A dataset provided by the European Space Agency

Name: Unveiling the nature of cyclic behavior in the period evolution of XTEJ1810-197
Published: 2015-04-01T22:00:00Z

Proposal ID	072078
Title	Unveiling the nature of cyclic behavior in the period evolution of XTEJ1810-197
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720780201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720780301
DOI	https://doi.org/10.5270/esa-1crju52
Principal Investigator, PI	Dr Federico Bernardini
Abstract	This program is aimed at obtaining a phase-coherent timing solution for theperiod evolution of XTEJ1810-197 (XTEJ), and at continuing the successful XMMmonitoring of this unique Anomalous X-ray Pulsar (AXP). AXPs are Magnetars,isolated neutron star (NS) whose emission is due to the decay of a superstrongmagnetic field, 10e+(14-15) G. The requested pointings are aimed at studying theperiod evolution of XTEJ with the goal of demonstrating the presence of a longterm (5yr) precession of its rotation axis. XTEJ could be a unique precessingMagnetar (only 3 candidate precessing NSs are known). This would shed light onthe physical properties of the NS crust/core core and on the physical propertiesof matter at extremely high density. We request two pointings to complete the monitoring campaign.
Publications	Evolution of the X-Ray Properties of the Transient Magnetar XTE J1810-197 \|Alford, J. A. J., Halpern, J. P., \| ApJ \| 818-122 \| 2016 \| 2016ApJ...818..122A \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...818..122A The variable spin-down rate of the transient magnetar XTE J1810-197 \|Pintore, Fabio, Bernardini, Federico, et al. \| MNRAS \| 458-2088 \| 2016 \| 2016MNRAS.458.2088P \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.458.2088P Radio Disappearance of the Magnetar XTE J1810-197 and Continued X-ray Timing \|Camilo, F., Ransom, S. M., et al. \| ApJ \| 820-110 \| 2016 \| 2016ApJ...820..110C \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...820..110C ERRATUM: The variable spin-down rate of the transient magnetar XTE J1810-197. \|Pintore, Fabio, Bernardini, Federico, et al. \| MNRAS \| 459-3620 \| 2016 \| 2016MNRAS.459.3620P \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.459.3620P 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 Systematic study of magnetar outbursts \|Coti Zelati, Francesco, Rea, Nanda, et al. \| MNRAS \| 474-961 \| 2018 \| 2018MNRAS.474..961C \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.474..961C The 11 yr of low activity of the magnetar XTE J1810-197 \|Pintore, Fabio, Mereghetti, Sandro, et al. \| MNRAS \| 483-3832 \| 2019 \| 2019MNRAS.483.3832P \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.3832P Variable absorption line in XTE J1810-197 \|Vurgun, Eda, Chakraborty, Manoneeta, et al. \| NewA \| 67-45 \| 2019 \| 2019NewA...67...45V \| http://ui.adsabs.harvard.edu/#abs/2019NewA...67...45V 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 common fundamental plane of X-ray emissions from pulsars and magnetars in quiescence \|Chu, Che-Yen, Chang, Hsiang-Kuang, \| MNRAS \| 526-1287 \| 2023 \| 2023MNRAS.526.1287C \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.1287C 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	2013-09-05T19:45:54Z/2014-03-05T05:45:57Z
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	2015-04-01T22:00:00Z
Keywords	"period evolution", "xtej1810 197 xtej", "XMM", "shed light", "precessing magnetar", "ns crust", "rotation axis", "successful xmm", "physical properties", "xtej1810 197", "phase coherent", "superstrong magnetic field", "core core", "candidate precessing nss", "requested pointings", "term 5yr precession"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Federico Bernardini, 2015, 'Unveiling the nature of cyclic behavior in the period evolution of XTEJ1810-197', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-1crju52