Proposal ID | 086484 |
Title | Confirming the nature of 5 tidal disruption event candidates |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0864840301 |
DOI | https://doi.org/10.57780/esa-c1hacl7 |
Principal Investigator, PI | Mr Andrea Sacchi |
Abstract | In a search for new TDEs candidates we cross-matched optical and x-rayscatalogues. We propose the observation of 5 of our best candidates\: thesegalaxies show a high x-rays luminosity (L_X>10^41 erg/sec) and an extremely softspectrum (Gamma>3) in the same energy band. As no other known source should beable to show a similar behaviour we are positive that these are unrecognizedTDEs. If these galaxies indeed hosted a TDE we expect that by now theirluminosity should have dropped by a significant factor (>5) allowing us toconfirm their nature. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2020-11-19T11:13:09Z/2021-04-30T11:06:41Z |
Version | 19.16_20210326_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 | 2022-05-27T00:00:00Z |
Keywords | "cross matched optical", "tdes candidates", "luminosity l_x", "unrecognized tdes", "soft spectrum gamma", "galaxy indeed hosted", "energy band", "candidates \:" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Mr Andrea Sacchi, 2022, 'Confirming the nature of 5 tidal disruption event candidates', 19.16_20210326_1200, European Space Agency, https://doi.org/10.57780/esa-c1hacl7 |