| Publications |
- Potential cooling of an accretion-heated neutron star crust in the low-mass X-ray binary 1RXS J180408.9-342058 |Parikh, A. S., Wijnands, R., et al. | MNRAS | 466-4074 | 2017 | 2017MNRAS.466.4074P | http://ui.adsabs.harvard.edu/#abs/2017MNRAS.466.4074P
- Further constraints on neutron star crustal properties in the low-mass X-ray binary 1RXS J180408.9-342058 |Parikh, A. S., Wijnands, R., et al. | MNRAS | 476-2230 | 2018 | 2018MNRAS.476.2230P | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.476.2230P
- Results from a Systematic Survey of X-Ray Emission from Hydrogen-poor Superluminous SNe |Margutti, R., Chornock, R., et al. | ApJ | 864-45 | 2018 | 2018ApJ...864...45M | http://ui.adsabs.harvard.edu/#abs/2018ApJ...864...45M
- Blasts from the Past: Supernova Shock Breakouts among X-Ray Transients in the XMM-Newton Archive |Alp, Dennis, Larsson, Josefin, | ApJ | 896-39 | 2020 | 2020ApJ...896...39A | http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...39A
- The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters |Pastor-Marazuela, I., Webb, N. A., et al. | A&A | 640-124 | 2020 | 2020A&A...640A.124P | http://ui.adsabs.harvard.edu/#abs/2020A&A...640A.124P
- Classification of 4XMM-DR9 sources by machine learning |Zhang, Yanxia, Zhao, Yongheng, | MNRAS | 503-5263 | 2021 | 2021MNRAS.503.5263Z | http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z
- Luminosity Function and Event Rate Density of XMM-Newton-selected Supernova Shock Breakout Candidates |Sun, Hui, Liu, He-Yang, et al. | ApJ | 927-224 | 2022 | 2022ApJ...927..224S | http://ui.adsabs.harvard.edu/#abs/2022ApJ...927..224S
- XMM-Newton-discovered Fast X-ray Transients: host galaxies and limits on contemporaneous detections of optical counterparts |Eappachen, D., Jonker, P. G., et al. | MNRAS | 527-11823 | 2024 | 2024MNRAS.52711823E | http://ui.adsabs.harvard.edu/#abs/2024MNRAS.52711823E
- The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions |Pan, Zeyang, Qu, Zhijie, et al. | ApJS | 271-62 | 2024 | 2024ApJS..271...62P | http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P
- From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources |Rodriguez, Antonio C., | PASP | 136-054201 | 2024 | 2024PASP..136e4201R | http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R
- 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
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| 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. |
