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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Re-analysis of the 267-GHz ALMA observations of Venus: No statistically significant detection of phosphine · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2010.09761/</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/2010.09761/feed.xml" rel="self" type="application/rss+xml" /><item><title>Re-analysis of the 267-GHz ALMA observations of Venus: No statistically significant detection of phosphine — mentioned by gus_massa</title><link>https://news.ycombinator.com/item?id=24985680</link><guid isPermaLink="false">urn:hackerpapers:mention:2010.09761:24985680</guid><pubDate>Wed, 04 Nov 2020 00:43:49 GMT</pubDate><description>&lt;p&gt;The idea is that you want to split your data as a sum of three parts: (a) a smooth function that is not interesting (b) noise (c) a big unexpected peak in an interesting part There is a nice preprint posted a few days ago: https://arxiv.org/abs/2010.09761 https://arxiv.org/abs/2010.09761.pdf They reanalyze the data than in the phosphine paper. --- If you look at figure 3, they have the data that is the skyscraper-like line, and they use a polynomial of degree 3 to approximate the signal, that is that curved unhappy smooth line. The smooth line is (a), when you subtract this smooth function…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2010.09761/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.EP</category></item><item><title>Re-analysis of the 267-GHz ALMA observations of Venus: No statistically significant detection of phosphine — mentioned by gus_massa</title><link>https://news.ycombinator.com/item?id=24964055</link><guid isPermaLink="false">urn:hackerpapers:mention:2010.09761:24964055</guid><pubDate>Mon, 02 Nov 2020 01:17:58 GMT</pubDate><description>&lt;p&gt;I was more convinced that the original paper may have problems by https://arxiv.org/abs/2010.09761 From that preprint: &amp;gt; We find that the 12th-order polynomial fit to the spectral passband utilised in the published study leads to spurious results. Using a 12th-order polynomial fit is very suspicious? And I think that it is very interesting to see Figure 2, top-left. The signal is very noisy and the polynomial fit is not convincing. That graph is a very big red flag.&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2010.09761/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.EP</category></item><item><title>Re-analysis of the 267-GHz ALMA observations of Venus: No statistically significant detection of phosphine — mentioned by _Nat_</title><link>https://news.ycombinator.com/item?id=24878354</link><guid isPermaLink="false">urn:hackerpapers:mention:2010.09761:24878354</guid><pubDate>Sat, 24 Oct 2020 10:53:38 GMT</pubDate><description>&lt;p&gt;[A study](https://arxiv.org/abs/2010.09761) posted 2020-10-19 challenges the claim that phosphine was detected in Venus&amp;#x27;s atmosphere. [The original claim](https://www.nature.com/articles/s41550-020-1174-4), posted 2020-10-14.&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2010.09761/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.EP</category></item><item><title>Re-analysis of the 267-GHz ALMA observations of Venus: No statistically significant detection of phosphine — HN submission</title><link>https://news.ycombinator.com/item?id=24854551</link><guid isPermaLink="false">urn:hackerpapers:submission:2010.09761:24854551</guid><pubDate>Thu, 22 Oct 2020 03:12:35 GMT</pubDate><description>&lt;p&gt;No statistically significant detection of phosphine on Venus&lt;/p&gt;&lt;p&gt;&lt;/p&gt;&lt;p&gt;2 points; 0 discussion replies on HN. &lt;a href="https://hackerpaper.kaipfister.de/p/2010.09761/"&gt;Paper and source history&lt;/a&gt;. A submission is not an endorsement.&lt;/p&gt;</description><category>astro-ph.EP</category></item><item><title>Re-analysis of the 267-GHz ALMA observations of Venus: No statistically significant detection of phosphine — HN submission</title><link>https://news.ycombinator.com/item?id=24847175</link><guid isPermaLink="false">urn:hackerpapers:submission:2010.09761:24847175</guid><pubDate>Wed, 21 Oct 2020 12:38:50 GMT</pubDate><description>&lt;p&gt;Re-analysis: No statistically significant detection of phosphine on Venus&lt;/p&gt;&lt;p&gt;&lt;/p&gt;&lt;p&gt;4 points; 1 discussion reply on HN. &lt;a href="https://hackerpaper.kaipfister.de/p/2010.09761/"&gt;Paper and source history&lt;/a&gt;. A submission is not an endorsement.&lt;/p&gt;</description><category>astro-ph.EP</category></item><item><title>Re-analysis of the 267-GHz ALMA observations of Venus: No statistically significant detection of phosphine — HN submission</title><link>https://news.ycombinator.com/item?id=24844142</link><guid isPermaLink="false">urn:hackerpapers:submission:2010.09761:24844142</guid><pubDate>Wed, 21 Oct 2020 01:53:54 GMT</pubDate><description>&lt;p&gt;Re-analysis of ALMA observations of Venus: No significant detection of phosphine&lt;/p&gt;&lt;p&gt;&lt;/p&gt;&lt;p&gt;5 points; 1 discussion reply on HN. &lt;a href="https://hackerpaper.kaipfister.de/p/2010.09761/"&gt;Paper and source history&lt;/a&gt;. A submission is not an endorsement.&lt;/p&gt;</description><category>astro-ph.EP</category></item></channel></rss>
