A dataset provided by the European Space Agency

Name: Prompt study of magnetar outbursts with XMM-Newton
Published: 2015-04-29T22:00:00Z

Proposal ID	069044
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=0690441801
DOI	https://doi.org/10.5270/esa-rn6ms6v
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 (total requested time of 75ks) aimed at gathering new physicalinsight on these sources, through the study of the very initial phases (within10 days) of the outburstsof known or newly discovered magnetars.
Publications	On the Fe K absorption - accretion state connection in the Galactic Centre neutron star X-ray binary AX J1745.6-2901 \|Ponti, G., Bianchi, S., et al. \| MNRAS \| 446-1536 \| 2015 \| 2015MNRAS.446.1536P \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.446.1536P The X-ray outburst of the Galactic Centre magnetar SGR J1745-2900 during the first 1.5 year \|Coti Zelati, F., Rea, N., et al. \| MNRAS \| 449-2685 \| 2015 \| 2015MNRAS.449.2685C \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.449.2685C Multiwavelength study of the flaring activity of Sagittarius A in 2014 February-April \|Mossoux, E., Grosso, N., et al. \| A&A \| 589-116 \| 2016 \| 2016A&A...589A.116M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...589A.116M High ionisation absorption in low mass X-ray binaries \|Ponti, G., Bianchi, S., et al. \| AN \| 337-512 \| 2016 \| 2016AN....337..512P \| http://ui.adsabs.harvard.edu/#abs/2016AN....337..512P 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 The puzzling orbital period evolution of the LMXB AX J1745.6-2901 \|Ponti, G., De, K., et al. \| MNRAS \| 464-840 \| 2017 \| 2017MNRAS.464..840P \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.464..840P Not that long time ago in the nearest galaxy: 3D slice of molecular gas revealed by a 110 yr old flare of Sgr A* \|Churazov, E., Khabibullin, I., et al. \| MNRAS \| 465-45 \| 2017 \| 2017MNRAS.465...45C \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.465...45C Polarization and long-term variability of Sgr A* X-ray echo \|Churazov, E., Khabibullin, I., et al. \| MNRAS \| 468-165 \| 2017 \| 2017MNRAS.468..165C \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.468..165C Sixteen years of X-ray monitoring of Sagittarius A: Evidence for a decay of the faint flaring rate from 2013 August, 13 months before a rise in the bright flaring rate \|Mossoux, Enmanuelle, Grosso, Nicolas, \| A&A \| 604-85 \| 2017 \| 2017A&A...604A..85M \| http://ui.adsabs.harvard.edu/#abs/2017A&A...604A..85M Chandra monitoring of the Galactic Centre magnetar SGR J1745-2900 during the initial 3.5 years of outburst decay \|Coti Zelati, F., Rea, N., et al. \| MNRAS \| 471-1819 \| 2017 \| 2017MNRAS.471.1819C \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.1819C Can Sgr A flares reveal the molecular gas density PDF? \|Churazov, E., Khabibullin, I., et al. \| MNRAS \| 471-3293 \| 2017 \| 2017MNRAS.471.3293C \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.3293C A transient, flat spectrum radio pulsar near the Galactic Centre \|Dexter, J., Degenaar, N., et al. \| MNRAS \| 468-1486 \| 2017 \| 2017MNRAS.468.1486D \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.468.1486D 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 Rapidly Varying Red Supergiant X-Ray Binary in the Galactic Center \|Gottlieb, Amy M., Eikenberry, Stephen S., et al. \| ApJ \| 896-32 \| 2020 \| 2020ApJ...896...32G \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...32G 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 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 SRG/eROSITA view of X-ray reflection in the Central Molecular Zone: a snapshot in September-October 2019 \|Khabibullin, Ildar, Churazov, Eugene, \| MNRAS \| 509-6068 \| 2022 \| 2022MNRAS.509.6068K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.6068K 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 X-ray polarization evidence for a 200-year-old flare of Sgr ASUP_OPEN*SUP_CLOSE \|Marin, Fr\\u00e9d\\u00e9ric, Churazov, Eugene, et al. \| Natur \| 619-41 \| 2023 \| 2023Natur.619...41M \| http://ui.adsabs.harvard.edu/#abs/2023Natur.619...41M 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 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	2014-04-03T05:06:00Z/2014-04-04T05:07:40Z
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	2015-04-29T22:00:00Z
Keywords	"pulse shape", "XMM", "initial phases", "signicant variability", "physical insight", "75 aimed", "spectral shape", "XMM-Newton", "pulsed fraction", "magnetar outburst", "huge magnetic fields", "xmm newton", "largest amount"
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-rn6ms6v