No abstract found for current proposal (This is a scientific proposal for an ESA mission. For specific information please contact ESDC Helpdesk - https://support.cosmos.esa.int/esdc)
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 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
A Search for New Galactic Magnetars in Archival Chandra and XMM-Newton Observations |Muno M. P. Gaensler B. M. et al. | ApJ | 680-639 | 2008 | 2008ApJ...680..639M | http://ui.adsabs.harvard.edu/#abs/2008ApJ...680..639M
Nonthermal emission properties of the northwestern rim of supernova remnant RX J0852.0-4622 |Kishishita T. Hiraga J. | A&A | 551-132 | 2013 | 2013A&A...551A.132K | http://ui.adsabs.harvard.edu/#abs/2013A&A...551A.132K
Sunyaev-Zeldovich 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
A survey of stellar X-ray flares from the XMM-Newton serendipitous source catalogue: HIPPARCOS-Tycho cool stars |Pye J. P. Rosen S. et al. | A&A | 581-28 | 2015 | 2015A&A...581A..28P | http://ui.adsabs.harvard.edu/#abs/2015A&A...581A..28P
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
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
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.
European Space Agency, Dr Fred Jansen XMM-Newton PS, 2003, 'EPIC routine calibration proposal: Vela SNR', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-8za1ehz
