| Name | 086501 |
| Title | An unprecedented view of high-frequency QPO phenomena in accreting black holes |
| URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0865010101 |
| DOI | https://doi.org/10.57780/esa-8nahomj |
| Author | European Space Agency |
| Description | We propose an 855 ks (9x95 ks) large program on the well-known narrow line Seyfert 1 galaxy, RE J1034+396, in order to study the X-ray quasi-periodic oscillation (QPO) in unprecedented detail. These signatures of strong gravity are common to high accretion-rate processes across the mass range. The QPO in RE J1034+396 is already confirmed in 6 XMM-Newton observations, though 4 of these are too short to study the feature at high frequency resolution. We will conclusively measure the harmonic oscillation and use spectral- timing methods to place important constraints on the underlying physical QPO mechanism. We will also use the dynamics of this feature to provide insight into the accretion/ejection processes associated with high- Eddington rates. This is an observation only XMM-Newton can make |
| Publication | No observations found associated with the current proposal |
| 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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, 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 |