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         title="Permalink to The optically bright post-AGB population of the LMC">The optically bright post-AGB population of the LMC</a></h2>
 
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    <abbr class="published" title="2012-09-20T18:43:00-06:00">
      2012/09/20
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    <address class="vcard author">
      By <a class="url fn" href="https://keflavich.github.io/blog/author/adam-keflavichgmailcom.html">Adam (keflavich@gmail.com)</a>
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  <div class="entry-content">
    <p>[<a class="reference external" href="http://adsabs.harvard.edu/abs/2011A%26A...530A..90V">ADS</a> ] [<a class="reference external" href="http://arxiv.org/abs/1104.2254">arXiv</a> ]</p>
<p>E. van Aarle, H. Van Winckel, T. Lloyd Evans, T. Ueta, P. R. Wood, and
A. G. Ginsburg</p>
<hr class="docutils" />
<p>A catalog of post-AGB stars in the LMC, useful in particular because
they are at a common distance. Post-AGB stars are quite luminous (&gt; 1000
L<sub>O</sub> usually), so easily detected in the LMC.</p>
<p>My contribution to this work was years ago; I worked on the <a class="reference external" href="http://sage.stsci.edu/">SAGE</a>
project for a few months at the University of Denver with <a class="reference external" href="http://mysite.du.edu/~tueta/Welcome.html">Toshiya
Ueta</a>. I generated a catalog of post-AGB objects and an online catalog
with automatic SED plotter. It was a pretty neat project, but I left
before I was able to convince others that my catalog was definitive;
nonetheless it was eventually used in this publication. As an aside,
that was my first foray into data languages, and I ended up using the
<a class="reference external" href="http://pdl.perl.org/">Perl Data Language</a> long before I learned of python and before I got a
free IDL license.</p>

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