http://www.colloquiam.com/wd/index.php?action=history&feed=atom&title=Klapp_et_al_2021a 2026-06-10T14:01:29Z Revision history for this page on the wiki MediaWiki 1.27.0-wmf.10 http://www.colloquiam.com/wd/index.php?title=Klapp_et_al_2021a&diff=218944&oldid=prev 2021-03-11T15:55:04Z

<p>Scipediacontent moved page <a href="/public/Draft_Content_175221066" class="mw-redirect" title="Draft Content 175221066">Draft Content 175221066</a> to <a href="/public/Klapp_et_al_2021a" title="Klapp et al 2021a">Klapp et al 2021a</a></p> <table class="diff diff-contentalign-left" data-mw="interface"> <tr style='vertical-align: top;' lang='en'> <td colspan='1' style="background-color: white; color:black; text-align: center;">← Older revision</td> <td colspan='1' style="background-color: white; color:black; text-align: center;">Revision as of 15:55, 11 March 2021</td> </tr><tr><td colspan='2' style='text-align: center;' lang='en'><div class="mw-diff-empty">(No difference)</div> </td></tr></table>

Scipediacontent http://www.colloquiam.com/wd/index.php?title=Klapp_et_al_2021a&diff=218943&oldid=prev 2021-03-11T15:55:01Z

<p>Created page with &quot;== Abstract == We have developed an artificial neural network, whose purpose is to automatically find in a database of synthetic stellar spectra the one which best reproduces...&quot;</p> <p><b>New page</b></p><div>== Abstract ==<br /> <br /> We have developed an artificial neural network, whose purpose is to automatically find in a database of synthetic stellar spectra the one which best reproduces an observed spectrum. Using the equivalent widths of selected spectral lines, the network fits a set of lines related to the physical parameters in the stellar atmosphere (i.e., temperature, gravity and mass loss rate). The main advantage of this approach is its scalability.<br /> <br /> == Full document ==<br /> &lt;pdf&gt;Media:Draft_Content_175221066p1205.pdf&lt;/pdf&gt;</div>

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