A dataset provided by the European Space Agency

Name: Challenging the rotation-activity paradigm II
Published: 2016-12-14T23:00:00Z

Proposal ID	076349
Title	Challenging the rotation-activity paradigm II
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763490301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763490501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763490701
DOI	https://doi.org/10.5270/esa-f5vodyl
Principal Investigator, PI	Dr Stefan Czesla
Abstract	We propose to obtain XMM-Newton snapshots of seven of the most slowly rotatingG-type superflare stars identified by the Kepler satellite to test whether theyadhere to the rotation-activity paradigm. While the strongest flares observed onthe Sun release about 1e32 erg, Kepler observed G-type dwarfs that producewhite-light flares releasing up to four orders of magnitude more energy.Curiously, many of these superflare stars are apparently slow rotators.Notwithstanding, our recent XMM-Newton campaign showed that these stars can beextremely bright X-ray sources (about 1e30 erg/s). Consequently, we identifiedthe slowest rotators among the superflare stars amenable to X-ray observationsto study their X-ray emission.
Publications	Dark matter distribution in X-ray luminous galaxy clusters with Emergent Gravity \|Ettori S. Ghirardini V. et al. \| MNRAS \| 470-29 \| 2017 \| 2017MNRAS.470L..29E \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470L..29E The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the intracluster medium out to R200 in Abell 2319 \|Ghirardini V. Ettori S. et al. \| A&A \| 614-7 \| 2018 \| 2018A&A...614A...7G \| http://ui.adsabs.harvard.edu/#abs/2018A&A...614A...7G Thermodynamic profiles of galaxy clusters from a joint X-ray/SZ analysis \|Shitanishi Jennifer A. Pierpaoli Elena et al. \| MNRAS \| 481-749 \| 2018 \| 2018MNRAS.481..749S \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.481..749S Iron in X-COP: Tracing enrichment in cluster outskirts with high accuracy abundance profiles \|Ghizzardi Simona Molendi Silvano et al. \| A&A \| 646-92 \| 2021 \| 2021A&A...646A..92G \| http://ui.adsabs.harvard.edu/#abs/2021A&A...646A..92G 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 The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation. I. Programme overview \|CHEX-MATE Collaboration Arnaud M. et al. \| A&A \| 650-104 \| 2021 \| 2021A&A...650A.104C \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.104C CHEX-MATE: Morphological analysis of the sample \|Campitiello M. G. Ettori S. et al. \| A&A \| 665-117 \| 2022 \| 2022A&A...665A.117C \| http://ui.adsabs.harvard.edu/#abs/2022A&A...665A.117C CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles \|Bartalucci I. Molendi S. et al. \| A&A \| 674-179 \| 2023 \| 2023A&A...674A.179B \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A.179B CHEX-MATE: X-ray absorption and molecular content of the interstellar medium toward galaxy clusters \|Bourdin H. De Luca F. et al. \| A&A \| 678-181 \| 2023 \| 2023A&A...678A.181B \| http://ui.adsabs.harvard.edu/#abs/2023A&A...678A.181B Pressure profiles of distant Galaxy clusters with Planck-SPT data \|Oppizzi Filippo De Luca Federico et al. \| EPJWC \| 257-00035 \| 2022 \| 2022EPJWC.25700035O \| http://ui.adsabs.harvard.edu/#abs/2022EPJWC.25700035O 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 CHEX-MATE: Turbulence in the intra-cluster medium from X-ray surface brightness fluctuations \|Dupourquu00e9 S. Clerc N. et al. \| A&A \| 687-A58 \| 2024 \| 2024A&A...687A..58D \| http://ui.adsabs.harvard.edu/#abs/2024A&A...687A..58D New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2015-09-13T00:12:51Z/2015-11-23T13:48:07Z
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	2016-12-14T23:00:00Z
Last Update	2025-08-04
Keywords	"slowly rotating", "kepler satellite", "xmm newton campaign", "slowest rotators", "1e30 erg", "xray emission", "type superflare stars", "XMM", "sun release", "apparently slow rotators", "type dwarfs", "rotation activity paradigm", "xmm newton snapshots", "superflare stars amenable", "bright xray sources", "XMM-Newton", "1e32 erg", "superflare stars", "strongest flare"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Stefan Czesla, 2016, 'Challenging the rotation-activity paradigm II', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-f5vodyl