A dataset provided by the European Space Agency

Name: XMM-Newton Observations of Five Eclipsing Binary Millisecond Pulsars
Published: 2017-07-07T22:00:00Z

Proposal ID	078353
Title	XMM-Newton Observations of Five Eclipsing Binary Millisecond Pulsars
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783530301
DOI	https://doi.org/10.5270/esa-xh5d2i1
Principal Investigator, PI	Prof Maura Mclaughlin
Abstract	We request XMM-Newton observations of five eclipsing binary millisecond pulsars(MSPs). All five have been detected with either Chandra or XMM-Newton and showorbital modulation consistent with intrabinary shock emission. The requestedobservations will enable us to model this variability over multiple full orbitsand derive constraints on the binary geometry and pulsar wind density andmagnetization. We will also be able to fit multi-component spectra to determinethe contributions from the MSPs themselves and the intrabinary shock. Thesestudies will lead to a better understanding of the population of these objectsand will also provide important constraints on the ablation and recyclingprocesses critical to MSP evolution scenarios.
Publications	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 A 350 MHz Green Bank Telescope Survey of Unassociated Fermi LAT Sources: Discovery and Timing of 10 Millisecond Pulsars \|Bangale, P., Bhattacharyya, B., et al. \| ApJ \| 966-161 \| 2024 \| 2024ApJ...966..161B \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...966..161B 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	2016-06-17T21:58:03Z/2016-06-18T13:13:03Z
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	2017-07-07T22:00:00Z
Keywords	"intrabinary shock", "recycling processes", "intrabinary shock emission", "XMM", "binary geometry", "msp evolution scenarios", "pulsar wind density", "XMM-Newton", "orbital modulation", "msps themselves", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Maura Mclaughlin, 2017, 'XMM-Newton Observations of Five Eclipsing Binary Millisecond Pulsars', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-xh5d2i1