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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The Young Suns Exoplanet Survey: Detection of a wide orbit planetary mass companion to a solar-type Sco-Cen member · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1912.04284/</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/1912.04284/feed.xml" rel="self" type="application/rss+xml" /><item><title>The Young Suns Exoplanet Survey: Detection of a wide orbit planetary mass companion to a solar-type Sco-Cen member — mentioned by mturmon</title><link>https://news.ycombinator.com/item?id=23920701</link><guid isPermaLink="false">urn:hackerpapers:mention:1912.04284:23920701</guid><pubDate>Wed, 22 Jul 2020 19:35:10 GMT</pubDate><description>&lt;p&gt;Just to emphasize one point you made: It appears the first companion planet (160 AU) was originally detected using direct imaging last year (preprint [1] is dated Dec 2019, see sec. 4 for methods). And I guess the second one was announced in OP, making it a multi-planet system. The point of this comment is to note that these 2 planets were originally detected by direct imaging, not by other techniques. [1] https://arxiv.org/pdf/1912.04284.pdf&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1912.04284/"&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>
