Rout. Cal.: 3x5 ks in single orbit (Prop. was 16096).Special RGS setup defined in obs 1, 2, 3 for all observations (no Refresh DIPPV)
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
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
The relative and absolute timing accuracy of the EPIC-pn camera on XMM-Newton from X-ray pulsations of the Crab and other pulsars |Martin-Carrillo A. Kirsch M. G. F. et al. | A&A | 545-126 | 2012 | 2012A&A...545A.126M | http://ui.adsabs.harvard.edu/#abs/2012A&A...545A.126M
A systematic cross-search for radio/infrared counterparts of XMM- Newton sources |Combi J. A. Albacete Colombo J. F. et al. | Ap&SS | 331-53 | 2011 | 2011Ap&SS.331...53C | http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C
Revealing the broad iron Kalpha line in Cygnus X-1 through simultaneous XMM-Newton RXTE and INTEGRAL observations |Duro Refiz Dauser Thomas et al. | A&A | 589-14 | 2016 | 2016A&A...589A..14D | http://ui.adsabs.harvard.edu/#abs/2016A&A...589A..14D
Morphological Properties of the Crab Nebula: A Detailed Multiwavelength Study Based on New VLA HST Chandra and XMM-Newton Images |Dubner G. Castelletti G. et al. | ApJ | 840-82 | 2017 | 2017ApJ...840...82D | http://ui.adsabs.harvard.edu/#abs/2017ApJ...840...82D
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 Arvind Parmar XMM-Newton MM, 2009, 'Timing verification with the Crab', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-jzlpjhi
