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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Statistical methods for exoplanet detection with radial velocities · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2308.00701/</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/2308.00701/feed.xml" rel="self" type="application/rss+xml" /><item><title>Statistical methods for exoplanet detection with radial velocities — mentioned by JumpCrisscross</title><link>https://news.ycombinator.com/item?id=44820095</link><guid isPermaLink="false">urn:hackerpapers:mention:2308.00701:44820095</guid><pubDate>Thu, 07 Aug 2025 02:54:43 GMT</pubDate><description>&lt;p&gt;&amp;gt; not sure about RV limits Radial velocity, how quickly a planet moves “back and forth towards an observer” as it revolved about its star [1]. Its amplitude suggests planetary mass, its spectral shape orbital eccentricity. [1] https://arxiv.org/pdf/2308.00701&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2308.00701/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.IM</category></item></channel></rss>
