A dataset provided by the European Space Agency

Proposal ID 090276
Title A Systematic Exploration of Late-time X-ray Emission from Optically-Loud TDEs
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DOI https://doi.org/10.57780/esa-ynqflmv
Principal Investigator, PI Ms Yuhan Yao
Abstract We propose to conduct deep X-ray observations of 12 nearby tidal disruptionevents (TDEs). This sample, selected from the first three years of the ZwickyTransient Facility operation, has good temporal coverage of early-time X-raydata. The proposed observations will be the first experiment to systematicallystudy the X-ray emission of optically bright TDEs at the time when the accretionis expected to transition from super-Eddington to sub-Eddington. This programwill help us to (1) investigate the timescale of delayed X-ray brightening, (2)explore the existence of disk corona and the efficiency of Comptonization, (3)measure the mass accretion rate, which directly tracks the mass fall-back rateat late time.
Publications
  • A Systematic Analysis of the X-Ray Emission in Optically Selected Tidal Disruption Events: Observational Evidence for the Unification of the Optically and X-Ray-selected Populations |Guolo Muryel Gezari Suvi et al. | ApJ | 966-160 | 2024 | 2024ApJ...966..160G | http://ui.adsabs.harvard.edu/#abs/2024ApJ...966..160G
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2022-05-13T15:32:01Z/2023-04-15T03:12:11Z
Version 20.10_20230417_1156
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 2024-05-06T00:00:00Z
Keywords "late time", "time xray data", "mass accretion rate", "systematic exploration", "disk corona", "super eddington", "optically bright tdes", "sub eddington", "xray emission", "temporal coverage", "delayed xray brightening", "conduct deep xray", "optically loud tdes"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Ms Yuhan Yao, 2024, 'A Systematic Exploration of Late-time X-ray Emission from Optically-Loud TDEs', 20.10_20230417_1156, European Space Agency, https://doi.org/10.57780/esa-ynqflmv