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
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	2025-01-27
Keywords	"hard xray sample", "xray pulses", "hard xray", "magnetic cvs", "galactic xray sources", "xmm newton", "broad band spectra", "XMM-Newton", "optical spectra", "swift satellites", "XMM", "magnetic cataclysmic variables", "volume limited sample"
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