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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1912.05705/</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/1912.05705/feed.xml" rel="self" type="application/rss+xml" /><item><title>PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter — mentioned by srl</title><link>https://news.ycombinator.com/item?id=26958502</link><guid isPermaLink="false">urn:hackerpapers:mention:1912.05705:26958502</guid><pubDate>Tue, 27 Apr 2021 16:55:49 GMT</pubDate><description>&lt;p&gt;Relatedly, NICER (an X-Ray telescope) launched in 2017, and has been observing pulsars to get radius measurements since then. See for instance https://arxiv.org/abs/1912.05705. (I think there&amp;#x27;s a more recent measurement but I can&amp;#x27;t find it on arXiv.) I don&amp;#x27;t have a good understanding of the relationships between all the different methods, but I do know that NICER&amp;#x27;s measurements have systematically given larger radii (albeit with huge error bars) than other methods do.&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1912.05705/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.HE</category></item></channel></rss>
