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After more than 40 years from their discovery, the long-lasting tension between predictions and observations of GRBs prompt emission spectra starts to be solved. We found that the observed spectra can be produced by the synchrotron process,…

High Energy Astrophysical Phenomena · Physics 2020-03-25 Maria Edvige Ravasio

We address the problem of parameter estimation for degenerate diffusion processes defined via the solution of Stochastic Differential Equations (SDEs) with diffusion matrix that is not full-rank. For this class of hypo-elliptic diffusions…

Statistics Theory · Mathematics 2024-09-04 Yuga Iguchi , Alexandros Beskos

Lattice models are crucial for studying thermodynamic properties in many physical, biological and chemical systems. We investigate Lattice Restricted Primitive Model (LRPM) of electrolytes with different discretization parameters in order…

Statistical Mechanics · Physics 2009-11-11 Maxim N. Artyomov , Anatoly B. Kolomeisky

The Gamma Ray Burst (GRB) 180720B is one of the brightest events detected by the Fermi satellite and the first GRB detected by the H.E.S.S. telescope above 100 GeV. We analyse the Fermi (GBM and LAT) and Swift (XRT and BAT) data and…

High Energy Astrophysical Phenomena · Physics 2020-04-22 M. Ronchi , F. Fumagalli , M. E. Ravasio , G. Oganesyan , M. Toffano , O. S. Salafia , L. Nava , S. Ascenzi , G. Ghirlanda , G. Ghisellini

Modern accelerator front ends almost exclusively include radio-frequency quadrupoles for initial capture and focusing of the low-energy beam. Dynamics in the RFQ define the longitudinal bunch parameters. Simulation of the SNS RFQ with…

Accelerator Physics · Physics 2021-01-04 K. Ruisard , A. Aleksandrov , S. Cousineau , A. Shishlo , V. Tzoganis , A. Zhukov

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

We have carried out a systematic analysis of the gamma-ray bursts' (GRBs) light curves detected in the SPI-ACS experiment onboard the INTEGRAL observatory aimed to search extended emission. The emission occasionally recorded after the…

High Energy Astrophysical Phenomena · Physics 2023-09-07 G. Yu. Mozgunov , P. Yu. Minaev , A. S. Pozanenko

The GLAST-AGILE Support Program (GASP) of the Whole Earth Blazar Telescope (WEBT) monitored BL Lacertae in 2008-2009 at radio, near-IR, and optical frequencies. During this period, high-energy observations were performed by XMM-Newton,…

The decay behavior of the specific intensity is studied for the spatial-frequency domain imaging (SFDI). It is shown using the radiative transport equation that the decay is given by a superposition of different decay modes, and the decay…

Optics · Physics 2022-08-19 Manabu Machida , Yoko Hoshi , Keiichiro Kagawa , Kazuki Takada

The dissipation of energy flux in blazar jets plays a key role in the acceleration of relativistic particles. Two possibilities are commonly considered for the dissipation processes, magnetic reconnection -- possibly triggered by…

High Energy Astrophysical Phenomena · Physics 2018-06-13 F. Tavecchio , M. Landoni , L. Sironi , P. Coppi

The recent launches of the Einstein Probe (EP) and the Space Variable Objects Monitor (SVOM) mission have led to the detection of a growing number of long GRBs with significant, early soft X-ray flux during their gamma-ray emission,…

High Energy Astrophysical Phenomena · Physics 2025-10-21 Ziming Wang , Chenyu Wang , He Gao , Hua Feng , An Li , Lin Lin , Songyu Shen

The detection of flares with the Swift satellite triggered a lot of bservational and theoretical interest in these phenomena. As a consequence a large analysis effort started within the community to characterize the phenomenon and at the…

We report high-resolution spectroscopy of 125 field stars previously observed as part of the Sloan Digital Sky Survey and its program for Galactic studies, the Sloan Extension for Galactic Understanding and Exploration (SEGUE). These…

Damped Lyman-$\alpha$ Absorber(DLA) of HI 21cm system is an ideal probe to directly measure cosmic acceleration in real-time cosmology via Sandage-Loeb(SL) test. During short observations toward two DLAs in the commissioning progress of…

Cosmology and Nongalactic Astrophysics · Physics 2023-03-31 Chang-Zhi Lu , Kang Jiao , Tingting Zhang , Tong-Jie Zhang , Ming Zhu

We test the models of synchrotron emission presented in Part I of this series (Lloyd & Petrosian, these proceedings) against the distributions and evolution of GRB spectral parameters (particularly the low energy index, $\alpha$). With…

Astrophysics · Physics 2018-11-06 Nicole M. Lloyd-Ronning , Vahe' Petrosian , Robert D. Preece

Convergence in high-probability (HP) has attracted increasing interest, due to implying exponentially decaying tail bounds and strong guarantees for individual runs of an algorithm. While many works study HP guarantees in centralized…

Machine Learning · Computer Science 2026-05-22 Aleksandar Armacki , Ali H. Sayed

We present an analysis of four epochs of H$\alpha$ and [S II] $\lambda\lambda$ 6716/6731 HST images of HH 1. For determining proper motions we explore a new method based on analysis of spatially degraded images obtained convolving the…

Astrophysics of Galaxies · Physics 2016-04-27 A. C. Raga , B. Reipurth , A. Esquivel , J. Bally

The origin of the prompt high-energy ($>100$MeV) emission of Gamma-ray Bursts (GRBs), detected by the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope, is still under debate, for which both the external shock origin…

High Energy Astrophysical Phenomena · Physics 2017-07-27 Qing-Wen Tang , Xiang-Yu Wang , Ruo-Yu Liu
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