A dataset provided by the European Space Agency

Name 060599
Title Unveiling the nature of the Period evolution of XTE J180-197
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605990201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605990301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605990401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605990501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605990601

DOI 10.5270/esa-47oolvz
Author Mr Federico Bernardini
Description This program is aimed at obtaining a phase coherent time solution for the period evolution of XTE J1810-197, and concluding the successful XMM monitoring of this unique Anomalous X--ray Pulsar (AXP).This source was identified as the first transient AXP in 2003.The transient X--ray behavior of this source (outburst flux increase of a factor 100) allowed us to monitor his time properties for a long time (5 yrs 9 obs.).In 2006 this source was also found to be a bright and highly polarized transient radio pulsar, a unique property among both AXPs and radio pulsars (RPs).The last pointings we requested are aimed at studying his time evolution, and checking the presence of a precession.This could be the unique Magnetar and one of the very few (3) neutron stars showing a precession period.
Publication Emission geometry, radiation pattern and magnetic topology of the magnetar XTE J1810-197 in its quiescent state . Bernardini, F., Perna, R., et all. . MNRAS . 418-638 . 2011 . 2011MNRAS.418..638B ,
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 X...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2009-09-05T14:28:01Z/2010-09-05T18:54:19Z
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 2011-09-23T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2011-09-23T00:00:00Z, 060599, 17.56_20190403_1200. https://doi.org/10.5270/esa-47oolvz