Poster Open Access
Jackman, James; Shkolnik, Evgenya; Million, Chase; Fleming, Scott
<?xml version='1.0' encoding='UTF-8'?> <record xmlns="http://www.loc.gov/MARC21/slim"> <leader>00000nam##2200000uu#4500</leader> <datafield tag="999" ind1="C" ind2="5"> <subfield code="x">Venot, O., Rocchetto, M., Carl, S., et al. 2016, ApJ, 830, 77. doi:10.3847/0004-637X/830/2/77</subfield> </datafield> <datafield tag="999" ind1="C" ind2="5"> <subfield code="x">Rimmer, P. B., Xu, J., Thompson, S. J., et al. 2018, Science Advances, 4, eaar3302. doi:10.1126/sciadv.aar3302</subfield> </datafield> <datafield tag="999" ind1="C" ind2="5"> <subfield code="x">Gunther, M.~N., Zhan, Z., Seager, S., et al. 2020, AJ, 159, 60. doi:10.3847/1538-3881/ab5d3a</subfield> </datafield> <datafield tag="999" ind1="C" ind2="5"> <subfield code="x">Million, C., Fleming, S.~W., Shiao, B., et al. 2016, ApJ, 833, 292. doi:10.3847/1538-4357/833/2/292</subfield> </datafield> <datafield tag="653" ind1=" " ind2=" "> <subfield code="a">Cool Stars on the main sequence</subfield> </datafield> <datafield tag="653" ind1=" " ind2=" "> <subfield code="a">Very low mass stars</subfield> </datafield> <controlfield tag="005">20210226134301.0</controlfield> <controlfield tag="001">4564321</controlfield> <datafield tag="711" ind1=" " ind2=" "> <subfield code="d">March 2-4, 2021</subfield> <subfield code="g">CS20.5</subfield> <subfield code="a">The 20.5th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun</subfield> <subfield code="c">Virtually anywhere</subfield> </datafield> <datafield tag="700" ind1=" " ind2=" "> <subfield code="u">Arizona State University</subfield> <subfield code="a">Shkolnik, Evgenya</subfield> </datafield> <datafield tag="700" ind1=" " ind2=" "> <subfield code="u">Million Concepts LLC</subfield> <subfield code="a">Million, Chase</subfield> </datafield> <datafield tag="700" ind1=" " ind2=" "> <subfield code="u">Space Telescope Science Institute</subfield> <subfield code="a">Fleming, Scott</subfield> </datafield> <datafield tag="700" ind1=" " ind2=" "> <subfield code="4">edt</subfield> <subfield code="a">Wolk, Scott</subfield> </datafield> <datafield tag="856" ind1="4" ind2=" "> <subfield code="s">949364</subfield> <subfield code="z">md5:892b9aaa23fa5237585392166d379d61</subfield> <subfield code="u">https://zenodo.org/record/4564321/files/Cool Stars 20.5 A4.pdf</subfield> </datafield> <datafield tag="856" ind1="4" ind2=" "> <subfield code="s">1035111</subfield> <subfield code="z">md5:b24c3b327c298bfca7fa0fd2a82cfe21</subfield> <subfield code="u">https://zenodo.org/record/4564321/files/Cool Stars 20.5 A4.png</subfield> </datafield> <datafield tag="542" ind1=" " ind2=" "> <subfield code="l">open</subfield> </datafield> <datafield tag="856" ind1="4" ind2=" "> <subfield code="y">Conference website</subfield> <subfield code="u">http://coolstars20.cfa.harvard.edu/cs20half</subfield> </datafield> <datafield tag="260" ind1=" " ind2=" "> <subfield code="c">2021-02-26</subfield> </datafield> <datafield tag="909" ind1="C" ind2="O"> <subfield code="p">openaire</subfield> <subfield code="p">user-coolstars20half</subfield> <subfield code="o">oai:zenodo.org:4564321</subfield> </datafield> <datafield tag="100" ind1=" " ind2=" "> <subfield code="u">Arizona State University</subfield> <subfield code="a">Jackman, James</subfield> </datafield> <datafield tag="245" ind1=" " ind2=" "> <subfield code="a">The Disconnect Between UV and White-Light Flares in Low-Mass Stars</subfield> </datafield> <datafield tag="980" ind1=" " ind2=" "> <subfield code="a">user-coolstars20half</subfield> </datafield> <datafield tag="540" ind1=" " ind2=" "> <subfield code="u">https://creativecommons.org/licenses/by/4.0/legalcode</subfield> <subfield code="a">Creative Commons Attribution 4.0 International</subfield> </datafield> <datafield tag="650" ind1="1" ind2="7"> <subfield code="a">cc-by</subfield> <subfield code="2">opendefinition.org</subfield> </datafield> <datafield tag="520" ind1=" " ind2=" "> <subfield code="a"><p>Contemporary studies of exoplanet habitability often use white-light measurements to estimate&nbsp;the ultraviolet (UV) effects of stellar flares, often by assuming a 9000K blackbody for the bolometric flare spectrum.&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.&nbsp;We have&nbsp;found from our preliminary results that the UV predictions of white-light flare rates do not accurately reflect the NUV or FUV&nbsp;flaring activity of low-mass stars and&nbsp;are working to quantify the scale of this disconnect.</p></subfield> </datafield> <datafield tag="773" ind1=" " ind2=" "> <subfield code="n">doi</subfield> <subfield code="i">isVersionOf</subfield> <subfield code="a">10.5281/zenodo.4564320</subfield> </datafield> <datafield tag="024" ind1=" " ind2=" "> <subfield code="a">10.5281/zenodo.4564321</subfield> <subfield code="2">doi</subfield> </datafield> <datafield tag="980" ind1=" " ind2=" "> <subfield code="a">poster</subfield> </datafield> </record>
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