A dataset provided by the European Space Agency

Name: Unveiling the quiescent state properties of the transient AXP XTE J1810-197
Published: 2008-10-26T00:00:00Z

Proposal ID	050465
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=0504650201
DOI	https://doi.org/10.5270/esa-4v4ewt1
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, and for a unified scheme for isolated neutron stars (NSs) encompassing dissimilar classes.
Publications	From outburst to quiescence: the decay of the transient AXP XTE J1810-197 \|Bernardini, F., Israel, G. L., et al. \| A&A \| 498-195 \| 2009 \| 2009A&A...498..195B \| http://ui.adsabs.harvard.edu/#abs/2009A&A...498..195B A Unified Timing and Spectral Model for the Anomalous X-ray Pulsars XTE J1810-197 and CXOU J164710.2-455216 \|Albano, A., Turolla, R., et al. \| ApJ \| 722-788 \| 2010 \| 2010ApJ...722..788A \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...722..788A The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S 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 Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X 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 Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V 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 Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P 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	2007-09-16T00:59:09Z/2007-09-16T21:48:07Z
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	2008-10-26T00:00:00Z
Keywords	"rosetta stone", "XMM", "emission mechanism", "unified scheme", "xte j1810 197", "transient xray", "flux levels", "spectral properties", "source represents", "xmm program", "broad band emission", "property amongst axps"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr GianLuca Israel, 2008, '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-4v4ewt1