A dataset provided by the European Space Agency

Name: Timing and spectral observation of 1RXS J171824.2-402934
Published: 2011-03-27T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	060516
Title	Timing and spectral observation of 1RXS J171824.2-402934
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605160101
DOI	https://doi.org/10.5270/esa-k06sd4q
Principal Investigator, PI	Mrs Alessandro Patruno
Abstract	We propose to perform an {it XMM-Newton} observation of the very faint neutronstar low mass X-ray binary 1RXS J171824.2-402934 to investigate the presence ofa coherent pulsation in the persistent emission of the source. In case ofdetection this will be the first ever detected persistent source with pulsedemission from an accreting neutron star. In case of non detection theobservation will be a emph{crucial experiment} to select current theories ofpulse formation. We will also perform for the first time an aperiodic timinganalysis to search for quasi periodic oscillations that if detected, will giveus precious information about the physics of the system. A spectral study willbe also be performed improving previous Chandra observations.
Publications	The X-ray spectral properties of very-faint persistent neutron star X-ray binaries \|Armas Padilla M. Degenaar N. \| MNRAS \| 434-1586 \| 2013 \| 2013MNRAS.434.1586A \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.434.1586A 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 Revealing the broad iron Kalpha line in Cygnus X-1 through simultaneous XMM-Newton RXTE and INTEGRAL observations \|Duro Refiz Dauser Thomas et al. \| A&A \| 589-14 \| 2016 \| 2016A&A...589A..14D \| http://ui.adsabs.harvard.edu/#abs/2016A&A...589A..14D 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 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 Possible Detection of X-Ray Emitting Circumstellar Material in the Synchrotron-dominated Supernova Remnant RX J1713.7-3946 \|Tateishi Dai Katsuda Satoru et al. \| ApJ \| 923-187 \| 2021 \| 2021ApJ...923..187T \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...923..187T 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2010-03-13T13:33:41Z/2010-03-14T10:53:58Z
Version	21.51_20241115_1113
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	2011-03-27T00:00:00Z
Last Update	2026-07-09
Keywords	"coherent pulsation", "precious information", "accreting neutron star", "XMM-Newton", "persistent source", "pulsed emission", "persistent emission", "quasi periodic oscillations", "1rxs j171824", "XMM", "pulse formation", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mrs Alessandro Patruno, 2011, 'Timing and spectral observation of 1RXS J171824.2-402934', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-k06sd4q
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.