A dataset provided by the European Space Agency

Name: Characterization of hard X-ray selected binaries: a census of magnetic CVs
Published: 2015-04-01T22:00:00Z

Proposal ID	072179
Title	Characterization of hard X-ray selected binaries: a census of magnetic CVs
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721790101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721790201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721790301
DOI	https://doi.org/10.5270/esa-w57qbsx
Principal Investigator, PI	Dr Domitilla de Martino
Abstract	Among hard X-ray galactic sources detected by the INTEGRAL and Swift surveysthose identified as white dwarf binaries (CVs) recently boosted in number. Themajority harbour asynchronously rotating magnetic primaries, suggesting thatthis subclass could be an important constituent of X-ray binary populations.XMM-Newton demonstrated its unique potential to unambiguously infer their truenature through the detection of X-ray spin pulses and the study of broad-bandspectra, that proved to be successful for more than 17 targets. We propose tocontinue our identification programme with the ultimate goal to obtain a truecensus of the first volume-limited sample of hard X-ray emitting white dwarfsystems.
Publications	Swift J2218.4+1925: a new hard-X-ray-selected polar observed with XMM-Newton \|Bernardini, F., de Martino, D., et al. \| MNRAS \| 445-1403 \| 2014 \| 2014MNRAS.445.1403B \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.445.1403B Swift J0525.6+2416 and IGR J04571+4527: two new hard X-ray-selected magnetic cataclysmic variables identified with XMM-Newton \|Bernardini, F., de Martino, D., et al. \| MNRAS \| 453-3100 \| 2015 \| 2015MNRAS.453.3100B \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.453.3100B 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 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 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 From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R 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	2013-11-25T19:06:55Z/2014-03-13T21:53:58Z
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.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2015-04-01T22:00:00Z
Keywords	"hard xray", "xray spin pulses", "XMM", "broad band spectra", "unambiguously infer", "xray binary populations", "identification programme", "XMM-Newton", "volume limited sample", "swift surveys", "magnetic cvs", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Domitilla de Martino, 2015, 'Characterization of hard X-ray selected binaries: a census of magnetic CVs', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-w57qbsx