A dataset provided by the European Space Agency

Name: Unveiling the quiescent state properties of the transient AXP XTE J1810-197
Published: 2010-03-26T00:00:00Z

Proposal ID	055280
Title	Unveiling the quiescent state properties of the transient AXP XTE J1810-197
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552800201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552800301
DOI	https://doi.org/10.5270/esa-mbwe2nz
Principal Investigator, PI	Dr GianLuca Israel
Abstract	This XMM program is aimed at studying the quiescent state of the Anomalous X-rayPulsar (AXP) XTE J1810-197. The transient X-ray behaviour of this source ismaking possible to study its properties over an unprecedented range of fluxlevels and energies. Moreover, the recent detetion of XTE J1810-197 as one ofthe brightest (fading) radio pulsars (a unique property amongst AXPs) make evenmore compelling the need of carrying out simultaneous multiwavelengthobservations and of considering its broad band emission as a whole whenmodelling the timing and spectral properties. Thus, this source represents aRosetta stone for our understanding of the nature and emission mechanism ofAXPs.
Publications	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 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 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	2009-03-05T13:13:30Z/2009-03-06T09:31:22Z
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	2010-03-26T00:00:00Z
Last Update	2025-01-27
Keywords	"broad band emission", "flux levels", "xmm program", "source represents", "emission mechanism", "transient xray", "spectral properties", "rosetta stone", "property amongst axps", "xte j1810 197", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr GianLuca Israel, 2010, 'Unveiling the quiescent state properties of the transient AXP XTE J1810-197', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-mbwe2nz