Name | 079575 |
Title | Measuring the High Energy Emission of Millisecond X-Ray Pulsars in Outburst |
URL | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0795750101 |
DOI | https://doi.org/10.5270/esa-0jlurl3 |
Author | Dr Sergey Tsygankov |
Description | We propose to perform two 170 ks INTEGRAL ToO observations of a transient millisecond X-ray pulsar in outburst. To constrain the broadband spectrum we also request one 30 ks simultaneous NuSTAR and two 50 ks XMM-Newton observations. The target can be either one of the fifteen known transient accreting millisecond X-ray pulsars (AMXPs) in the case of a new outburst or a "newly" observed object of this class. These observations allow us to study the broad band spectrum in detail from hard to soft X-ray energies as well as the timing properties or eclipsing features of the source during its outburst. We will detect type-I X-ray bursts, and-or for the first time also burst oscillations at high-energy (if present). |
Publication | No observations found associated with the current proposal |
Instrument | EMOS1, EMOS2, EPN, RGS1, RGS2 |
Temporal Coverage | 2018-09-03T17:49:09Z/2018-09-04T04:00:49Z |
Version | 19.17_20220121_1250 |
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 | 2019-10-01T22:00:00Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2019-10-01T22:00:00Z, 079575, 19.17_20220121_1250. https://doi.org/10.5270/esa-0jlurl3 |