A dataset provided by the European Space Agency

Name: Unveiling the nature of newly discovered X-ray pulsators
Published: 2015-09-19T22:00:00Z

Proposal ID	074398
Title	Unveiling the nature of newly discovered X-ray pulsators
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743980101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743980301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743980401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0743980501
DOI	https://doi.org/10.5270/esa-5j94yy7
Principal Investigator, PI	Prof GianLuca Israel
Abstract	In the largest ever systematic search in soft X-rays for coherent periodicitiesabout 400,000 light curves of sources serendipitously detected by the SwiftX-Ray Telescope (XRT) and the Chandra Advanced CCD Imaging Spectrometer (ACIS)we have discovered so far (the project is still on-going) 35 new X-raypulsators. In this proposal we ask for XMM-Newton follow-up observations forfive of them, which either show unusual characteristics or their properties aresuggesting the presence of an accreting neutron star. The requested observationswill allow us to unveil their nature and test magnetic gating accretionscenarios, a regime which has remained unexplored so far.
Publications	Swift J201424.9+152930: discovery of a new deeply eclipsing binary with 491-s and 3.4-h modulations \|Esposito, P., Israel, G. L., et al. \| MNRAS \| 450-1705 \| 2015 \| 2015MNRAS.450.1705E \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.450.1705E 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 classification of X-ray sources in the Galactic Bulge Survey \|Wevers, T., Torres, M. A. P., et al. \| MNRAS \| 470-4512 \| 2017 \| 2017MNRAS.470.4512W \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470.4512W X-ray chimneys in the Galactic Centre \|Chernyakova, Masha, \| Natur \| 567-318 \| 2019 \| 2019Natur.567..318C \| http://ui.adsabs.harvard.edu/#abs/2019Natur.567..318C An X-ray chimney extending hundreds of parsecs above and below the Galactic Centre \|Ponti, G., Hofmann, F., et al. \| Natur \| 567-347 \| 2019 \| 2019Natur.567..347P \| http://ui.adsabs.harvard.edu/#abs/2019Natur.567..347P A Comparison of the X-Ray Properties of FU Ori-type Stars to Generic Young Stellar Objects \|Kuhn, Michael A., Hillenbrand, Lynne A., \| ApJ \| 883-117 \| 2019 \| 2019ApJ...883..117K \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...883..117K The Galactic center chimneys: the base of the multiphase outflow of the Milky Way \|Ponti, G., Morris, M. R., et al. \| A&A \| 646-66 \| 2021 \| 2021A&A...646A..66P \| http://ui.adsabs.harvard.edu/#abs/2021A&A...646A..66P 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 A deep XMM-Newton observation of the X-Persei-like binary system CXOU J225355.1+624336 \|La Palombara, N., Sidoli, L., et al. \| A&A \| 649-118 \| 2021 \| 2021A&A...649A.118L \| http://ui.adsabs.harvard.edu/#abs/2021A&A...649A.118L Tracing the Milky Way.s Vestigial Nuclear Jet \|Cecil, Gerald, Wagner, Alexander Y., et al. \| ApJ \| 922-254 \| 2021 \| 2021ApJ...922..254C \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...922..254C The episodic and multiscale Galactic Centre \|Bryant, Aaron, Krabbe, Alfred, \| NewAR \| 93-101630 \| 2021 \| 2021NewAR..9301630B \| http://ui.adsabs.harvard.edu/#abs/2021NewAR..9301630B X-ray astronomy comes of age \|Wilkes, Belinda J., Tucker, Wallace, et al. \| Natur \| 606-261 \| 2022 \| 2022Natur.606..261W \| http://ui.adsabs.harvard.edu/#abs/2022Natur.606..261W Scientific objectives of the Hot Universe Baryon Surveyor (HUBS) mission \|Bregman, Joel, Cen, Renyue, et al. \| SCPMA \| 66-299513 \| 2023 \| 2023SCPMA..6699513B \| http://ui.adsabs.harvard.edu/#abs/2023SCPMA..6699513B The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way \|Sarkar, Kartick C., \| A&ARv \| 32-1 \| 2024 \| 2024A&ARv..32....1S \| http://ui.adsabs.harvard.edu/#abs/2024A&ARv..32....1S 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 Periodicity from X-ray sources within the inner Galactic disk \|Mondal, Samaresh, Ponti, Gabriele, et al. \| A&A \| 686-A125 \| 2024 \| 2024A&A...686A.125M \| http://ui.adsabs.harvard.edu/#abs/2024A&A...686A.125M 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	2014-02-28T07:33:51Z/2014-08-31T14:45:51Z
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	2015-09-19T22:00:00Z
Keywords	"XMM", "remained unexplored", "xray pulsators", "coherent periodicities", "soft xray", "accreting neutron star", "XMM-Newton", "000 light curves", "xmm newton", "systematic search"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof GianLuca Israel, 2015, 'Unveiling the nature of newly discovered X-ray pulsators', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5j94yy7