A dataset provided by the European Space Agency

Name: A time-resolved study of the injection of mass onto a dormant SMBH
Published: 2017-12-20T23:00:00Z

Proposal ID	076364
Title	A time-resolved study of the injection of mass onto a dormant SMBH
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763640201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763640401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763640501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763640601
DOI	https://doi.org/10.5270/esa-362nqmr
Principal Investigator, PI	Mr Richard Saxton
Abstract	We propose to extend a program, running since AO-7, designed to find tidaldisruption events at the peak of their emission by a near-real time comparisonof XMM-Newton slew data with the ROSAT all-sky survey. Candidate events will bemonitored with XMM-Newton and Swift pointed observations, as well as spacedoptical spectra, to follow their temporal and spectral evolution. During thisprogram we have discovered and monitored flares from two optically quiescentgalaxies, SDSS J120136.02+300305.5 and 2MASX 07400785-8539307 and been able toshow, that their peak X-ray emission is reprocessed and not simply thehigh-energy tail of thermal emission as previously thought.
Publications	XMMSL2 J144605.0+685735: a slow tidal disruption event \|Saxton, R. D., Read, A. M., et al. \| A&A \| 630-98 \| 2019 \| 2019A&A...630A..98S \| http://ui.adsabs.harvard.edu/#abs/2019A&A...630A..98S The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters \|Pastor-Marazuela, I., Webb, N. A., et al. \| A&A \| 640-124 \| 2020 \| 2020A&A...640A.124P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...640A.124P 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 X-rays to physical parameters: a comprehensive analysis of thermal tidal disruption event X-ray spectra \|Mummery, Andrew, Wevers, Thomas, et al. \| MNRAS \| 519-5828 \| 2023 \| 2023MNRAS.519.5828M \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.519.5828M 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	2016-09-08T15:50:06Z/2016-11-27T16:39:44Z
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	2017-12-20T23:00:00Z
Keywords	"2masx 07400785 8539307", "sdss j120136", "real time comparison", "monitored flare", "XMM-Newton", "spectral evolution", "thermal emission", "xmm newton", "optically quiescent galaxy", "time resolved", "ROSAT", "SDSS", "candidate events", "energy tail", "XMM", "spaced optical spectra", "sky survey", "tidal disruption events", "dormant smbh", "peak xray emission"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Richard Saxton, 2017, 'A time-resolved study of the injection of mass onto a dormant SMBH', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-362nqmr