A dataset provided by the European Space Agency

Name: Characterizing the X-ray properties of a new intriguing binary system
Published: 2012-03-30T00:00:00Z

Proposal ID	065383
Title	Characterizing the X-ray properties of a new intriguing binary system
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653830101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653830201
DOI	https://doi.org/10.5270/esa-sqxg6jq
Principal Investigator, PI	Dr Andrea Possenti
Abstract	PSR J1723-28 may represent the second known case (after PSR J1023+0038;Archibald et al. 2009, Science) of a just-formed baby millisecond pulsar.That provides unprecedented possibilities for investigating the last stages ofthe so-called recycling process and the related activation of a millisecondpulsar. In the framework of a large multiwavelength campaign, we request here a55 ks exposure (thus sampling a full orbit of PSR J1723-28) in order to: (i)firmly establishing the X-ray counterpart to the binary; (ii) investigating thenature of the X-ray emission; (iii) constraining the distribution of plasma inthe system and the geometry of the X-ray emission, thanks to the comparision ofthe variability simultaneously observed in the X-ray emission and in the pulsed radio emission.
Publications	Exploring the X-Ray and gamma-Ray Properties of the Redback Millisecond Pulsar PSR J1723-2837 \|Hui C. Y. Tam P. H. T. et al. \| ApJ \| 781-21 \| 2014 \| 2014ApJ...781L..21H \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...781L..21H X-Ray and gamma-Ray Studies of the Millisecond Pulsar and Possible X-Ray Binary/Radio Pulsar Transition Object PSR J1723-2837 \|Bogdanov Slavko Esposito Paolo et al. \| ApJ \| 781-6 \| 2014 \| 2014ApJ...781....6B \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...781....6B 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 Strengthening the bounds on the r-mode amplitude with X-ray observations of millisecond pulsars \|Boztepe Tuu011fba Gu00f6u011fu00fcu0219 Ersin et al. \| MNRAS \| 498-2734 \| 2020 \| 2020MNRAS.498.2734B \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.498.2734B 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	2011-03-03T10:58:47Z/2011-03-04T04:40:11Z
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	2012-03-30T00:00:00Z
Last Update	2025-01-27
Keywords	"ii investigating", "intriguing binary system", "millisecond pulsar", "xray counterpart", "xray properties", "pulsed radio emission", "psr j1023", "related activation", "xray emission", "multiwavelength campaign", "psr j1723", "iii constraining"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Andrea Possenti, 2012, 'Characterizing the X-ray properties of a new intriguing binary system', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-sqxg6jq