A dataset provided by the European Space Agency

Name: A late time look at the relativistic tidal disruption event Swift 2058+0516
Published: 2013-05-12T00:00:00Z

Proposal ID	069483
Title	A late time look at the relativistic tidal disruption event Swift 2058+0516
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0694830201
DOI	https://doi.org/10.5270/esa-c2c2gc8
Principal Investigator, PI	Dr Andrew Levan
Abstract	In March and May this year, our collaboration discovered two examples of anapparently new class of high energy transient. Named Swift 1644+57 and Swift2058+0516, they are exceptionally X-ray bright events, accompanied by emissionacross the electromagnetic spectrum. A working model is that these are the tidaldisruption of a star by the central black hole in a distant galaxy, althoughalternative models remain plausible. Here we seek long term observations ofSwift 2058+0516. Using XMM-Newton we will measure both the lightcurve andspectrum at late times while the source is too faint for the Swift-XRT. In doingso we will determine late time properties of the object (e.g. disc vs jet) andcompare the lightcurve to the expectations for tidal disruption events.
Publications	Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y A Multiwavelength Study of the Relativistic Tidal Disruption Candidate Swift J2058.4+0516 at Late Times \|Pasham, Dheeraj R., Cenko, S. Bradley, et al. \| ApJ \| 805-68 \| 2015 \| 2015ApJ...805...68P \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...805...68P The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F New Physical Insights about Tidal Disruption Events from a Comprehensive Observational Inventory at X-Ray Wavelengths \|Auchettl, Katie, Guillochon, James, \| ApJ \| 838-149 \| 2017 \| 2017ApJ...838..149A \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...838..149A Radiative interaction between the relativistic jet and optically thick envelope in tidal disruption events \|Lu, Wenbin, Krolik, Julian, et al. \| MNRAS \| 471-1141 \| 2017 \| 2017MNRAS.471.1141L \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.1141L Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Central Black Hole Mass in the Distant Tidal Disruption Event Candidate of Swift J2058.4+0516 \|Zhang, XueGuang, \| ApJ \| 928-182 \| 2022 \| 2022ApJ...928..182Z \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...928..182Z The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-05-01T17:21:43Z/2012-05-02T08:40:23Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2013-05-12T00:00:00Z
Keywords	"alternative models", "swift 2058", "XMM", "tidal disruption events", "energy transient", "named swift 1644", "tidal disruption", "electromagnetic spectrum", "distant galaxy", "XMM-Newton", "late time properties", "swift xrt", "central blackhole", "xray bright events", "late time look", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Andrew Levan, 2013, 'A late time look at the relativistic tidal disruption event Swift 2058+0516', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-c2c2gc8