| Publications |
- 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 XMM Cluster Survey: optical analysis methodology and the first data release |Mehrtens, Nicola, Romer, A. Kathy, et al. | MNRAS | 423-1024 | 2012 | 2012MNRAS.423.1024M | http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M
- Mining for normal galaxies in the first XMM-Newton Serendipitous Source Catalog |Georgakakis, A. E., Chavushyan, V., et al. | MNRAS | 367-1017 | 2006 | 2006MNRAS.367.1017G | http://ui.adsabs.harvard.edu/#abs/2006MNRAS.367.1017G
- The XMM Cluster Survey: X-ray analysis methodology |Lloyd-Davies, E. J., Romer, A. Kathy, et al. | MNRAS | 418-14 | 2011 | 2011MNRAS.418...14L | http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L
- Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters |Xiao, Weike, Chen, Chen, et al. | MNRAS | 432-41 | 2013 | 2013MNRAS.432L..41X | http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X
- 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
- Anisotropy of the galaxy cluster X-ray luminosity-temperature relation |Migkas, Konstantinos, Reiprich, Thomas H., | A&A | 611-50 | 2018 | 2018A&A...611A..50M | http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M
- The XMM Cluster Survey: Present status and latest results |Viana, P. T. P., Mehrtens, N., et al. | AN | 334-462 | 2013 | 2013AN....334..462V | http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V
- Testing emergent gravity on galaxy cluster scales |Tamosiunas, Andrius, Bacon, David, et al. | JCAP | 5-53 | 2019 | 2019JCAP...05..053T | http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T
- Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline |Hollowood, Devon L., Jeltema, Tesla, et al. | ApJS | 244-22 | 2019 | 2019ApJS..244...22H | http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H
- Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters |Palmese, A., Annis, J., et al. | MNRAS | 493-4591 | 2020 | 2020MNRAS.493.4591P | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P
- 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. |
