| Publications |
- A Hot Cocoon in the Ultralong GRB 130925A: Hints of a POPIII-like Progenitor in a Low-Density Wind Environment |Piro, Luigi, Troja, Eleonora, et al. | ApJ | 790-15 | 2014 | 2014ApJ...790L..15P | http://ui.adsabs.harvard.edu/#abs/2014ApJ...790L..15P
- XMM-Newton publication statistics |Ness, J.-U., Parmar, A. N., et al. | AN | 335-210 | 2014 | 2014AN....335..210N | http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N
- The Million Optical - Radio/X-ray Associations (MORX) Catalogue |Flesch, Eric W., | PASA | 33-52 | 2016 | 2016PASA...33...52F | http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F
- Dust scattering X-ray expanding rings around gamma-ray bursts |Mereghetti, S., Tiengo, A., | NCimB | 121-1111 | 2006 | 2006NCimB.121.1111M | http://ui.adsabs.harvard.edu/#abs/2006NCimB.121.1111M
- High-redshift Extremely Red Quasars in X-Rays |Goulding, Andy D., Zakamska, Nadia L., et al. | ApJ | 856-4 | 2018 | 2018ApJ...856....4G | http://ui.adsabs.harvard.edu/#abs/2018ApJ...856....4G
- Observation of inverse Compton emission from a long \\u03b3-ray burst |MAGIC Collaboration, Acciari, V. A., et al. | Natur | 575-459 | 2019 | 2019Natur.575..459M | http://ui.adsabs.harvard.edu/#abs/2019Natur.575..459M
- Investigation of Coronal Properties of X-Ray Bright G-dwarf Stars Based on the Solar Surface Magnetic Field-Corona Relationship |Takasao, Shinsuke, Mitsuishi, Ikuyuki, et al. | ApJ | 901-70 | 2020 | 2020ApJ...901...70T | http://ui.adsabs.harvard.edu/#abs/2020ApJ...901...70T
- 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
- The variable absorption in the X-ray spectrum of GRB 190114C |Campana, Sergio, Lazzati, Davide, et al. | A&A | 649-135 | 2021 | 2021A&A...649A.135C | http://ui.adsabs.harvard.edu/#abs/2021A&A...649A.135C
- Gamma-Ray Bursts Afterglow Physics and the VHE Domain |Miceli, Davide, Nava, Lara, | Galax | 10-66 | 2022 | 2022Galax..10...66M | http://ui.adsabs.harvard.edu/#abs/2022Galax..10...66M
- 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. |
