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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Gravitational redshifting of galaxies in the SPIDERS cluster catalogue · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2102.11156/</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/2102.11156/feed.xml" rel="self" type="application/rss+xml" /><item><title>Gravitational redshifting of galaxies in the SPIDERS cluster catalogue — mentioned by Keysh</title><link>https://news.ycombinator.com/item?id=29604889</link><guid isPermaLink="false">urn:hackerpapers:mention:2102.11156:29604889</guid><pubDate>Sat, 18 Dec 2021 14:56:26 GMT</pubDate><description>&lt;p&gt;One important caveat to all this is that the gravitational redshift for a galaxy or galaxy cluster is an incredibly tiny effect. For example, the mean gravitational redshift for massive galaxy clusters has been measured (e.g., link below), and has a value of ~ 10 or 15 km/s. This can be compared with the typical motions of galaxies within a cluster (dispersions of ~ 1000 km/s) and the cosmological redshift of the clusters (for the sample in the paper I linked to, it&amp;#x27;s equivalent to an average Doppler shift of ~ 50,000 km/s). In order to make that measurement, the authors had to combine…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2102.11156/"&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>
