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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>HAT-P-11b: A Super-Neptune Planet Transiting a Bright K Star in the Kepler Field · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/0901.0282/</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/0901.0282/feed.xml" rel="self" type="application/rss+xml" /><item><title>HAT-P-11b: A Super-Neptune Planet Transiting a Bright K Star in the Kepler Field — mentioned by bfe</title><link>https://news.ycombinator.com/item?id=8366156</link><guid isPermaLink="false">urn:hackerpapers:mention:0901.0282:8366156</guid><pubDate>Thu, 25 Sep 2014 08:14:10 GMT</pubDate><description>&lt;p&gt;Progress on all fronts is driving the progress in exoplanets. The Kepler space telescope has been a huge driver, and Hubble, Spitzer, and big ground-based telescopes have played a big role; this new discovery is based on Hubble and Spitzer data runs plus comparison with Kepler data. Exoplanet search will take a giant leap with the planned launch of the TESS space telescope in 2017. But this exoplanet was first discovered by a small network of at the time 6 extremely modest telescopes (just 110mm / ~4.3 inch objective diameter) automatically controlled by one Linux box in a project built by…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/0901.0282/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.EP</category></item></channel></rss>
