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This paper discusses Swift observations of the gamma-ray burst GRB 050315 (z=1.949) from 80 s to 10 days after the onset of the burst. The X-ray light curve displayed a steep early decay (t^-5) for ~200 s and several breaks. However, both…

We report on the temporal and spectral characteristics of the early X-ray emission from the Gamma Ray Burst 051117A as observed by Swift. The superb quality of the early X-ray light-curve and spectra of this source, one of the brightest…

The gamma-ray burst (GRB) 221009A, with its extreme brightness, has provided the opportunity to explore GRB prompt and afterglow emission behavior on short time scales with high statistics. In conjunction with detection up to very…

High Energy Astrophysical Phenomena · Physics 2023-08-30 James Rodi , Pietro Ubertini

BAT and XRT observations of two recent well-covered GRBs observed by Swift, GRB 050315 and GRB 050319, show clearly a prompt component joining the onset of the afterglow emission. By fitting a power law form to the gamma-ray spectrum, we…

We present observations of the unusually bright and long gamma-ray burst GRB 050820A, one of the best-sampled broadband data sets in the Swift era. The gamma-ray light curve is marked by a soft precursor pulse some 200 s before the main…

We analyze the Swift XRT light curves and spectra of the gamma-ray bursts (GRBs) for which the redshift has been measured. The sample consists of seven GRBs. The soft X-ray light curves of all these GRBs are separated into at least two…

The early optical emission of the moderately high redshift ($z=3.08$) GRB 060607A shows a remarkable broad and strong peak with a rapid rise and a relatively slow power-law decay. It is not coincident with the strong early-time flares seen…

We report the results of Swift observations of the Gamma Ray Burst GRB 050603. With a V magnitude V=18.2 about 10 hours after the burst the optical afterglow was the brightest so far detected by Swift and one of the brightest optical…

The gamma-ray burst GRB 180720B is very peculiar. On one hand, some interesting features have been found by performing the detailed time-resolved spectral analysis in the prompt phase. First, the `flux-tracking' pattern is exhibited both…

High Energy Astrophysical Phenomena · Physics 2019-12-24 Ming-Ya Duan , Xiang-Gao Wang

We report on the observations of gamma-ray burst (GRB) 190114C by the Fermi Gamma-ray Space Telescope and the Neil Gehrels Swift Observatory. The early-time observations reveal multiple emission components that evolve independently, with a…

High Energy Astrophysical Phenomena · Physics 2020-02-19 M. Ajello , M. Arimoto , M. Axelsson , L. Baldini , G. Barbiellini , D. Bastieri , R. Bellazzini , A. Berretta , E. Bissaldi , R. D. Blandford , R. Bonino , E. Bottacini , J. Bregeon , P. Bruel , R. Buehler , E. Burns , S. Buson , R. A. Cameron , R. Caputo , P. A. Caraveo , E. Cavazzuti , S. Chen , G. Chiaro , S. Ciprini , J. Cohen-Tanugi , D. Costantin , S. Cutini , F. D'Ammando , M. DeKlotz , P. de la Torre Luque , F. de Palma , A. Desai , N. Di Lalla , L. Di Venere , F. Fana Dirirsa , S. J. Fegan , A. Franckowiak , Y. Fukazawa , S. Funk , P. Fusco , F. Gargano , D. Gasparrini , N. Giglietto , R. Gill , F. Giordano , M. Giroletti , J. Granot , D. Green , I. A. Grenier , M. H. Grondin , S. Guiriec , E. Hays , D. Horan , G. Jóhannesson , D. Kocevski , M. Kovac'evic' , M. Kuss , S. Larsson , L. Latronico , M. Lemoine-Goumard , J. Li , I. Liodakis , F. Longo , F. Loparco , M. N. Lovellette , P. Lubrano , S. Maldera , D. Malyshev , A. Manfreda , G. Martí-Devesa , M. N. Mazziotta , J. E. McEnery , I. Mereu , M. Meyer , P. F. Michelson , W. Mitthumsiri , T. Mizuno , M. E. Monzani , E. Moretti , A. Morselli , I. V. Moskalenko , M. Negro , E. Nuss , N. Omodei , M. Orienti , E. Orlando , M. Palatiello , V. S. Paliya , D. Paneque , Z. Pei , M. Persic , M. Pesce-Rollins , V. Petrosian , F. Piron , H. Poon , T. A. Porter , G. Principe , J. L. Racusin , S. Rainò , R. Rando , B. Rani , M. Razzano , S. Razzaque , A. Reimer , O. Reimer , F. Ryde , P. M. Saz Parkinson , D. Serini , C. Sgrò , E. J. Siskind , G. Spandre , P. Spinelli , H. Tajima , K. Takagi , M. N. Takahashi , D. Tak , J. B. Thayer , D. J. Thompson , D. F. Torres , E. Troja , J. Valverde , B. Van Klaveren , K. Wood , M. Yassine , G. Zaharijas , P. N. Bhat , M. S. Briggs , W. Cleveland , M. Giles , A. Goldstein , M. Hui , C. Malacaria , R. Preece , O. Roberts , P. Veres , A. von Kienlin , S. B. Cenko , P. O'Brien , A. P. Beardmore , A. Lien , J. P. Osborne , A. Tohuvavohu , V. D'Elia , A. D'A , M. Perri , J. Gropp , N. Klingler , M. Capalbi , G. Tagliaferri , M. Stamatikos

The robotic ROTSE-III telescope network detected prompt optical emission contemporaneous with the gamma-ray emission of Swift events GRB051109A and GRB051111. Both datasets have continuous coverage at high signal-to-noise levels from the…

We present and discuss the results of an extensive observational campaign devoted to GRB071010A, a long-duration gamma-ray burst detected by the Swift satellite. This event was followed for almost a month in the optical/near-infrared (NIR)…

Using the Swift data of GRB 050315, we progress on the uniqueness of our theoretically predicted Gamma-Ray Burst (GRB) structure as composed by a proper-GRB (P-GRB), emitted at the transparency of an electron-positron plasma with suitable…

Swift discovered XRF 050416A with the BAT and began observing it with its narrow field instruments only 64.5 s after the burst onset. Its very soft spectrum classifies this event as an X-ray flash. The afterglow X-ray emission was monitored…

We have conducted a thorough and blind search for emission lines in >70 Swift X-ray afterglows of total exposure ~10^7s. We find that most afterglows are consistent with pure power-laws plus extinction. Significant outliers to the…

Astrophysics · Physics 2008-11-26 Nathaniel R. Butler

We present a multi-wavelength study of GRB 081008, at redshift 1.967, by Swift, ROTSE-III and GROND. Compared to other Swift GRBs, GRB 081008 has a typical gamma-ray isotropic equivalent energy output (10^53 erg) during the prompt phase,…

The unique capability of the Swift satellite to perform a prompt and autonomous slew to a newly detected Gamma-Ray Burst (GRB) has yielded the discovery of interesting new properties of GRB X-ray afterglows, such as the steep early…

When a massive star explodes as a Gamma Ray Burst information about this explosion is retained in the properties of the prompt and afterglow emission. We report on new relationships between the prompt and X-ray afterglow emission of…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Dirk Grupe , John A. Nousek , Peter Veres , Binbin Zhang , Neil Gehrels

We review the fireball shock model of gamma-ray burst prompt and early afterglow emission in light of rapid follow-up measurements made and enabled by the multi-wavelength Swift satellite. These observations are leading to a reappraisal and…

Astrophysics · Physics 2007-05-23 D. B. Fox , P. Meszaros