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
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902760101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902760201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902760301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902760401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902760501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902760701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902760801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902760901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902761101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902761401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902761501
...
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0902761601

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 21.51_20241115_1113
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
Last Update 2026-07-09
Keywords XMM-Newton, OM, RGS, EPIC, X-ray, Multi-Mirror, SAS
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', 21.51_20241115_1113, European Space Agency, https://doi.org/10.57780/esa-ynqflmv
Rights Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.