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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Direct Imaging and Spectroscopy of a Planetary Mass Candidate Companion to a Young Solar Analog · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/0809.1424/</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/0809.1424/feed.xml" rel="self" type="application/rss+xml" /><item><title>Direct Imaging and Spectroscopy of a Planetary Mass Candidate Companion to a Young Solar Analog — mentioned by contact_fusion</title><link>https://news.ycombinator.com/item?id=14638465</link><guid isPermaLink="false">urn:hackerpapers:mention:0809.1424:14638465</guid><pubDate>Mon, 26 Jun 2017 17:14:16 GMT</pubDate><description>&lt;p&gt;That image is quite stunning. As the 2008 press release [1] states, this image was one of the first successes at direct imaging an exoplanet. It raised some interesting questions, such as why such a massive planet could be found so far out (330 AU!) The scientific paper for this observation can be found in [2] for those interested more astrophysical detail. I feel compelled to offer an astronomer&amp;#x27;s clarification though. The planet in this image is not &amp;quot;resolved&amp;quot; in the technical sense. A resolved image usually means that fine details about the object are discernible spatially. For example…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/0809.1424/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph</category></item></channel></rss>
