A dataset provided by the European Space Agency

Name 067106
Title Unveiling the nature of cyclic behavior in the period evolution of XTEJ1810-197
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671060101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0671060201

DOI 10.5270/esa-b8u9kqx
Author Mr Federico Bernardini
Description The program is aimed at obtaining a phase-coherent timing solution for the period evolution of XTEJ1810-97 (XTE),continuing the successful X-ray monitoring of this unique Anomalous X-ray Pulsar (AXP).XTE is a transient magnetar, a neutron star (NS) whose quiescent emission is likely due to the decay of an extremely strong magnetic field (10e15 G).Previous analysis suggested a long term precession (2100 d) of the source spin axis.The pointings we request are aimed at studying the period evolution of XTE and prove the long term precession.XTE could be a unique precessing Magnetar.The effective presence of long-term precession could shed light on the physical properties of the NS crust-core, thus, on the physical properties of extremely high density matter
Publication 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 ,
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 ,
The variable spin-down rate of the transient magnetar XTE J1810-197 . Pintore, Fabio, Bernardini, Federico, et all. . MNRAS . 458-2088 . 2016 . 2016MNRAS.458.2088P ,
Radio Disappearance of the Magnetar XTE J1810-197 and Continued X-ray Timing . Camilo, F., Ransom, S. M., et all. . ApJ . 820-110 . 2016 . 2016ApJ...820..110C ,
ERRATUM: 'The variable spin-down rate of the transient magnetar XTE J1810-197. . Pintore, Fabio, Bernardini, Federico, et all. . MNRAS . 459-3620 . 2016 . 2016MNRAS.459.3620P ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Systematic study of magnetar outbursts . Coti Zelati, Francesco, Rea, Nanda, et all. . MNRAS . 474-961 . 2018 . 2018MNRAS.474..961C ,
The 11 yr of low activity of the magnetar XTE J1810-197 . Pintore, Fabio, Mereghetti, Sandro, et all. . MNRAS . 483-3832 . 2019 . 2019MNRAS.483.3832P ,
Variable absorption line in XTE J1810-197 . Vurgun, Eda, Chakraborty, Manoneeta, et all...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-04-03T00:39:35Z/2011-09-09T13:10:22Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2012-09-30T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-09-30T00:00:00Z, 067106, 17.56_20190403_1200. https://doi.org/10.5270/esa-b8u9kqx