From INTEGRAL and Swift surveys a significant fraction of hard X-ray sourceswere found to be magnetic Cataclysmic Variables(CVs) of the Intermediate Polar(IP) type. Optical follow-ups of virgul100 unidentified INTEGRAL sources show thatvirgul15% of the new detections have magnetic CV-like spectra. A timely question iswhether IPs provide an important contribution to the hard X-ray sky and hencestill represent a hidden population of galactic X-ray sources. We propose tocontinue our identification programme of newly discovered CVs, which are strongmagnetic candidates. The detection of X-ray pulses and the study of their broadband X-ray spectra will allow a firm identification of their nature and willprovide further insights in physics of this emerging class of accreting compact objects.
Publications
Very fast photometric and X-ray observations of the intermediate polar V2069 Cygni (RX J2123.7+4217) |Nasiroglu, I., Slowikowska, A., et al. | MNRAS | 420-3350 | 2012 | 2012MNRAS.420.3350N | http://ui.adsabs.harvard.edu/#abs/2012MNRAS.420.3350N
Exploring the end states of massive stars using the X-ray emission of neutron stars and supernova remnants |Prinz, Tobias, | PhDT | 0-305 | 2013 | 2013PhDT.......305P | http://ui.adsabs.harvard.edu/#abs/2013PhDT.......305P
A Study on White Dwarf Masses in Cataclysmic Variables Based on XMM-Newton and Suzaku Observations |Yu, Zhuo-Li, Xu, Xiao-Jie, | RAA | 22-45003 | 2022 | 2022RAA....22d5003Y | http://ui.adsabs.harvard.edu/#abs/2022RAA....22d5003Y
The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions |Pan, Zeyang, Qu, Zhijie, et al. | ApJS | 271-62 | 2024 | 2024ApJS..271...62P | http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P
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
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2009-04-30T10:45:58Z/2010-03-11T23:15:39Z
Version
17.56_20190403_1200
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.
European Space Agency, Dr Domitilla de Martino, 2011, 'X-ray characterization of INTEGRAL Cataclysmic Variable candidates', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-i2jis9s
