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Related papers: Swift J2058.4+0516: Discovery of a Possible Second…

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We present observations of Swift J1112.2-8238, and identify it as a candidate relativistic tidal disruption flare (rTDF). The outburst was first detected by Swift/BAT in June 2011 as an unknown, long-lived (order of days) $\gamma$-ray…

High Energy Astrophysical Phenomena · Physics 2015-08-19 G. C. Brown , A. J. Levan , E. R. Stanway , N. R. Tanvir , S. B. Cenko , E. Berger , R. Chornock , A. Cucchiaria

We report a multiwavelength (X-ray, ultraviolet/optical/infrared, radio) analysis of the relativistic tidal disruption event candidate Sw J2058+05 from 3 months to 3 yr post-discovery in order to study its properties and compare its…

We present late-time follow-up of the relativistic tidal disruption flare candidate Swift J1112.2-8238. We confirm the previously determined redshift of $z=0.8900\pm0.0005$ based on multiple emission line detections. {\em HST} imaging of…

High Energy Astrophysical Phenomena · Physics 2017-09-01 G. C. Brown , A. J. Levan , E. R. Stanway , T. Kruhler , N. R. Tanvir , L. J. M. Davies , A. Fruchter , S. B. Cenko , B. D. Metzger

Active galactic nuclei (AGN), powered by long-term accretion onto central supermassive black holes, produce relativistic jets with lifetimes of greater than one million yr that preclude observations at birth. Transient accretion onto a…

We present late-time multi-wavelength observations of Swift J1644+57, suggested to be a relativistic tidal disruption flare (TDF). Our observations extend to >4 years from discovery, and show that 1.4 years after outburst the relativistic…

On March 28, 2011, the Swift Burst Alert Telescope triggered on an object that had no analog in over six years of Swift operations. Follow-up observations by the Swift X-ray Telescope (XRT) found a new, bright X-ray source covering 3 orders…

High Energy Astrophysical Phenomena · Physics 2016-02-03 V. Mangano , D. N. Burrows , B. Sbarufatti , J. K. Cannizzo

We report on the X-ray properties of the new transient Swift J0840.7$-$3516, discovered with Swift/BAT in 2020 February, using extensive data of Swift, MAXI, NICER, and NuSTAR. The source flux increased for $\sim 10^3$ s after the…

Sw 1644+57/GRB 110328A is a remarkable cosmological X-ray outburst detected by the {\it Swift} satellite. Its early-time ($t\lesssim 0.1$ days since the trigger) X-ray emission resembles some gamma-ray bursts (GRBs), e.g., GRB 090417B. But…

High Energy Astrophysical Phenomena · Physics 2015-05-28 Lang Shao , Fu-Wen Zhang , Yi-Zhong Fan , Da-Ming Wei

Swift J1842.5$-$1124 is a transient Galactic black hole X-ray binary candidate, which underwent a new outburst in May 2020. We performed multi-epoch MeerKAT radio observations under the ThunderKAT Large Survey Programme, coordinated with…

High Energy Astrophysical Phenomena · Physics 2021-12-15 X. Zhang , W. Yu , S. E. Motta , R. Fender , P. Woudt , J. C. A. Miller-Jones , G. R. Sivakoff

The recently discovered high-energy transient Swift J164449.3+573451 (Sw J1644+57) is thought to arise from the tidal disruption of a passing star by a dormant massive black hole. Modeling of the broadband emission suggests the presence of…

High Energy Astrophysical Phenomena · Physics 2015-05-28 Xiang-Yu Wang , Ruo-Yu Liu , Zi-Gao Dai , K. S. Cheng

IGR J11215-5952 is a hard X-ray transient source discovered in April 2005 with INTEGRAL and a confirmed member of the new class of High Mass X-ray Binaries, the Supergiant Fast X-ray Transients (SFXTs). Archival INTEGRAL data and RXTE…

Astrophysics · Physics 2007-06-13 P. Romano , L. Sidoli , V. Mangano , S. Mereghetti , G. Cusumano

We present deep infrared (Ks band) imaging polarimetry and radio (1.4 and 4.8 GHz) polarimetry of the enigmatic transient Swift J164449.3+573451. This source appears to be a short lived jet phenomenon in a galaxy at redshift z = 0.354,…

SDSS J120136.02+300305.5 was detected in an XMM-Newton slew from June 2010 with a flux 56 times higher than an upper limit from ROSAT, corresponding to Lx~3x10^44 ergs/s. It has the optical spectrum of a quiescent galaxy (z=0.146). Overall…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 R. D. Saxton , A. M. Read , P. Esquej , S. Komossa , S. Dougherty , P. Rodriguez-Pascual , D. Barrado

We present continued radio and X-ray observations of the previously relativistic tidal disruption event (TDE) Swift J164449.3+573451 (\sw) extending to about 9.4 years post disruption, as part of ongoing campaigns with the Jansky Very Large…

High Energy Astrophysical Phenomena · Physics 2021-02-24 Yvette Cendes , Tarraneh Eftekhari , Edo Berger , Emil Polisensky

We present continued radio and X-ray observations of the relativistic tidal disruption event Swift J164449.3+573451 extending to $\delta t \approx 2000$ d after discovery. The radio data were obtained with the VLA as part of a long-term…

High Energy Astrophysical Phenomena · Physics 2018-02-28 T. Eftekhari , E. Berger , B. A. Zauderer , R. Margutti , K. D. Alexander

We report on observations of black hole Swift J1357.2-0933, a member of the modest population of very faint X-ray transients. This source has previously shown intense dips in the optical lightcurve, a phenomena that has been linked to the…

We present the discovery of a luminous X-ray transient, serendipitously detected by Swift's X-ray Telescope (XRT) on 2020 February 5, located in the nucleus of the galaxy SDSS J143359.16+400636.0 at z=0.099 (luminosity distance $D_{\rm…

We present preliminary results from the analysis of simultaneous multiwavelength observations of the black hole candidate Swift J1753.5-0127. The source is still continuing its outburst started in May 2005, never leaving the Low/Hard State.…

We report on Swift observations of the Narrow-Line Seyfert 1 galaxy (NLS1) RX J0148.3--2758. It was observed for 41.6 ks in 2005 May and for 15.8 ks in 2005 December. On short as well as on long timescales RX J0148.3--2758 is a highly…

We present continued radio observations of the tidal disruption event SwiftJ164449.3+573451 extending to \sim216 days after discovery. The data are part of a long-term program to monitor the expansion and energy scale of the relativistic…

High Energy Astrophysical Phenomena · Physics 2015-06-03 E. Berger , A. Zauderer , G. G. Pooley , A. M. Soderberg , R. Sari , A. Brunthaler , M. F. Bietenholz
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