From solar to stellar flare characteristics. On a new peak size distribution for G-, K-, and M-dwarf star flares

<p>This dataset contains additional material for the research paper &quot;From solar to stellar flare characteristics. On a new peak size distribution for G-, K-, and M-dwarf star flares&quot;, Astron. Astrophys., 2018.</p> <p>Based on the flare list available at http://156.17.94.1/sphinx_l1_catalogue/SphinX_cat_main.html, here peak X-ray flare intensities of&nbsp; Q- to C-class flares measured by the SphinX instrument (see, e.g., Kotov, 2011; Sylvester et al., 2011, 2012; Gburek et al., 2011a,b, 2013; Gryciuk et al., 2017) during the solar minimum of <strong>2009</strong> and their corresponding GOES E &gt; 10 MeV peak proton fluxes are given.</p> <p><br> Column 1: Month<br> Column 2: Day<br> Column 3: X-ray flux peak hour<br> Column 4: X-ray flux peak minute<br> Column 5: X-ray flare peak intensity (W/m²)<br> Column 5: GOES E &gt; 10 MeV peak proton flux (pfu)<br> Column 6: Flare location (according to the SphinX-database)</p>