A dataset provided by the European Space Agency

Name: Prompt study of AXP outbursts with XMM
Published: 2009-11-05T00:00:00Z

Proposal ID	055297
Title	Prompt study of AXP outbursts with XMM
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552971101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552971201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552971301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552971401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0552971501
DOI	https://doi.org/10.5270/esa-20tpcrq
Principal Investigator, PI	Dr GianLuca Israel
Abstract	The discovery of transient AXPs has has opened a new perspective in the fieldconfirming that a relatively large number of members of this class has not beendiscovered yet, and suggesting that others would manifest themself in the futurethrough outbursts. This proposal is aimed at gathering new insights on thephysics of AXPs through the study of the very initial phases (within 10-15days)of their outbursts.
Publications	The first outburst of the new magnetar candidate SGR0501+4516 \|Rea, N., Israel, G. L., et al. \| MNRAS \| 396-2419 \| 2009 \| 2009MNRAS.396.2419R \| http://ui.adsabs.harvard.edu/#abs/2009MNRAS.396.2419R Quiescent state and outburst evolution of SGR 0501+4516 \|Camero, A., Papitto, A., et al. \| MNRAS \| 438-3291 \| 2014 \| 2014MNRAS.438.3291C \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.438.3291C 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 The Short Bursts in SGR-1806 20, 1E 1048-5937, and SGR 0501+4516 \|Qu, Zhijie, Li, Zhaosheng, et al. \| PASP \| 127-211 \| 2015 \| 2015PASP..127..211Q \| http://ui.adsabs.harvard.edu/#abs/2015PASP..127..211Q X-Ray Perspective of the Twisted Magnetospheres of Magnetars \|Weng, Shan-Shan, Gogus, Ersin, et al. \| ApJ \| 805-81 \| 2015 \| 2015ApJ...805...81W \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...805...81W 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 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 X-Ray Observations of Magnetar SGR 0501+4516 from Outburst to Quiescence \|Mong, Y.-L., Ng, C.-Y., \| ApJ \| 852-86 \| 2018 \| 2018ApJ...852...86M \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...852...86M Magnetar outbursts: an observational review \|Rea, Nanda, Esposito, Paolo, \| ASSP \| 21-247 \| 2011 \| 2011ASSP...21..247R \| http://ui.adsabs.harvard.edu/#abs/2011ASSP...21..247R 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 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	2008-08-29T07:06:02Z/2008-09-30T13:44:00Z
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	2009-11-05T00:00:00Z
Keywords	"XMM", "transient axps", "initial phases", "axp outburst", "manifest themself"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr GianLuca Israel, 2009, 'Prompt study of AXP outbursts with XMM', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-20tpcrq