Poster Open Access

The Disconnect Between UV and White-Light Flares in Low-Mass Stars

Jackman, James; Shkolnik, Evgenya; Million, Chase; Fleming, Scott


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        <foaf:name>Million, Chase</foaf:name>
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    <dct:title>The Disconnect Between UV and White-Light Flares in Low-Mass Stars</dct:title>
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    <dct:issued rdf:datatype="http://www.w3.org/2001/XMLSchema#gYear">2021</dct:issued>
    <dcat:keyword>Cool Stars on the main sequence</dcat:keyword>
    <dcat:keyword>Very low mass stars</dcat:keyword>
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        <foaf:name>Wolk, Scott</foaf:name>
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    <dct:issued rdf:datatype="http://www.w3.org/2001/XMLSchema#date">2021-02-26</dct:issued>
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    <dct:description>&lt;p&gt;Contemporary studies of exoplanet habitability often use white-light measurements to estimate&amp;nbsp;the ultraviolet (UV) effects of stellar flares, often by assuming a 9000K blackbody for the bolometric flare spectrum.&amp;nbsp;We have combined TESS and archival GALEX photometry to test the UV predictions of white-light flare rates using the 9000K model and discuss the background and our methodology in this poster.&amp;nbsp;We have&amp;nbsp;found from our preliminary results that the UV predictions of white-light flare rates do not accurately reflect the NUV or FUV&amp;nbsp;flaring activity of low-mass stars and&amp;nbsp;are working to quantify the scale of this disconnect.&lt;/p&gt;</dct:description>
    <dct:description>{"references": ["Venot, O., Rocchetto, M., Carl, S., et al. 2016, ApJ, 830, 77. doi:10.3847/0004-637X/830/2/77", "Rimmer, P. B., Xu, J., Thompson, S. J., et al. 2018, Science Advances, 4, eaar3302. doi:10.1126/sciadv.aar3302", "Gunther, M.~N., Zhan, Z., Seager, S., et al. 2020, AJ, 159, 60. doi:10.3847/1538-3881/ab5d3a", "Million, C., Fleming, S.~W., Shiao, B., et al. 2016, ApJ, 833, 292. doi:10.3847/1538-4357/833/2/292"]}</dct:description>
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