A dataset provided by the European Space Agency

Name: Prompt study of magnetar outbursts with XMM-Newton
Published: 2015-11-14T23:00:00Z

Proposal ID	072241
Title	Prompt study of magnetar outbursts with XMM-Newton
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722412501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722412601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722412701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722412801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722412901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0722413001
DOI	https://doi.org/10.5270/esa-lnahuuk
Principal Investigator, PI	Dr GianLuca Israel
Abstract	AXPs and SGRs are believed to be magnetars, ultra-magnetised neutron starspowered by huge magnetic fields. They are characterized by bursts, glitches,signicant variability in flux, spectral shape, pulse shape, pulsed fraction.They go through long stretches of quiescence, interrupted by periods ofactivity. Observations performed during, or immediately after such periods yieldthe largest amount of information on magnetars emission, allowing to test thetheoretical models on a variety of phenomena and source states. We propose arapid ToO program aimed at gathering new physical insight on these sources,through the study of the very initial phases (within 10 days) of the outburstsof known or newly discovered magnetars.
Publications	The discovery monitoring and environment of SGR J1935+2154 \|Israel G. L. Esposito P. et al. \| MNRAS \| 457-3448 \| 2016 \| 2016MNRAS.457.3448I \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.457.3448I Radio Pulsation Search and Imaging Study of SGR J1935+2154 \|Surnis Mayuresh. P. Joshi Bhal Chandra et al. \| ApJ \| 826-184 \| 2016 \| 2016ApJ...826..184S \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...826..184S 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 X-Ray and Radio Observations of the Magnetar SGR J1935+2154 during Its 2014 2015 and 2016 Outbursts \|Younes George Kouveliotou Chryssa et al. \| ApJ \| 847-85 \| 2017 \| 2017ApJ...847...85Y \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...847...85Y 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 Revisiting the Distance Environment and Supernova Properties of SNR G57.2+0.8 that Hosts SGR 1935+2154 \|Zhou Ping Zhou Xin et al. \| ApJ \| 905-99 \| 2020 \| 2020ApJ...905...99Z \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...905...99Z 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 Spin Evolution of the Magnetar SGR J1935+2154 \|Ge Ming-Yu Yang Yuan-Pei et al. \| RAA \| 24-015016 \| 2024 \| 2024RAA....24a5016G \| http://ui.adsabs.harvard.edu/#abs/2024RAA....24a5016G 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	2014-09-26T22:10:22Z/2014-10-28T02:43:03Z
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	2015-11-14T23:00:00Z
Last Update	2025-01-27
Keywords	"huge magnetic fields", "physical insight", "pulse shape", "xmm newton", "spectral shape", "XMM-Newton", "largest amount", "initial phases", "XMM", "pulsed fraction", "program aimed", "signicant variability"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr GianLuca Israel, 2015, 'Prompt study of magnetar outbursts with XMM-Newton', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-lnahuuk