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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using only Population II Distance Indicators · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1604.01788/</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/1604.01788/feed.xml" rel="self" type="application/rss+xml" /><item><title>The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using only Population II Distance Indicators — mentioned by sanxiyn</title><link>https://news.ycombinator.com/item?id=19838957</link><guid isPermaLink="false">urn:hackerpapers:mention:1604.01788:19838957</guid><pubDate>Mon, 06 May 2019 12:56:03 GMT</pubDate><description>&lt;p&gt;I am very excited about Wendy Freedman&amp;#x27;s number. Her program is called CCHP(Carnegie-Chicago Hubble Program). The first paper was in 2016: https://arxiv.org/abs/1604.01788. The idea is to use only Population II stars, while Adam Riess&amp;#x27;s number uses Population I stars. If the number is in between, that&amp;#x27;s really cool.&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1604.01788/"&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>
