A dataset provided by the European Space Agency

Name: Characterization of hard X-ray selected binaries:a census of magnetic CVs
Published: 2017-04-14T22:00:00Z

Proposal ID	076112
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=0761120101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761120201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761120301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761120401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761120501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761120701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761120801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0761120901
DOI	https://doi.org/10.5270/esa-kwioxdz
Principal Investigator, PI	Dr Domitilla de Martino
Abstract	A large number of hard X-ray galactic sources are detected in the INTEGRAL andSwift surveys, among them virgul20percent are accreting white dwarf (WD) binaries(CVs). The majority harbours asynchronously rotating magnetic primaries, whichnowdays are disputed to be the dominant galactic population of low-luminosityX-ray sources. While optical follow-ups allow to find magnetic CV candidates,asecure identification of their true nature resides in the X-rays. WithXMM-Newton we could successfully prove or disprove the magnetic nature for 24sources. We here propose to continue our identification programme with 8 newcandidates with the ultimate goal to obtain a true census of the firstvolume-limited sample of hard X-ray CVs.
Publications	Broad-band characteristics of seven new hard X-ray selected cataclysmic variables \|Bernardini, F., de Martino, D., et al. \| MNRAS \| 470-4815 \| 2017 \| 2017MNRAS.470.4815B \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470.4815B 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 Timing analysis of a sample of five cataclysmic variable candidates observed by the XMM-Newton satellite \|Nucita, A. A., Lezzi, S. M., et al. \| MNRAS \| 517-118 \| 2022 \| 2022MNRAS.517..118N \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517..118N 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	2015-05-05T05:32:23Z/2016-04-01T18:06:38Z
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	2017-04-14T22:00:00Z
Keywords	"hard xray", "hard xray cvs", "magnetic cv candidates", "XMM", "secure identification", "successfully prove", "identification programme", "XMM-Newton", "dominant galactic population", "volume limited sample", "swift surveys", "magnetic cvs", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Domitilla de Martino, 2017, '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-kwioxdz