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X-ray flashes (XRFs) are a class of high-energy transients whose nature is still open to question. Similar in many aspects to common gamma-ray bursts (GRBs), their strong X-ray emission is accompanied by very low or absent emission in the…

High Energy Astrophysical Phenomena · Physics 2016-10-18 Riccardo Ciolfi

INTEGRAL monitoring of the Galactic Plane is revealing a growing number of recurrent X-ray transients, characterised by short outbursts with very fast rise times (~ tens of minutes) and typical durations of a few hours. Here we show that…

Twenty-two extragalactic fast X-ray transients (FXTs) have now been discovered from two decades of Chandra data (analyzing ~259 Ms of data), with 17 associated with distant galaxies (>100 Mpc). Different mechanisms and progenitors have been…

High Energy Astrophysical Phenomena · Physics 2024-01-04 J. Quirola-Vásquez , F. E. Bauer , P. G. Jonker , W. N. Brandt , D. Eappachen , A. J. Levan , E. Lopez , B. Luo , M. E. Ravasio , H. Sun , Y. Q. Xue , G. Yang , X. C. Zheng

Fast X-ray transients (FXRTs) are short-lived X-ray outbursts with diverse progenitor scenarios, including compact object mergers, stellar core-collapses and tidal disruption events. The Einstein Probe (EP) has enabled the rapid discovery…

Fast Radio Bursts (FRBs) are short lived ($\sim$ msec), energetic transients (having a peak flux density of $\sim$ Jy) with no known prompt emission in other energy bands. We present results of a search for prompt X-ray emissions from 41…

High Energy Astrophysical Phenomena · Physics 2021-05-21 Akash Anumarlapudi , Varun Bhalerao , Shriharsh P. Tendulkar , Arvind Balasubramanian

The Swift X-ray Telescope (XRT) has discovered that flares are quite common in early X-ray afterglows of Gamma-Ray Bursts (GRBs), being observed in roughly 50% of afterglows with prompt followup observations. The flares range in fluence…

Recent data gathered and triggered by the SWIFT satellite have greatly improved our knowledge of long-duration gamma ray bursts (GRBs) and X-ray flashes (XRFs). This is particularly the case for the X-ray data at all times. We show that the…

Astrophysics · Physics 2009-09-29 Shlomo Dado , Arnon Dar , Alvaro De Rujula

The phenomenology of a subclass of High Mass X-ray Binaries hosting a blue supergiant companion, the so-called Supergiant Fast X-ray Transients (SFXTs), is reviewed. Their number is growing, mainly thanks to the discoveries performed by the…

High Energy Astrophysical Phenomena · Physics 2011-04-01 Lara Sidoli

Recent works have discovered two fast ($\approx 10$ ks) extragalactic X-ray transients in the Chandra Deep Field-South (CDF-S XT1 and XT2). These findings suggest that a large population of similar extragalactic transients might exist in…

High Energy Astrophysical Phenomena · Physics 2019-06-19 Guang Yang , W. N. Brandt , S. F. Zhu , F. E. Bauer , B. Luo , Y. Q. Xue , X. C. Zheng

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

The detection of x-ray afterglows of gamma-ray burst (GRB) sources has enabled the optical discovery that GRBs are at cosmological distances, which confirms that the enormous luminosities required must produce a relativistically expanding…

Astrophysics · Physics 2009-10-30 Jonathan E. Grindlay

Ultra-long Gamma-Ray Bursts are a class of high energy transients lasting several hours. Their exact nature is still elusive, and several models have been proposed to explain them. Because of the limited coverage of wide field gamma-ray…

High Energy Astrophysical Phenomena · Physics 2019-06-03 B. Gendre , Q. T. Joyce , N. B. Orange , G. Stratta , J. L. Atteia , M. Boer

Supergiant Fast X-ray Transients are a class of Galactic High Mass X-ray Binaries with supergiant companions. Their extreme transient X-ray flaring activity was unveiled thanks to INTEGRAL/IBIS observations. The SFXTs dynamic range, with…

High Energy Astrophysical Phenomena · Physics 2013-02-01 Lara Sidoli

X-Ray Flashes (XRFs) are soft gamma-ray bursts whose nature is not clear. Their soft spectrum can be due to cosmological effects (high redshift), an off-axis view of the jet or can be intrinsic to the source. We use SWIFT observations to…

Astrophysics · Physics 2009-11-11 B. Gendre , A. Galli , L. Piro

The discovery of a number of gamma-ray bursts with duration exceeding 1,000 seconds, in particular the exceptional case of GRB 111209A with a duration of about 25,000 seconds, has opened the question on whether these bursts form a new class…

High Energy Astrophysical Phenomena · Physics 2015-03-09 Michel Boer , Bruce Gendre , Giulia Stratta

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

Fast radio bursts (FRBs) are extremely strong radio flares lasting several milliseconds, most of which come from unidentified objects at a cosmological distance. They can be apparently repeating or not. In this paper, we analyzed 18…

Over the past few years, $\sim$30 extragalactic fast X-ray transients (FXRTs) have been discovered, mainly in Chandra and XMM-Newton data. Their nature remains unclear, with proposed origins including a double neutron star merger, a tidal…

The physical nature of Fast Radio Bursts (FRBs), a new type of cosmological transients discovered recently, is not known. It has been suggested that FRBs can be produced when a spinning supra-massive neutron star loses centrifugal support…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Bing Zhang

We report the discovery of a transient and fading hard X-ray emission in the BATSE lightcurves of a sample of short gamma-ray bursts. We have summed each of the four channel BATSE light curves of 76 short bursts to uncover the average…

Astrophysics · Physics 2009-11-07 Davide Lazzati , Enrico Ramirez-Ruiz , Gabriele Ghisellini