A dataset provided by the European Space Agency

Name: Unveiling the nature of five new discovered X-ray pulsators
Published: 2014-10-12T00:00:00Z

Proposal ID	072357
Title	Unveiling the nature of five new discovered X-ray pulsators
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723570201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723570401
DOI	https://doi.org/10.5270/esa-p5v8j90
Principal Investigator, PI	Dr GianLuca Israel
Abstract	During a systematic search (the largest ever in the high energy band) forcoherent periodicities in about 400,000 light curves of serendipitous sourcesdetected by Swift X-Ray Telescope (XRT) and Chandra Advanced CCD ImagingSpectrometer (ACIS) we identified (the project is still on-going) 26 new X-raypulsators. In this proposal we ask for XMM-Newton follow-up observations forfive of them, which either show unusual properties or are not covered by furtherarchival data. The requested observations will allow us to unveil their nature.We also expect to identify new classes of neutron stars and white dwarfs and/orextending our understanding of the physics of accretion toward lowerluminosities.
Publications	The X-ray emission of the high-mass X-ray binary IGR J17200-3116 \|Esposito P. Israel G. L. et al. \| MNRAS \| 441-1126 \| 2014 \| 2014MNRAS.441.1126E \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.441.1126E The Chandra ACIS Timing Survey Project: glimpsing a sample of faint X-ray pulsators \|Israel G. L. Esposito P. et al. \| MNRAS \| 462-4371 \| 2016 \| 2016MNRAS.462.4371I \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.462.4371I 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 Spectroscopic identification of INTEGRAL high-energy sources with VLT/ISAAC \|Fortin F. Chaty S. et al. \| A&A \| 618-150 \| 2018 \| 2018A&A...618A.150F \| http://ui.adsabs.harvard.edu/#abs/2018A&A...618A.150F 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 The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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	2013-09-19T02:49:32Z/2013-09-30T12:08:14Z
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	2014-10-12T00:00:00Z
Last Update	2025-01-27
Keywords	"000 light curves", "xray pulsators", "neutron stars", "white dwarfs", "xmm newton", "systematic search", "coherent periodicities", "XMM-Newton", "lower luminosities", "XMM", "archival data", "energy band"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr GianLuca Israel, 2014, 'Unveiling the nature of five new discovered X-ray pulsators', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-p5v8j90