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Time-resolved spectroscopy and photometry of an M dwarf flare star YZ Canis Minoris with OISTER and TESS: Blue asymmetry in H$\alpha$ line during the non-white light flare

, , , , , , , , , , , , , , , , , and . (2020)cite arxiv:2009.14412Comment: 39 pages, 15 figures, supplementary table (CSV format); accepted for publication in PASJ.

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The Evolution of $T = 10^4$ K Blackbody-Like Continuum Radiation in the Impulsive Phase of dMe Flares, , and . (2018)cite arxiv:1810.07226Comment: 6 pages, 2 Figures. Conference Proceedings to the Cambridge Workshops of Cool Stars, Stellar Systems and the Sun #20 (Cool Stars 20, July 29 - August 3, 2018; Boston, MA).Time-resolved spectroscopy and photometry of an M dwarf flare star YZ Canis Minoris with OISTER and TESS: Blue asymmetry in H$\alpha$ line during the non-white light flare, , , , , , , , , and 8 other author(s). (2020)cite arxiv:2009.14412Comment: 39 pages, 15 figures, supplementary table (CSV format); accepted for publication in PASJ.A Unified Computational Model for Solar and Stellar Flares, , and . (Jul 15, 2015)