| Publications |
- X-ray spectroscopic studies of stars |Gudel, M., | AdSpR | 32-2045 | 2003 | 2003AdSpR..32.2045G | http://ui.adsabs.harvard.edu/#abs/2003AdSpR..32.2045G
- First light measurements with the XMM-Newton reflection grating spectrometers: Evidence for an inverse first ionisation potential effect and anomalous Ne abundance in the Coronae of HR 1099 |Brinkman, A. C., Behar, E., et al. | A&A | 365-324 | 2001 | 2001A&A...365L.324B | http://ui.adsabs.harvard.edu/#abs/2001A&A...365L.324B
- The XMM-Newton view of stellar coronae: Flare heating in the coronae of HR 1099 |Audard, M., Gudel, M., | A&A | 365-318 | 2001 | 2001A&A...365L.318A | http://ui.adsabs.harvard.edu/#abs/2001A&A...365L.318A
- The first decade of science with Chandra and XMM-Newton |Santos-Lleo, Maria, Schartel, Norbert, et al. | Natur | 462-997 | 2009 | 2009Natur.462..997S | http://ui.adsabs.harvard.edu/#abs/2009Natur.462..997S
- 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
- Investigations of stellar coronae with XMM-Newton |Audard, M., | AdSpR | 32-927 | 2003 | 2003AdSpR..32..927A | http://ui.adsabs.harvard.edu/#abs/2003AdSpR..32..927A
- X-ray emission from the stellar population in M 32 |Revnivtsev, M., Churazov, E., et al. | A&A | 473-783 | 2007 | 2007A&A...473..783R | http://ui.adsabs.harvard.edu/#abs/2007A&A...473..783R
- 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 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
- Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function |Vagnetti, F., Middei, R., et al. | A&A | 593-55 | 2016 | 2016A&A...593A..55V | http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V
- 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
- Why solar astronomers should be interested in stars |Pallavicini, R., | AdSpR | 32-885 | 2003 | 2003AdSpR..32..885P | http://ui.adsabs.harvard.edu/#abs/2003AdSpR..32..885P
- Long-term variations in the X-ray activity of HR 1099 |Perdelwitz, V., Navarrete, F. H., et al. | A&A | 616-161 | 2018 | 2018A&A...616A.161P | http://ui.adsabs.harvard.edu/#abs/2018A&A...616A.161P
- 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
- 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. |
