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Related papers: MAXI J1820+070 with NuSTAR II. Flaring during the …

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During a pointed 2018 NuSTAR observation, we detected a flare with a 2.2 hour duration from the magnetar 1RXS J170849.0$-$400910. The flare, which rose in $\sim25$ seconds to a maximum flux 6 times larger than the persistent emission, is…

High Energy Astrophysical Phenomena · Physics 2020-02-12 George Younes , Matthew G. Baring , Chryssa Kouveliotou , Zorawar Wadiasingh , Daniela Huppenkothen , Alice K. Harding

In this letter we report a tentative detection of soft time lags (i.e. variability of softer photons lags behind the variability of harder photons) in one $XMM-Newton$ observation of the tidal disruption event (TDE) candidate AT 2018fyk…

High Energy Astrophysical Phenomena · Physics 2022-01-05 Wenda Zhang

We present a rapid timing analysis of optical (HiPERCAM and ULTRACAM) and X-ray (NICER) observations of the X-ray transient Swift J1858.6-0814 during 2018 and 2019. The optical light curves show relatively slow, large amplitude (~1 mags in…

High Energy Astrophysical Phenomena · Physics 2023-01-25 T. Shahbaz , J. A. Paice , K. M. Rajwade , A. Veledina , P. Gandhi. , V. S. Dhillon , T. R. Marsh , S. Littlefair , M. R. Kennedy , R. P. Breton , C. J. Clark

We report results of a comprehensive study of the soft gamma-ray (30 keV to 1.7 MeV) emission of GROJ0422+32 during its first known outburst in 1992. These results were derived from the BATSE earth-occultation database with the JPL data…

Astrophysics · Physics 2009-11-07 J. C. Ling , Wm. A. Wheaton

The Galactic microquasar SS433 occasionally exhibits a major flare when the intensity of its emission increases significantly and rapidly. We present an analysis of high-resolution, almost-nightly optical spectra obtained before, during and…

Astrophysics of Galaxies · Physics 2015-05-27 Katherine Blundell , Linda Schmidtobreick , Sergei Trushkin

On 2 September 2017 MAXI J1535-571 went into outburst and peaked at ~5 Crab in the 2-20 keV energy range. Early in the flare INTEGRAL performed Target of Opportunity pointings and monitored the source as it transitioned from the hard state…

High Energy Astrophysical Phenomena · Physics 2023-02-13 James Rodi , E. Jourdain , J. P. Roques

We detected flaring flux variability that regularly occurred with the period of 23.9 days on a 6.7 GHz methanol maser emission at Vlsr = 25.30 km/s in G 014.23-00.50 through highly frequent monitoring using the Hitachi 32-m radio telescope.…

We present a spectral and timing study of the NuSTAR and Swift observations of the black hole candidate IGR J17091-3624 in the hard state during its outburst in 2016. Disk reflection is detected in each of the NuSTAR spectra taken in three…

1ES1927+654 is a nearby active galactic nucleus that has shown an enigmatic outburst in optical/UV followed by X-rays, exhibiting strange variability patterns at timescales of months-years. Here we report the unusual X-ray, UV, and radio…

MAXI J1820$+$070 is a transient black hole binary (BHB) discovered on 2018 March 11. The unprecedented rich statistics brought by the NICER X-ray telescope allows detailed timing analysis up to $\sim$1~kHz uncompromised by the photon shot…

High Energy Astrophysical Phenomena · Physics 2023-03-15 Tomoki Omama , Masahiro Tsujimoto , Ken Ebisawa , Misaki Mizumoto

MAXI J1820+070 is a new low-mass microquasar hosting a black hole recently discovered in X-rays by the MAXI instrument. It is the counterpart of ASASSN-18ey, discovered in optical a few days before by ASAS-SN. This source underwent a major…

High Energy Astrophysical Phenomena · Physics 2019-09-10 J. Hoang , E. Molina , M. López , M. Ribó , O. Blanch , J. Cortina , G. Maier , N. Park , M. de Naurois , E. de Ona Wilhelmi , J. P. Ernenwein , D. Malyshev , A. Mitchell , S. Ohm , R. Zanin

We present a multi-wavelength spectral and temporal analysis of the blazar OJ 287 during its recent activity between December 2015 -- May 2016, showing strong variability in the near-infrared (NIR) to X-ray energies with detection at…

A multiwavelength temporal and spectral analysis of flares of 3C 279 during November 2017--July 2018 are presented in this work. Three bright gamma-ray flares were observed simultaneously in X-ray and Optical/UV along with a prolonged…

High Energy Astrophysical Phenomena · Physics 2020-03-04 Raj Prince

The black hole candidate MAXI J1535-571 is a recently discovered X-ray transient. We report on the monitoring observations of Swift Gamma-Ray Burst Mission during outburst. The source transits from the hard state to the intermediate state,…

High Energy Astrophysical Phenomena · Physics 2018-08-15 Lian Tao , YuPeng Chen , Can Gungor , Yue Huang , FangJun Lu , JinLu Qu , LiMing Song , Liang Zhang , Shu Zhang , ShuangNan Zhang

We have studied the 1999 soft X-ray transient outburst of XTE J1859+226 at radio and X-ray wavelengths. The event was characterised by strong variability in the disc, corona and jet - in particular, a number of radio flares (ejections) took…

We study the rheology of amorphous packings of soft, frictionless particles close to jamming. Implementing a quasistatic simulation method we generate a well defined ensemble of states that directly samples the system at its yield-stress. A…

Soft Condensed Matter · Physics 2010-06-28 Claus Heussinger , Jean-Louis Barrat

We use the relativistic hydrodynamics code Cosmos++ to model the evolution of the radio nebula triggered by the Dec. 27, 2004 giant flare event of soft gamma repeater 1806-20. We primarily focus on the rebrightening and centroid motion…

Astrophysics · Physics 2008-11-26 Jay D. Salmonson , P. Chris Fragile , Peter Anninos

IGR J08408-4503 is a supergiant fast X-ray transient discovered in 2006 with a confirmed association with a O8.5Ib(f) supergiant star, HD 74194. We report on the analysis of two outbursts caught by Swift/BAT on 2006 October 4 and 2008 July…

We analyzed two observations of the low-mass black hole X-ray binary MAXI J1348-630 from Nuclear Spectroscopic Telescope Array (NuSTAR) during low hard state and hard intermediate state in the 2019 outburst. The reflection components are…

High Energy Astrophysical Phenomena · Physics 2023-04-27 Hanji Wu , Wei Wang , Na Sai

We have analyzed the optical light curves of the blazar OJ 287 obtained with the Transiting Exoplanet Survey Satellite (TESS) over about 80 days from 2021 October 13 to December 31, with an unprecedented sampling of 2 minutes. Although…

High Energy Astrophysical Phenomena · Physics 2023-11-07 Shubham Kishore , Alok C. Gupta , Paul J. Wiita
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