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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>A Near-Infrared Period-Luminosity Relation for Miras in NGC 4258, an Anchor for a New Distance Ladder · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1801.02711/</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/1801.02711/feed.xml" rel="self" type="application/rss+xml" /><item><title>A Near-Infrared Period-Luminosity Relation for Miras in NGC 4258, an Anchor for a New Distance Ladder — mentioned by xelxebar</title><link>https://news.ycombinator.com/item?id=16864812</link><guid isPermaLink="false">urn:hackerpapers:mention:1801.02711:16864812</guid><pubDate>Wed, 18 Apr 2018 05:14:19 GMT</pubDate><description>&lt;p&gt;Not quite sure, but I think this is the main paper in question: https://arxiv.org/abs/1801.02711 Just reading the titles of Riess&amp;#x27; other papers on arXiv gives an interesting peek at the clever work that went into getting this H0 measurement. Thanks for sharing!&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1801.02711/"&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>
