Swift J1749.4-2807 is the first (and only) eclipsing accreting X-ray millisecondpulsar. At variance with all the other transient low mass X-ray binaries, SwiftJ1749 is the only source showing eclipses and a hard component in its X-rayquiescent spectrum. This opens the unique opportunity to discriminate betweenmodels that have been proposed for the quiescent emission of neutron startransients. Based on a detailed feasibility we need to follow Swift J1749 forthree orbital periods, totalling 100 ks, to probe the quiescent spectrum with aneclipse mapping technique.
An X-ray chimney extending hundreds of parsecs above and below the Galactic Centre |Ponti, G., Hofmann, F., et al. | Natur | 567-347 | 2019 | 2019Natur.567..347P | http://ui.adsabs.harvard.edu/#abs/2019Natur.567..347P
The Galactic center chimneys: the base of the multiphase outflow of the Milky Way |Ponti, G., Morris, M. R., et al. | A&A | 646-66 | 2021 | 2021A&A...646A..66P | http://ui.adsabs.harvard.edu/#abs/2021A&A...646A..66P
Robust constraints on feebly interacting particles using XMM-Newton |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-L101305 | 2024 | 2024PhRvD.109j1305L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L
Multimessenger search for electrophilic feebly interacting particles from supernovae |Luque, Pedro De la Torre, Balaji, Shyam, | PhRvD | 109-103028 | 2024 | 2024PhRvD.109j3028L | http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L
Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints |De la Torre Luque, Pedro, Balaji, Shyam, | ApJ | 968-46 | 2024 | 2024ApJ...968...46D | http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2017-03-01T07:09:31Z/2017-03-02T13:01:11Z
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.
European Space Agency, Dr Paolo D.Avanzo, 2018, 'Observation of the quiescent X-ray emission of Swift J1749.4 2807', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-wz5mzu0
