Proposal ID | 069157 |
Title | A detailed look at an understudied ULX QPO |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0691570101 |
DOI | https://doi.org/10.5270/esa-af0d1cu |
Principal Investigator, PI | Dr Matthew Middleton |
Abstract | The study of quasi-periodic oscillations (QPOs) is of increasing importance inhelping us to understand the enigmatic population of ultra-luminous X-raysources (ULXs). Whilst few in number, these signals present an opportunity tounderstand the accretion flow and provide a diagnostic of the central, unknownmass by comparison of the joint spectral and timing characteristics of theemission to those of well studied X-ray binaries (XRBs) and active galacticnuclei (AGNs). We propose a single orbit observation of NGC 6946 X-1, providingonly the second unambiguous high-quality dataset on a ULX with a QPO. This willallow the QPO and broad-band variability to be probed using the latest jointspectral/timing methods, allowing robust tests for models of the emission properties of this ULX. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2012-10-21T17:50:58Z/2012-10-23T02:59:19Z |
Version | 17.56_20190403_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 | 2013-11-07T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "ngc 6946 x", "robust tests", "quality dataset", "NGC 6946", "enigmatic population", "emission properties", "understudied ulx qpo", "single orbit", "broad band variability", "xray binary xrbs", "accretion flow" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Matthew Middleton, 2013, 'A detailed look at an understudied ULX QPO', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-af0d1cu |