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Related papers: The Fluence Duration Bias

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If $\gamma$-ray bursts are at cosmological distances, then not only their constituent pulses but also the intervals between pulses should be time-dilated. Unlike time-dilation measures of pulse emission, intervals would appear to require…

Astrophysics · Physics 2009-10-28 J. P. Norris , J. T. Bonnell , R. J. Nemiroff , J. D. Scargle

We predict the redshift distribution of long Gamma-Ray Bursts (GRBs) with Monte Carlo simulations. Our improved analysis constrains free parameters with three kinds of observation: (i) the log(N)-log(P) diagram of BATSE bursts; (ii) the…

Astrophysics · Physics 2008-11-26 F. Daigne , E. M. Rossi , R. Mochkovitch

A recent work has found a tight global relation between the GRB prompt fluence, peak flux (based on the optimum time scale determined from the Bayesian Blocks-based analysis) and duration using data from the Fermi Gamma-Ray burst monitor,…

High Energy Astrophysical Phenomena · Physics 2022-06-17 S. Pradyumna , Shantanu Desai

We present an updated catalog of 113 X-ray flares detected by Swift in the ~33% of the X-ray afterglows of Gamma-Ray Bursts (GRB). 43 flares have a measured redshift. For the first time the analysis is performed in 4 different X-ray energy…

High Energy Astrophysical Phenomena · Physics 2015-05-18 G. Chincarini , J. Mao , R. Margutti , M. G. Bernardini , C. Guidorzi , F. Pasotti , D. Giannios , M. Della Valle , A. Moretti , P. Romano , P. D'Avanzo , G. Cusumano , P. Giommi

Two dimensional turbulence has a remarkable tendency to self-organize into large, coherent structures, forming a mean flow. The purpose of this paper is to elucidate how these structures are sustained, and what determines them and the…

Fluid Dynamics · Physics 2018-02-05 Anna Frishman

We report detections of fast radio bursts (FRBs) from the repeating source FRB 20201124A with Apertif/WSRT and GMRT, and measurements of basic burst properties, especially the dispersion measure (DM) and fluence. Based on comparisons of…

High Energy Astrophysical Phenomena · Physics 2025-04-23 A. V. Bilous , J. van Leeuwen , Y. Maan , I. Pastor-Marazuela , L. C. Oostrum , K. M. Rajwade , Y. Y. Wang

A bright burst, followed by an X-ray tail lasting ~10 ks, was detected during an XMM-Newton observation of the magnetar 1E 1547.0-5408 carried out on 2009 February 3. The burst, also observed by SWIFT/BAT, had a spectrum well fit by the sum…

High Energy Astrophysical Phenomena · Physics 2017-03-22 Fabio Pintore , Sandro Mereghetti , Andrea Tiengo , Giacomo Vianello , Elisa Costantini , Paolo Esposito

The number of classes of gamma-ray bursts (GRBs), besides the well-established short and long ones, remains a debatable issue. It was already shown, however, that when invoking skewed distributions, the $\log T_{90}$ and $\log T_{90} - \log…

High Energy Astrophysical Phenomena · Physics 2020-01-08 Mariusz Tarnopolski

We study the fluence distributions of over 3040 bursts from SGR 1806-20 and over 1963 bursts from SGR 1900+14 using the complete set of observations available from the Rossi X-Ray Timing Explorer/Proportional Counter Array through March…

High Energy Astrophysical Phenomena · Physics 2012-07-03 Zachary Prieskorn , Philip Kaaret

I compare the burst detection sensitivity of CGRO's BATSE, Swift's BAT, the GLAST Burst Monitor (GBM) and EXIST as a function of a burst's spectrum and duration. A detector's overall burst sensitivity depends on its energy sensitivity and…

Astrophysics · Physics 2009-11-11 David L. Band

Gamma-Ray Bursts have been observed out to very high redshifts and provide time measures that are directly related to intrinsic time scales of the burst. Einstein's theory of relativity is quite definite that if the universe is expanding…

General Physics · Physics 2010-09-12 David F. Crawford

Flux penetrations into three-dimensional Nb superconducting strip arrays, where two layers of strip arrays are stacked by shifting a half period, are studied using a magneto-optical imaging method. Flux avalanches are observed when the…

Superconductivity · Physics 2013-07-25 Y. Tsuchiya , Y. Mawatari , J. Ibuka , S. Tada , S. Pyon , S. Nagasawa , M. Hidaka , M. Maezawa , T. Tamegai

The use of the annual maximum series for flood frequency analyses limits the considered information to one event per year and one sample that is assumed to be homogeneous. However, flood may have different generating processes, such as…

Applications · Statistics 2021-11-29 Svenja Fischer

Wall turbulence has a sublayer where the mean wall-normal flux of the streamwise momentum is constant. Via the law of the wall, this mean flux is related to the wall-normal profile of the mean streamwise velocity. However, the momentum flux…

Fluid Dynamics · Physics 2023-07-10 H. Mouri , J. Ito

From Galactic binary sources, to extragalactic magnetized neutron stars, to long-duration GRBs without associated supernovae, the types of sources we now believe capable of producing bursts of gamma-rays continues to grow apace. With this…

Astrophysics · Physics 2009-06-23 Joshua S. Bloom , Nathaniel R. Butler , Daniel A. Perley

We report on the temporal behavior of the high-energy power law continuum component of gamma-ray burst spectra with data obtained by the Burst and Transient Source Experiment. We have selected 126 high fluence and high flux bursts from the…

We report our discovery in Swift satellite data of a transient gamma-ray counterpart (3.2$\sigma$ confidence) to the fast radio burst FRB131104, the first such counterpart to any FRB. The transient has duration $T_{90} \gtrsim 100$s and…

High Energy Astrophysical Phenomena · Physics 2022-02-09 J. J. DeLaunay , D. B. Fox , K. Murase , P. Mészáros , A. Keivani , C. Messick , M. A. Mostafá , F. Oikonomou , G. Tešić , C. F. Turley

We study the distribution of the durations of gamma-ray bursts (GRBs) in the unified model of short and long GRBs recently proposed by Yamazaki, Ioka, and Nakamura. Monte Carlo simulations show clear bimodal distributions, with…

Astrophysics · Physics 2009-11-10 Kenji Toma , Ryo Yamazaki , Takashi Nakamura

The observed log-normal flux distributions in the high energy emission from blazars have been interpreted as being due to variability stemming from non-linear multiplicative processes generated dynamically from the accretion disc. On the…

High Energy Astrophysical Phenomena · Physics 2018-07-26 Atreyee Sinha , Rukaiya Khatoon , Ranjeev Misra , Sunder Sahayanathan , Soma Mandal , Rupjyoti Gogoi , Nilay Bhatt

In this note, we critically discuss the issue of the possible finiteness of the turbulence lifetime in subcritical transition to turbulence in shear flows, which attracted a lot of interest recently. We briefly review recent experimental…

Soft Condensed Matter · Physics 2015-06-04 Olivier Dauchot , Eric Bertin
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