We propose to observe nearby repeating fast radio bursts (FRBs) with XMM Newtonto probe for X-ray counterparts to radio bursts. This will test whether they areconsistent with predictions from young magnetar progenitor theories. Recentevidence, such as the detection of a FRB-like burst from the Galactic magnetarSGR 1935+2154, suggests that magnetars may be the engines of at least some FRBs.We will compare X-ray observables, like burst luminosity and temporalproperties, to those predicted from magnetar progenitor theories. To probe asdeep as possible, we will provide fully simultaneous radio coverage to providetimes of radio bursts during the XMM observations. This will allow us to searchfor X-ray bursts in as narrow a time and spatial window as possible.
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2022-12-09T10:02:51Z/2022-12-15T18:46:03Z
Version
20.09_20221024_1724
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.
European Space Agency, Ms Amanda Cook, 2024, 'SIMULTANEOUS XMM-NEWTON AND RADIO OBSERVATIONS OF REPEATING FAST RADIO BURSTS', 20.09_20221024_1724, European Space Agency, https://doi.org/10.57780/esa-r3yvh51
