A dataset provided by the European Space Agency

Name: PSR J1023+0038: a tool to investigate the accretion and ejection in LMXBs
Published: 2018-07-27T22:00:00Z

Proposal ID	078470
Title	PSR J1023+0038: a tool to investigate the accretion and ejection in LMXBs
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784700201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784700301
DOI	https://doi.org/10.5270/esa-89dzpot
Principal Investigator, PI	Dr Sergio Campana
Abstract	PSR J1023+0038 is a binary system that hosts a neutron star and a low-mass, mainsequence companion star. It has been observed to switch on timescales of yearsbetween states as a radio millisecond pulsar and a LMXB. After its last switchto an X-ray state in 2013, the source has been the object of an extensivemulti-wavelength monitoring, during which the switch between three flux X-raymodes (high, low and flare) on timescales of 10 s has been observed. Here wepropose a model to account for these switches and ask for the first strictlysimultaneous NuSTAR-EPIC-Swift-OM-VLT observation to probe our model usingcorrelations and lags (a profitable tool to probe the emission mechanism), aswell as establish differences among the power spectra of the multi-band light curves.
Publications	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 Peering at the outflow mechanisms in the transitional pulsar PSR J1023+0038: simultaneous VLT XMM-Newton and Swift high-time resolution observations \|Baglio M. C. Vincentelli F. et al. \| A&A \| 631-104 \| 2019 \| 2019A&A...631A.104B \| http://ui.adsabs.harvard.edu/#abs/2019A&A...631A.104B 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 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 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 Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-05-08T03:29:38Z/2017-06-10T05:04:43Z
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	2018-07-27T22:00:00Z
Last Update	2025-08-04
Keywords	"NuSTAR", "psr j1023", "radio millisecond pulsar", "binary system", "neutron star", "profitable tool", "EPIC", "emission mechanism", "power spectra", "low mass", "flux xray modes", "extensive multi wavelength"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Sergio Campana, 2018, 'PSR J1023+0038: a tool to investigate the accretion and ejection in LMXBs', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-89dzpot