A dataset provided by the European Space Agency

Name: RX J1605.3+3249: as close to a magnetar as a Magnificent Seven INS can get
Published: 2017-03-07T23:00:00Z

Proposal ID	076446
Title	RX J1605.3+3249: as close to a magnetar as a Magnificent Seven INS can get
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0764460201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0764460301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0764460401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0764460501
DOI	https://doi.org/10.5270/esa-pbt2i39
Principal Investigator, PI	Dr Adriana Mancini Pires
Abstract	RX J1605.3+3249 is one of the intriguing isolated neutron stars (INSs) known asthe Magnificent Seven (M7). An evolutionary link with magnetars may explainwhy they rotate more slowly, are hotter, and have higher magnetic fields thanother pulsars of similar age. A recent XMM-Newton observation finally revealedthe neutron star spin period. The amplitude of the modulation is stronglyenergy-dependent. Further observations will be used to determine a precisetiming solution and to perform phase-resolved spectroscopy. These will provideinvaluable information on the geometry of the emitting regions, and will allowus to precisely determine the high value of spin down hinted by analysis ofarchival data, which places the source closer to a magnetar than any other M7 INS.
Publications	A deep XMM-Newton look on the thermally emitting isolated neutron star RX J1605.3+3249 \|Pires A. M. Schwope A. D. et al. \| A&A \| 623-73 \| 2019 \| 2019A&A...623A..73P \| http://ui.adsabs.harvard.edu/#abs/2019A&A...623A..73P Universal detection of high-temperature emission in X-ray isolated neutron stars \|Yoneyama Tomokage Hayashida Kiyoshi et al. \| PASJ \| 71-17 \| 2019 \| 2019PASJ...71...17Y \| http://ui.adsabs.harvard.edu/#abs/2019PASJ...71...17Y A Joint NICER and XMM-Newton View of the Magnificent Thermally Emitting X-Ray Isolated Neutron Star RX J1605.3+3249 \|Malacaria Christian Bogdanov Slavko et al. \| ApJ \| 880-74 \| 2019 \| 2019ApJ...880...74M \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...880...74M A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha Vineet Chand Hum et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O Hard X-Ray Excess from the Magnificent Seven Neutron Stars \|Dessert Christopher Foster Joshua W. \| ApJ \| 904-42 \| 2020 \| 2020ApJ...904...42D \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904...42D Axion Emission Can Explain a New Hard X-Ray Excess from Nearby Isolated Neutron Stars \|Buschmann Malte Co Raymond T. et al. \| PhRvL \| 126-21102 \| 2021 \| 2021PhRvL.126b1102B \| http://ui.adsabs.harvard.edu/#abs/2021PhRvL.126b1102B 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 Deep eROSITA observations of the magnificent seven isolated neutron stars \|Mancini Pires Adriana Schwope Axel \| IAUS \| 363-288 \| 2023 \| 2023IAUS..363..288M \| http://ui.adsabs.harvard.edu/#abs/2023IAUS..363..288M 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 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	2015-07-21T20:19:26Z/2016-02-11T16:05:16Z
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	2017-03-07T23:00:00Z
Last Update	2025-01-27
Keywords	"magnetic fields", "rx j1605", "M7", "emitting region", "magnificent ins", "xmm newton", "XMM-Newton", "source closer", "evolutionary link", "invaluable information", "J1605.3", "XMM", "m7 ins", "energy dependent", "archival data"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Adriana Mancini Pires, 2017, 'RX J1605.3+3249: as close to a magnetar as a Magnificent Seven INS can get', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-pbt2i39