| Publications |
- The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue |Watson, M. G., Schroder, A. C., et al. | A&A | 493-339 | 2009 | 2009A&A...493..339W | http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W
- Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras |Mateos, S., Saxton, R. D., et al. | A&A | 496-879 | 2009 | 2009A&A...496..879M | http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M
- The eclipsing bursting X-ray binary EXO 0748-676 revisited by XMM-Newton |Bonnet-Bidaud, J. M., Haberl, F., et al. | A&A | 365-282 | 2001 | 2001A&A...365L.282B | http://ui.adsabs.harvard.edu/#abs/2001A&A...365L.282B
- XMM-Newton light curves of the low-mass X-ray binary EXO 0748-676: Dips, eclipses, and bursts |Homan, J., Wijnands, R., | A&A | 412-799 | 2003 | 2003A&A...412..799H | http://ui.adsabs.harvard.edu/#abs/2003A&A...412..799H
- Properties of the background of EPIC-pn onboard XMM-Newton |Katayama, H., Takahashi, I., et al. | A&A | 414-767 | 2004 | 2004A&A...414..767K | http://ui.adsabs.harvard.edu/#abs/2004A&A...414..767K
- Gravitationally redshifted absorption lines in the X-ray burst spectra of a neutron star |Cottam, J., Paerels, F., | Natur | 420-51 | 2002 | 2002Natur.420...51C | http://ui.adsabs.harvard.edu/#abs/2002Natur.420...51C
- Exospheric solar wind charge exchange as seen by XMM-Newton |Carter, J. A., Semba, S., | AN | 333-313 | 2012 | 2012AN....333..313C | http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C
- Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog |Lin, Dacheng, Webb, Natalie A., | ApJ | 756-27 | 2012 | 2012ApJ...756...27L | http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L
- The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton |De Luca, A., Molendi, S., | A&A | 419-837 | 2004 | 2004A&A...419..837D | http://ui.adsabs.harvard.edu/#abs/2004A&A...419..837D
- Automatic Classification of Time-variable X-Ray Sources |Lo, Kitty K., Farrell, Sean, et al. | ApJ | 786-20 | 2014 | 2014ApJ...786...20L | http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L
- The diversity of quasars unified by accretion and orientation |Shen, Yue, Ho, Luis C., | Natur | 513-210 | 2014 | 2014Natur.513..210S | http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S
- Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift |Yershov, V. N., | Ap&SS | 354-97 | 2014 | 2014Ap&SS.354...97Y | http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y
- In-orbit performance of the soft X-ray imaging system aboard Hitomi (ASTRO-H) |Nakajima, Hiroshi, Maeda, Yoshitomo, et al. | PASJ | 70-21 | 2018 | 2018PASJ...70...21N | http://ui.adsabs.harvard.edu/#abs/2018PASJ...70...21N
- The Spectrum of the Universe |Hill, Ryley, Masui, Kiyoshi W., | ApSpe | 72-663 | 2018 | 2018ApSpe..72..663H | http://ui.adsabs.harvard.edu/#abs/2018ApSpe..72..663H
- 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
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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. |
