A dataset provided by the European Space Agency

Name: Do normal coronae produce superflaresquestionMark
Published: 2017-07-07T22:00:00Z

Proposal ID	078378
Title	Do normal coronae produce superflares?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783780301
DOI	https://doi.org/10.5270/esa-1pta1p5
Principal Investigator, PI	Dr Stefan Czesla
Abstract	We propose to obtain XMM-Newton observations of three spectroscopically singlesuperflare stars with large rotation periods (Prot >10 d) to test whether theircoronae adhere to the rotation--activity paradigm. While the strongest flaresobserved on the Sun release about 1e32 erg, Kepler observed a rare species ofG-type dwarfs that produce white-light flares releasing up to four orders ofmagnitude more energy. Notwithstanding their enormous optical outbursts, weidentified two single superflare stars, whose coronae seem to adhere to theconventional rotation--activity relation. Combining the available information,we identified the best single superflare stars to enlarge the sample of ourX-ray study.
Publications	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 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	2016-06-16T05:23:17Z/2016-06-16T13:28:17Z
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	2017-07-07T22:00:00Z
Keywords	"optical outburst", "rotation activity paradigm", "XMM", "superflares ?.", "coronae adhere", "sun release", "type dwarfs", "1e32 erg", "single superflare stars", "normal coronae", "strongest flare", "XMM-Newton", "rotation periods prot", "rare species", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Stefan Czesla, 2017, 'Do normal coronae produce superflaresquestionMark', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-1pta1p5