soft gamma-rays, which have fascinated astronomers and astrophysicists since their unexpected discovery in 1960s. The X-ray/optical/radio afterglow observations confirm the…

Astrophysics · Physics 2009-05-07 Yi-Zhong Fan , Tsvi Piran

X-Ray Light Curves of Gamma-ray Bursts Detected with the All-Sky Monitor on RXTE

We present X-ray light curves (1.5-12 keV) for fifteen gamma-ray bursts (GRBs) detected by the All-Sky Monitor on the Rossi X-ray Timing Explorer. We compare these soft X-ray light curves with count rate histories obtained by the…

Astrophysics · Physics 2009-11-06 D. A. Smith , A. Levine , H. Bradt , K. Hurley , M. Feroci , P. Butterworth , S. Golenetskii , G. Pendleton , S. Phengchamnan

Gamma-Ray Bursts from Extragalactic Magnetar Flares

The prototype for events that we call MFs - "March Fifth" events or "Magnetar Flares" - was observed on March 5, 1979. There is evidence that MFs are powered by catastrophic magnetic instabilities in ultramagnetized neutron stars. These…

Astrophysics · Physics 2009-11-06 Robert C. Duncan

Observation of GRBs with AGILE

Since its early phases of operation, the AGILE satellite is observing Gamma Ray Bursts (GRBs) over an energy range potentially spanning six orders of magnitude. In the hard X-ray band the SuperAGILE imager provides localization of about one…

High Energy Astrophysical Phenomena · Physics 2009-06-09 M. Marisaldi , G. Barbiellini , E. Costa , S. Cutini , E. Del Monte , I. Donnarumma , Y. Evangelista , M. Feroci , F. Fuschino , M. Galli , A. Giuliani , C. Labanti , I. Lapshov , F. Lazzarotto , P. Lipari , F. Longo , S. Mereghetti , E. Moretti , L. Pacciani , M. Rapisarda , P. Soffitta , M. Tavani , M. Trifoglio , S. Vercellone

Gamma-Ray Bursts are Produced Predominately in the Early Universe

It is known that some observed gamma-ray bursts (GRBs) are produced at cosmological distances and that the GRB production rate may follow the star formation rate. We model the BATSE-detected intensity distribution of long GRBs in order to…

Astrophysics · Physics 2007-05-23 J. R. Lin , S. N. Zhang , T. P. Li

Gamma-ray Bursts

Gamma-ray bursts are flashes of high-energy radiation lasting from a fraction of a second to several hours. Military satellites made the first detections of GRBs in the late 1960s. The $\gamma$-ray emission forms from shocks in a…

High Energy Astrophysical Phenomena · Physics 2025-10-08 Andrew J. Levan

A Search for Prompt Very High Energy Emission from Satellite-detected Gamma-ray Bursts using Milagro

Gamma-ray bursts (GRBs) have been detected up to GeV energies and are predicted by many models to emit in the very high energy (VHE, > 100 GeV) regime too. Detection of such emission would allow us to constrain GRB models. Since its launch,…

Astrophysics · Physics 2007-10-15 Milagro Collaboration , P. M. Saz Parkinson , B. L. Dingus

Gamma-Ray Spectra & Variability of the Crab Nebula Emission Observed by BATSE

We report ~ 600 days of BATSE earth-occultation observations of the total gamma-ray (30 keV to 1.7 MeV) emission from the Crab nebula, between 1991 May 24 (TJD 8400) and 1994 October 2 (TJD 9627). Lightcurves from 35-100, 100-200, 200-300,…

Astrophysics · Physics 2009-11-10 J. C. Ling , Wm. A. Wheaton

Gamma-Ray Burst observations with Fermi

After seven years of science operation, the Fermi mission has brought great advances in the study of Gamma-ray Bursts (GRBs). Over 1600 GRBs have been detected by the Gamma-ray Burst Monitor, and more than 100 of these are also detected by…

High Energy Astrophysical Phenomena · Physics 2015-07-19 Elisabetta Bissaldi , Francesco Longo , Nicola Omodei , Giacomo Vianello , Andreas von Kienlin

Average power density spectrum of Swift long gamma-ray bursts in the observer and in the source rest frames

We calculate the average power density spectra (PDS) of 244 long gamma-ray bursts detected with the Swift Burst Alert Telescope in the 15-150 keV band from January 2005 to August 2011. For the first time we derived the average PDS in the…

High Energy Astrophysical Phenomena · Physics 2015-06-04 C. Guidorzi , R. Margutti , L. Amati , S. Campana , M. Orlandini , P. Romano , M. Stamatikos , G. Tagliaferri