A dataset provided by the European Space Agency

Name: Unveiling the magnetic nature of new hard X-ray emitting CVs
Published: 2010-04-02T00:00:00Z

Proposal ID	055143
Title	Unveiling the magnetic nature of new hard X-ray emitting CVs
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551430301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551430401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0551430601
DOI	https://doi.org/10.5270/esa-gkk1pe9
Principal Investigator, PI	Dr Domitilla de Martino
Abstract	An unexpected large fraction of Cataclysmic Variables (CVs) has been identifiedas optical counterparts of hard X-ray sources in the INTEGRAL and Swift surveys.Most of them belong to the magnetic class of the Intermediate Polars (IPs),suggesting a potentially important role in the study of galactic populations ofX-ray sources. To date many new CVs still need to be properly classified. Herewe propose to observe 6 new hard X-ray CV systems to detect X-ray pulsations atthe white dwarf rotational period which, together with their spectralproperties, will provide firm constraints on their suspected magnetic nature.
Publications	The intriguing nature of the high-energy gamma ray source XSS J12270-4859 \|de Martino D. Falanga M. et al. \| A&A \| 515-25 \| 2010 \| 2010A&A...515A..25D \| http://ui.adsabs.harvard.edu/#abs/2010A&A...515A..25D Characterization of new hard X-ray cataclysmic variables \|Bernardini F. de Martino D. et al. \| A&A \| 542-22 \| 2012 \| 2012A&A...542A..22B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...542A..22B The bright unidentifiedgamma-ray source 1FGL J1227.9-4852: can it be associated with a low-mass X-ray binary? \|Hill A. B. Szostek A. et al. \| MNRAS \| 415-235 \| 2011 \| 2011MNRAS.415..235H \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.415..235H An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley David B. Shelton Robin L. \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H X-ray follow-ups of XSS J12270-4859: a low-mass X-ray binary with gamma-ray Fermi-LAT association \|de Martino D. Belloni T. et al. \| A&A \| 550-89 \| 2013 \| 2013A&A...550A..89D \| http://ui.adsabs.harvard.edu/#abs/2013A&A...550A..89D 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 Interaction of the Fermi Bubbles with the Milky Ways Hot Gas Halo \|Miller Matthew J. Bregman Joel N. \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M 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 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 X-ray study of high-and-low luminosity modes and peculiar low-soft-and-hard activity in the transitional pulsar XSS J12270-4859 \|Miraval Zanon A. Campana S. et al. \| A&A \| 635-30 \| 2020 \| 2020A&A...635A..30M \| http://ui.adsabs.harvard.edu/#abs/2020A&A...635A..30M An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu Zhijie Huang Rui et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q 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 Gamma-Ray Orbital Modulation of the Transitioning Millisecond Pulsar Binary XSS J12270-4859 \|An Hongjun \| ApJ \| 924-91 \| 2022 \| 2022ApJ...924...91A \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...924...91A The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu Zhijie Koutroumpa Dimitra et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q 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	2009-01-05T15:47:41Z/2009-03-19T01:39:41Z
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	2010-04-02T00:00:00Z
Last Update	2025-01-27
Keywords	"magnetic class", "swift surveys", "galactic populations", "properly classified", "suspected magnetic", "xray pulsations", "cataclysmic variables cvs", "firm constraints", "spectral properties", "intermediate polars ips", "xray sources", "optical counterparts", "hard xray sources"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Domitilla de Martino, 2010, 'Unveiling the magnetic nature of new hard X-ray emitting CVs', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-gkk1pe9