A dataset provided by the European Space Agency

Name: Orbitally Resolved Spectral Studies of Three Eclipsing Millisecond Pulsars
Published: 2014-11-13T00:00:00Z

Proposal ID	072507
Title	Orbitally Resolved Spectral Studies of Three Eclipsing Millisecond Pulsars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0725070101
DOI	https://doi.org/10.5270/esa-2c4ci0b
Principal Investigator, PI	Dr Mallory Roberts
Abstract	We propose to observe three recently discovered eclipsing millisecond pulsars,two redbacks and one black widow, in order to characterize their X-rayemission as a function of orbital phase as a probe of their intrabinary shocks.These may be the best systems to probe the magnetization of pulsar winds as afunction of distance from the magnetosphere, and perhaps give some observationalguidance to magnetic field suppression during accretion. We also wish to obtaingood quality UV light curves to complement ground based optical work of theheated companions and search for potential UV emission from the shock.
Publications	Exploring the Intrabinary Shock from the Redback Millisecond Pulsar PSR J2129-0429 \|Hui C. Y. Hu C. P. et al. \| ApJ \| 801-27 \| 2015 \| 2015ApJ...801L..27H \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...801L..27H 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 Broad-band high-energy emissions of the redback millisecond pulsar PSR J2129-0429 \|Kong Albert K. H. Takata Jumpei et al. \| MNRAS \| 478-3987 \| 2018 \| 2018MNRAS.478.3987K \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478.3987K X-Ray and Optical Studies of the Redback System PSR J2129-0429 \|Al Noori Hind Roberts Mallory S. E. et al. \| ApJ \| 861-89 \| 2018 \| 2018ApJ...861...89A \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...861...89A 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 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	2013-10-28T08:37:03Z/2013-10-29T06:58:43Z
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	2014-11-13T00:00:00Z
Last Update	2025-01-27
Keywords	"", "magnetic field suppression", "pulsar winds", "orbital phase", "intrabinary shoc", "potential uv emission", "complement ground", "black widow "", "eclipsing millisecond pulsars", "orbitally resolved spectral", "xray emission", "heated companions"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Mallory Roberts, 2014, 'Orbitally Resolved Spectral Studies of Three Eclipsing Millisecond Pulsars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2c4ci0b