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Multiwavelength observations of PSR J2021+4026 across a mode change reveal a phase shift in its X-ray emission |Razzano M. Fiori A. et al. | A&A | 676-91 | 2023 | 2023A&A...676A..91R | http://ui.adsabs.harvard.edu/#abs/2023A&A...676A..91R
A phase-resolved Fermi-LAT analysis of the mode-changing pulsar PSR J2021+4026 shows hints of a multipolar magnetosphere |Fiori A. Razzano M. et al. | A&A | 685-A70 | 2024 | 2024A&A...685A..70F | http://ui.adsabs.harvard.edu/#abs/2024A&A...685A..70F
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
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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 Fred Jansen XMM-Newton MM, 2016, 'Timing verification with the Crab', 19.17_20220121_1250, European Space Agency, https://doi.org/10.5270/esa-5c3yyhz