| Proposal ID | 086501 |
| Title | An unprecedented view of high-frequency QPO phenomena in accreting black holes |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0865010101 |
| DOI | https://doi.org/10.57780/esa-8nahomj |
| Principal Investigator, PI | Dr William Alston |
| Abstract | We propose an 855 ks (9x95 ks) large program on the well-known narrow lineSeyfert 1 galaxy, RE J1034+396, in order to study the X-ray quasi-periodicoscillation (QPO) in unprecedented detail. These signatures of strong gravityare common to high accretion-rate processes across the mass range. The QPO in REJ1034+396 is already confirmed in 6 XMM-Newton observations, though 4 of theseare too short to study the feature at high frequency resolution. We willconclusively measure the harmonic oscillation and use spectral- timing methodsto place important constraints on the underlying physical QPO mechanism. We willalso use the dynamics of this feature to provide insight into theaccretion/ejection processes associated with high- Eddington rates. This is an observation only XMM-Newton can make |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2020-11-20T07:11:04Z/2021-05-31T22:16:02Z |
| 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 | 2022-06-25T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "accreting black holes", "eddington rates", "xmm newton", "XMM-Newton", "re j1034", "frequency resolution", "frequency qpo phenomena", "physical qpo mechanism", "narrow line seyfert", "mass range", "XMM", "harmonic oscillation", "ejection processes", "accretion rate processes", "855 9x95" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr William Alston, 2022, 'An unprecedented view of high-frequency QPO phenomena in accreting black holes', 19.16_20210326_1200, European Space Agency, https://doi.org/10.57780/esa-8nahomj |