A dataset provided by the European Space Agency

Name: Probing the Accretion History of the Transition Object PSR J1023+0038
Published: 2015-06-30T22:00:00Z

Proposal ID	074261
Title	Probing the Accretion History of the Transition Object PSR J1023+0038
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0742610101
DOI	https://doi.org/10.5270/esa-e5kgpak
Principal Investigator, PI	Dr Slavko Bogdanov
Abstract	The extraordinary binary radio millisecond pulsar PSR J1023+0038 is a missinglink between low-mass X-ray binaries and rotation-powered millisecond pulsars.In the past few months it has ceased emission in the radio, possibly because ithas reverted back to an X-ray binary phase. We propose a monitoringspectroscopic and timing study of this system to look for the signature ofongoing or recent accretion in this system in the pulsed thermal emission fromthe neutron star. This investigation may offer unique insight into thetransition process of millisecond pulsars from accretion to rotation power.
Publications	Coordinated X-Ray Ultraviolet Optical and Radio Observations of the PSR J1023+0038 System in a Low-mass X-Ray Binary State \|Bogdanov Slavko Archibald Anne M. et al. \| ApJ \| 806-148 \| 2015 \| 2015ApJ...806..148B \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...806..148B Accretion-powered Pulsations in an Apparently Quiescent Neutron Star Binary \|Archibald Anne M. Bogdanov Slavko et al. \| ApJ \| 807-62 \| 2015 \| 2015ApJ...807...62A \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...807...62A A physical scenario for the high and low X-ray luminosity states in the transitional pulsar PSR J1023+0038 \|Campana S. Coti Zelati F. et al. \| A&A \| 594-31 \| 2016 \| 2016A&A...594A..31C \| http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..31C Timing Observations of PSR J1023+0038 During a Low-mass X-Ray Binary State \|Jaodand Amruta Archibald Anne M. et al. \| ApJ \| 830-122 \| 2016 \| 2016ApJ...830..122J \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...830..122J Simultaneous broadband observations and high-resolution X-ray spectroscopy of the transitional millisecond pulsar PSR J1023+0038 \|Coti Zelati F. Campana S. et al. \| A&A \| 611-14 \| 2018 \| 2018A&A...611A..14C \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..14C The First Continuous Optical Monitoring of the Transitional Millisecond Pulsar PSR J1023+0038 with Kepler \|Papitto A. Rea N. et al. \| ApJ \| 858-12 \| 2018 \| 2018ApJ...858L..12P \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...858L..12P Probing X-ray emission in different modes of PSR J1023+0038 with a radio pulsar scenario \|Campana S. Miraval Zanon A. et al. \| A&A \| 629-8 \| 2019 \| 2019A&A...629L...8C \| http://ui.adsabs.harvard.edu/#abs/2019A&A...629L...8C Spin-down rate of the transitional millisecond pulsar PSR J1023+0038 in the optical band with Aqueye+ \|Burtovoi Aleksandr Zampieri Luca et al. \| MNRAS \| 498-98 \| 2020 \| 2020MNRAS.498L..98B \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.498L..98B 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 UV and X-ray pulse amplitude variability in the transitional millisecond pulsar PSR J1023+0038 \|Miraval Zanon A. Ambrosino F. et al. \| A&A \| 660-63 \| 2022 \| 2022A&A...660A..63M \| http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..63M X-ray variability of transitional millisecond pulsars: a faint stable and fluctuating disc \|Linares Manuel De Marco Barbara et al. \| MNRAS \| 512-5269 \| 2022 \| 2022MNRAS.512.5269L \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.512.5269L 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	2014-06-10T03:27:28Z/2014-06-11T15:52:28Z
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	2015-06-30T22:00:00Z
Last Update	2025-01-27
Keywords	"xray binary phase", "ceased emission", "pulsed thermal emission", "transition process", "rotation power", "neutron star", "accretion history", "millisecond pulsars"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Slavko Bogdanov, 2015, 'Probing the Accretion History of the Transition Object PSR J1023+0038', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-e5kgpak