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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Detection of intercluster gas in superclusters using the thermal Sunyaev-Zel'dovich effect · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1805.04555/</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/1805.04555/feed.xml" rel="self" type="application/rss+xml" /><item><title>Detection of intercluster gas in superclusters using the thermal Sunyaev-Zel'dovich effect — mentioned by nfc</title><link>https://news.ycombinator.com/item?id=17955961</link><guid isPermaLink="false">urn:hackerpapers:mention:1805.04555:17955961</guid><pubDate>Mon, 10 Sep 2018 23:21:19 GMT</pubDate><description>&lt;p&gt;You are right that this could be the case, and it&amp;#x27;s mentioned in at least one of the papers [1] where they say that a better understanding of the physical state of this gas is needed to estimate its contributions to the baryonic mass. [1] https://arxiv.org/abs/1805.04555 Now we can get to discuss the third paper ;)&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1805.04555/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.CO</category></item></channel></rss>
