A dataset provided by the European Space Agency

Name: XMM-Newton Observation of the eclipsing pulsar X1822-371
Published: 2018-03-28T22:00:00Z

Proposal ID	078482
Title	XMM-Newton Observation of the eclipsing pulsar X1822-371
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784820101
DOI	https://doi.org/10.5270/esa-fzlvqy7
Principal Investigator, PI	Ms Ann-Sofie Bak Nielsen
Abstract	We propose to perform an XMM-Newton observation of the LMXB X1822-371 within thecycle AO-15. The aim of the observation is to investigate why the orbital periodseems to have an evolution over a time scale that is much shorter that what isexpected from LMXBs. With this observation we will also precisely determine thespin and orbital evolution over the last 20 years.
Publications	Updated orbital ephemeris of the ADC source X 1822-371: a stable orbital expansion over 40 years \|Mazzola S. M. Iaria R. et al. \| A&A \| 625-12 \| 2019 \| 2019A&A...625L..12M \| http://ui.adsabs.harvard.edu/#abs/2019A&A...625L..12M 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 Spectral analysis of the low-mass X-ray pulsar 4U 1822-371: Reflection component in a high-inclination system \|Anitra A. Di Salvo T. et al. \| A&A \| 654-160 \| 2021 \| 2021A&A...654A.160A \| http://ui.adsabs.harvard.edu/#abs/2021A&A...654A.160A Confirmation of the presence of a CRSF in the NICER spectrum of X 1822-371 \|Iaria R. Di Salvo T. et al. \| A&A \| 683-A79 \| 2024 \| 2024A&A...683A..79I \| http://ui.adsabs.harvard.edu/#abs/2024A&A...683A..79I 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	2017-03-06T00:18:34Z/2017-03-06T19:26:54Z
Version	19.17_20220121_1250
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	2018-03-28T22:00:00Z
Last Update	2025-01-27
Keywords	"X1822-371", "cycle ao", "xmm newton", "orbital period", "XMM-Newton", "lmxb x1822 371", "time scale", "XMM", "orbital evolution"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Ms Ann-Sofie Bak Nielsen, 2018, 'XMM-Newton Observation of the eclipsing pulsar X1822-371', 19.17_20220121_1250, European Space Agency, https://doi.org/10.5270/esa-fzlvqy7