| 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
- Narrow absorption features in the co-added XMM-Newton RGS spectra of isolated neutron stars |Hohle, M. M., Haberl, F., et al. | MNRAS | 419-1525 | 2012 | 2012MNRAS.419.1525H | http://ui.adsabs.harvard.edu/#abs/2012MNRAS.419.1525H
- Modelling the spectral response of the Swift-XRT CCD camera: experience learnt from in-flight calibration |Godet, O., Beardmore, A. P., et al. | A&A | 494-775 | 2009 | 2009A&A...494..775G | http://ui.adsabs.harvard.edu/#abs/2009A&A...494..775G
- An All-Sky Atlas of Radio/X-ray Associations |Flesch, E., | PASA | 27-283 | 2010 | 2010PASA...27..283F | http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F
- 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 XMM-Newton serendipitous ultraviolet source survey catalogue |Page, M. J., Brindle, C., et al. | MNRAS | 426-903 | 2012 | 2012MNRAS.426..903P | http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P
- 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
- 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
- Timing the Nearby Isolated Neutron Star RX J1856.5-3754 |van Kerkwijk, M. H., Kaplan, D. L., | ApJ | 673-163 | 2008 | 2008ApJ...673L.163V | http://ui.adsabs.harvard.edu/#abs/2008ApJ...673L.163V
- Hard X-Ray Excess from the Magnificent Seven Neutron Stars |Dessert, Christopher, Foster, Joshua W., | ApJ | 904-42 | 2020 | 2020ApJ...904...42D | http://ui.adsabs.harvard.edu/#abs/2020ApJ...904...42D
- Axion Emission Can Explain a New Hard X-Ray Excess from Nearby Isolated Neutron Stars |Buschmann, Malte, Co, Raymond T., et al. | PhRvL | 126-21102 | 2021 | 2021PhRvL.126b1102B | http://ui.adsabs.harvard.edu/#abs/2021PhRvL.126b1102B
- 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
|
| 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. |
