A dataset provided by the European Space Agency

Name: XMM observations of fast spinning HXRTs quiescence
Published: 2008-09-27T00:00:00Z

Proposal ID	050528
Title	XMM observations of fast spinning HXRTs quiescence
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0505280101
DOI	https://doi.org/10.5270/esa-xwqsbp5
Principal Investigator, PI	Dr Sergio Campana
Abstract	We propose XMM-Newton observations of two hard X--ray transients containing fastspinning and/or high magnetic field neutron stars to probe their quiescentemission. Due to their faintness these sources are likely in a regime which doesnot allow matter to fall directly onto the neutron star surface (propellerstate). The proposed observations will allow us to study 4U 0115+63 and V0332+53at the deepest levels ever observed for this class of sources to shed light onthe physics of the disk-magnetosphere interaction and on the heating of themagnetic polar caps in the high magnetic field regime.
Publications	An All-Sky Atlas of Radio/X-ray Associations \|Flesch E. \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin Dacheng Webb Natalie A. \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L The diversity of quasars unified by accretion and orientation \|Shen Yue Ho Luis C. \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 The X-ray properties of Be/X-ray pulsars in quiescence \|Tsygankov Sergey S. Wijnands Rudy et al. \| MNRAS \| 470-126 \| 2017 \| 2017MNRAS.470..126T \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470..126T Recurrent low-level luminosity behaviour after a giant outburst in the Be/X-ray transient 4U 0115+63 \|Rouco Escorial A. Wijnands R. et al. \| A&A \| 638-152 \| 2020 \| 2020A&A...638A.152R \| http://ui.adsabs.harvard.edu/#abs/2020A&A...638A.152R 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 Three-dimensional Velocity Diagnostics to Constrain the Type Ia Origin of Tychos Supernova Remnant \|Uchida Hiroyuki Kasuga Tomoaki et al. \| ApJ \| 962-159 \| 2024 \| 2024ApJ...962..159U \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...962..159U 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	2007-07-21T01:20:27Z/2007-07-21T10:05:39Z
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	2008-09-27T00:00:00Z
Keywords	"magnetic polar caps", "deepest levels", "4u 0115", "XMM", "magnetic field regime", "xmm newton", "disk magnetosphere interaction", "shed light", "quiescent emission", "XMM-Newton", "fast spinning"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Sergio Campana, 2008, 'XMM observations of fast spinning HXRTs quiescence', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xwqsbp5