A dataset provided by the European Space Agency

Name: Late-time observations of a candidate relativistic tidal disruption flare
Published: 2017-11-11T23:00:00Z

Proposal ID	078479
Title	Late-time observations of a candidate relativistic tidal disruption flare
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784790101
DOI	https://doi.org/10.5270/esa-u0lebko
Principal Investigator, PI	Mr Gregory Brown
Abstract	The exceptional properties of a handful of extremely long-lived, Swift-BATdetected flares have marked them as a new class of event, likely, but notuniquely caused by the creation of a relativistic jet during the tidaldisruption of star. Here we propose to obtain a further observation of by farthe best studied event, Swift J1644+57, 6 years after the initial outburst.Swift J1644+57 displayed a sharp cut-off in its X-ray emission approximately 500days post trigger and has since plateaued at a level a factor >100 lower thanbefore the drop. Our observations will determine if this emission is caused by acontinuation of transient emission after the switch-off of a relativistic jet,or if it is due to the presence of an AGN in the host galaxy.
Publications	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 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 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	2016-10-18T14:20:23Z/2016-10-19T06:10:23Z
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	2017-11-11T23:00:00Z
Keywords	"transient emission", "late time", "sharp cut", "tidal disruption", "relativistic jet", "swift j1644", "post trigger", "xray emission approximately", "swift bat", "initial outburst"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Gregory Brown, 2017, 'Late-time observations of a candidate relativistic tidal disruption flare', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-u0lebko