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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Radial-velocity discovery of a second planet in the TOI-1338/BEBOP-1 circumbinary system · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2301.10794/</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/2301.10794/feed.xml" rel="self" type="application/rss+xml" /><item><title>Radial-velocity discovery of a second planet in the TOI-1338/BEBOP-1 circumbinary system — mentioned by 7373737373</title><link>https://news.ycombinator.com/item?id=36307751</link><guid isPermaLink="false">urn:hackerpapers:mention:2301.10794:36307751</guid><pubDate>Tue, 13 Jun 2023 09:37:40 GMT</pubDate><description>&lt;p&gt;With the radial velocity method they used, anytime - it&amp;#x27;s a telescope with a spectrometer that only relies on the planets wobbling the stars around a bit to produce a doppler shift. With the transit method (observing the planet passing in front of the host star(s) by seeing a temporary reduction in light: https://en.wikipedia.org/wiki/Methods_of_detecting_exoplanet...), apparently yes, but not often and it is unclear when. The paper (https://arxiv.org/pdf/2301.10794.pdf) states: &amp;gt; A visual inspection of TESS lightcurves shows no transit of TOI-1338/BEBOP-1c, however, thanks to orbital…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2301.10794/"&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>
