A dataset provided by the European Space Agency

Name: Testing Reflection in Intermediate Polars: Joint XMM-Newton+NuSTAR Observations
Published: 2015-10-02T22:00:00Z

Proposal ID	074312
Title	Testing Reflection in Intermediate Polars: Joint XMM-Newton+NuSTAR Observations
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743120101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743120301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743120401
DOI	https://doi.org/10.5270/esa-hgb5r5v
Principal Investigator, PI	Dr Koji Mukai
Abstract	We propose joint XMM-Newton and NuSTAR observations of 3 intermediate polars(IPs) to test our understanding of reflection, widely observed in accretingbinaries and in active galactic nuclei. A physical fit requires a consistenttreatment of the reflection bump and the 6.4 keV line, but only the latter hasbeen reliably observed in IPs to date. We will fit the phase-averaged spectra ofour targets to derive the reflection amplitude. We will also measure the spinmodulation in the reflection component in IPs for the first time. This will helpverify the theory of angle dependent reflection, help break any remainingdegeneracy in fitting the phase-averaged spectra, and allow us to determine thesystem geometry of individual IPs with non-sinusoidal X-ray spin modulations.
Publications	Unambiguous Detection of Reflection in Magnetic Cataclysmic Variables: Joint NuSTAR-XMM-Newton Observations of Three Intermediate Polars \|Mukai, K., Rana, V., et al. \| ApJ \| 807-30 \| 2015 \| 2015ApJ...807L..30M \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...807L..30M 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 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	2014-07-07T04:19:14Z/2014-09-16T06:53:30Z
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	2015-10-02T22:00:00Z
Keywords	"NuSTAR", "reflection component", "XMM-Newton", "xmm newton", "reflection amplitude", "kev line", "XMM", "testing reflection", "spin modulation", "system geometry", "accreting binary", "intermediate polars ips", "individual ips", "reflection bump", "intermediate polars", "active galactic nuclei", "angle dependent reflection", "physical fit", "phase averaged spectra"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Koji Mukai, 2015, 'Testing Reflection in Intermediate Polars: Joint XMM-Newton+NuSTAR Observations', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hgb5r5v