A dataset provided by the European Space Agency

Name: Early Phase Coverage of X-ray Flares Associated with Tidal Disruption Events
Published: 2018-04-21T22:00:00Z

Proposal ID	074425
Title	Early Phase Coverage of X-ray Flares Associated with Tidal Disruption Events
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744250301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0744250401
DOI	https://doi.org/10.5270/esa-zdkoevw
Principal Investigator, PI	Dr Wenfei Yu
Abstract	X-ray spectral lines are expected at the beginning of the X-ray flaresassociated with tidal disruption events (TDE), providing great opportunity toprobe the spin of dormant supermassive black holes (SMBHs) as well as detectBardeen-Petterson (BP) effect. Little is known about the early phase of TDEsobservationally. Coverage of the early phase will shed light on accretionphysics under extreme conditions inaccessible in other systems. We propose anintensive coverage of the early phase of bright TDE X-ray flares with joint XMMand Swift observations. The observations would lead to the first detection of BPdisks expected around spinning SMBHs and the first application of reverberationmapping of the innermost accretion flow around a previously quiescent SMBH.
Publications	The complex evolution of the X-ray binary transient MAXI J1807+132 along the decay of its discovery outburst \|Jimenez-Ibarra, F., Munoz-Darias, T., et al. \| MNRAS \| 484-2078 \| 2019 \| 2019MNRAS.484.2078J \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.484.2078J 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 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	2017-03-29T20:49:58Z/2017-03-30T16:37:14Z
Version	19.17_20220121_1250
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	2018-04-21T22:00:00Z
Keywords	"quiescent smbh", "innermost accretion flow", "accretion physics", "XMM", "tidal disruption events", "shed light", "reverberation mapping", "bp dis", "xray flare", "spinning smbhs", "conditions inaccessible", "tdes observationally", "xray spectral lines", "intensive coverage"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Wenfei Yu, 2018, 'Early Phase Coverage of X-ray Flares Associated with Tidal Disruption Events', 19.17_20220121_1250, European Space Agency, https://doi.org/10.5270/esa-zdkoevw