A dataset provided by the European Space Agency

Name: Properties of X-ray activity cycles on young solar-like stars: epsilon Eridanae
Published: 2019-02-07T23:00:00Z

Proposal ID	080116
Title	Properties of X-ray activity cycles on young solar-like stars: epsilon Eridanae
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0801160301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0801160401
DOI	https://doi.org/10.5270/esa-z9g12g5
Principal Investigator, PI	Dr Beate Stelzer
Abstract	We propose to continue our XMM-Newton monitoring of the young, solar analogepsEri with the aim to understand dynamo cycles in the early life of the Sun.XMM-Newton has recently detected an X-ray cycle in another young solar analog,iota Hor, displaying cycle characteristics suggesting violent activity of theSun at an age of virgul600 Myr. Such behavior may affect the evolution of planetatmospheres. To verify if the pecularities of the cycle on iotaHor are typicalfor the dynamos on such young stars we intend to search for the X-ray cycle ofepsEri, the second youngest star with known CaII cycle (Pcyc virgul 3.0yrs). We askhere for two snapshots (2 x 5 ksec), which we will combine with the previouslyexecuted or scheduled observations from our AO14 and AO15 programs.
Publications	An X-ray activity cycle on the young solar-like star \\u220a Eridani \|Coffaro, M., Stelzer, B., et al. \| A&A \| 636-49 \| 2020 \| 2020A&A...636A..49C \| http://ui.adsabs.harvard.edu/#abs/2020A&A...636A..49C 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 Characterizing X-ray activity cycles of young solar-like stars with solar observations \|Coffaro, Martina, Stelzer, Beate, \| AN \| 343-10066 \| 2022 \| 2022AN....34310066C \| http://ui.adsabs.harvard.edu/#abs/2022AN....34310066C In the Trenches of the Solar-Stellar Connection. VI. Total EclipSS \|Ayres, Thomas, Buzasi, Derek, \| ApJS \| 263-41 \| 2022 \| 2022ApJS..263...41A \| http://ui.adsabs.harvard.edu/#abs/2022ApJS..263...41A A multi-wavelength view of the multiple activity cycles of \\u03f5 Eridani \|Fuhrmeister, B., Coffaro, M., et al. \| A&A \| 672-149 \| 2023 \| 2023A&A...672A.149F \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A.149F
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2017-08-26T15:09:47Z/2018-01-16T21:19:55Z
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	2019-02-07T23:00:00Z
Keywords	"solar analog", "planet atmospheres", "solar analog epseri", "XMM", "xray activity cycles", "violent activity", "epsilon eridanae", "dynamo cycles", "XMM-Newton", "displaying cycle characteristics", "iota hor", "ao15 programs", "xray cycle", "caii cycle pcyc", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Beate Stelzer, 2019, 'Properties of X-ray activity cycles on young solar-like stars: epsilon Eridanae', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-z9g12g5