| Publications |
- Calibration and in-orbit performance of the reflection grating spectrometer onboard XMM-Newton |de Vries, C. P., den Herder, J. W., et al. | A&A | 573-128 | 2015 | 2015A&A...573A.128D | http://ui.adsabs.harvard.edu/#abs/2015A&A...573A.128D
- The Rotation of the Hot Gas around the Milky Way |Hodges-Kluck, Edmund J., Miller, Matthew J., | ApJ | 822-21 | 2016 | 2016ApJ...822...21H | http://ui.adsabs.harvard.edu/#abs/2016ApJ...822...21H
- 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
- Discovery of Galactic O iv and O v X-ray absorption due to transition temperature gas in the PKS 2155-304 spectrum |Nevalainen, J., Wakker, B., et al. | A&A | 605-47 | 2017 | 2017A&A...605A..47N | http://ui.adsabs.harvard.edu/#abs/2017A&A...605A..47N
- The Hard X-Ray Emission of the Blazar PKS 2155-304 |Gaur, Haritma, Chen, Liang, et al. | ApJ | 850-209 | 2017 | 2017ApJ...850..209G | http://ui.adsabs.harvard.edu/#abs/2017ApJ...850..209G
- X-ray spectral variability of blazars using principal component analysis |Gallant, D., Gallo, L. C., | MNRAS | 480-1999 | 2018 | 2018MNRAS.480.1999G | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480.1999G
- To be or not to be: the case of the hot WHIM absorption in the blazar PKS 2155-304 sight line |Nevalainen, J., Tempel, E., et al. | A&A | 621-88 | 2019 | 2019A&A...621A..88N | http://ui.adsabs.harvard.edu/#abs/2019A&A...621A..88N
- Variability studies and modelling of the blazar PKS 2155-304 in the light of a decade of multi-wavelength observations |Chevalier, J., Sanchez, D. A., et al. | MNRAS | 484-749 | 2019 | 2019MNRAS.484..749C | http://ui.adsabs.harvard.edu/#abs/2019MNRAS.484..749C
- Short-Term X-ray Variability during Different Activity Phases of Blazars S5 0716+714 and PKS 2155-304 |Kushwaha, Pankaj, Pal, Main, | Galax | 8-66 | 2020 | 2020Galax...8...66K | http://ui.adsabs.harvard.edu/#abs/2020Galax...8...66K
- 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
- Nitrogen X-ray absorption in the local ISM |Gatuzz, Efrain, Garc\\u00eda, Javier A., | MNRAS | 504-4460 | 2021 | 2021MNRAS.504.4460G | http://ui.adsabs.harvard.edu/#abs/2021MNRAS.504.4460G
- An XMM-Newton catalogue of BL Lacs |de la Calle P\\u00e9rez, I., \\u00c1lvarez Crespo, N., et al. | A&A | 655-48 | 2021 | 2021A&A...655A..48D | http://ui.adsabs.harvard.edu/#abs/2021A&A...655A..48D
- 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. |
