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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Recovering the Physical Properties of Molecular Gas in Galaxies from CO SLED Modeling · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1803.07084/</link><description>Collected HN comments and submissions linking this paper.</description><language>en</language><lastBuildDate>Mon, 02 Nov 2026 11:16:22 GMT</lastBuildDate><atom:link href="https://hackerpaper.kaipfister.de/p/1803.07084/feed.xml" rel="self" type="application/rss+xml" /><item><title>Recovering the Physical Properties of Molecular Gas in Galaxies from CO SLED Modeling — mentioned by privong</title><link>https://news.ycombinator.com/item?id=16660816</link><guid isPermaLink="false">urn:hackerpapers:mention:1803.07084:16660816</guid><pubDate>Fri, 23 Mar 2018 17:57:58 GMT</pubDate><description>&lt;p&gt;I am working on testing (&amp;quot;ground truthing&amp;quot;) common observational astronomy modeling techniques against hydrodynamic simulations. The basic approach is to generate synthetic/mock observations from the simulations, apply typical model-fitting approaches, and then see how the model results compare with the properties of the original simulations. Our first paper on this has recently been accepted (https://arxiv.org/abs/1803.07084) and we&amp;#x27;re preparing a second paper looking at emission from dust in new simulations which more realistically treat the cosmological history of galaxies.&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1803.07084/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.GA</category></item></channel></rss>
