Published September 13, 2023 | Version 1.0
Dataset Open

The corona of a fully convective star with a near-polar flare

Authors/Creators

  • 1. Leibniz Institute for Astrophysics Potsdam (AIP)
  • 2. ROR icon Netherlands Institute for Radio Astronomy
  • 3. Universität Tübingen
  • 4. ROR icon Leibniz Institute for Astrophysics Potsdam

Description

Raw XMM-Newton EPIC data, data reduction scripts for XMM-SAS, and reduced images and spectra extracted with XSPEC. The observations include the X-ray emission of TIC 277539431, a rapidly rotating M7 dwarf star that produced a polar flare in 2021, observed by the Transiting Exoplanet Survey Satellite (see Ilin et al. 2021).

Publications based on this data set will be linked as they appear.

Notes

This dataset was made possible by the Deutsche Luft- und Raumfahrtgesellschaft (FKZ 50 OR 2209, project X-ray Loops). This work is based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA.

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