A dataset provided by the European Space Agency

Name: Characterization of hard X-ray selected binaries: a census of magnetic CVs
Published: 2013-05-15T00:00:00Z

Proposal ID	067185
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=0671850201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671850301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671850601
DOI	https://doi.org/10.5270/esa-226vz0x
Principal Investigator, PI	Dr Domitilla de Martino
Abstract	The INTEGRAL and SWIFT satellites detected a large number of galactic X-raysources above 20keV,among which ~6-7% identified as accreting white dwarfbinaries. Among known systems most harbour asynchronously rotating magneticprimaries, suggesting that this formerly small subclass could be an importantcontributor to the galactic X-ray binary populations. However, most newlydiscovered sources are proposed as magnetic cataclysmic variables throughoptical spectra. XMM-Newton demonstrated unique potential to infer their truenature through the detection of X-ray pulses and study of broad-band spectra. Wepropose 6 new sources that, if all confirmed as magnetics, will increase by 35%the hard X-ray sample enabling a true census of the first volume-limited sample
Publications	On the nature of the hard X-ray sources SWIFT J1907.3-2050 IGR J12123-5802 and IGR J19552+0044 \|Bernardini F. de Martino D. et al. \| MNRAS \| 435-2822 \| 2013 \| 2013MNRAS.435.2822B \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.435.2822B Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y 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 V1082-Sgr: A magnetic cataclysmic variable with a lobe-filling companion star \|Xu Xiaojie Shao Yong \| MNRAS \| 489-3031 \| 2019 \| 2019MNRAS.489.3031X \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489.3031X 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 The EXTraS project: Exploring the X-ray transient and variable sky \|De Luca A. Salvaterra R. et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D 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 Classifying the high-energy sky with spectral and timing methods \|Kreikenbohm Annika \| PhDT \| 0-105 \| 2019 \| 2019PhDT.......105K \| http://ui.adsabs.harvard.edu/#abs/2019PhDT.......105K Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-01-07T15:25:52Z/2012-04-29T15:56:29Z
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	2013-05-15T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "hard xray", "XMM-Newton", "broad band spectra", "hard xray sample", "magnetic cvs", "volume limited sample", "xmm newton", "swift satellites", "xray pulses", "optical spectra", "galactic xray sources", "magnetic cataclysmic variables"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Domitilla de Martino, 2013, '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-226vz0x