<?xml version="1.0" encoding="UTF-8"?>
<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Parallax Beyond a Kiloparsec from Spatially Scanning the Wide Field Camera 3 on the Hubble Space Telescope · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1401.0484/</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/1401.0484/feed.xml" rel="self" type="application/rss+xml" /><item><title>Parallax Beyond a Kiloparsec from Spatially Scanning the Wide Field Camera 3 on the Hubble Space Telescope — mentioned by teraflop</title><link>https://news.ycombinator.com/item?id=17805163</link><guid isPermaLink="false">urn:hackerpapers:mention:1401.0484:17805163</guid><pubDate>Mon, 20 Aug 2018 23:33:13 GMT</pubDate><description>&lt;p&gt;&amp;quot;Accurate to within 100 light years&amp;quot; isn&amp;#x27;t really a meaningful statement. The page you linked to is a simplified explanation that says the method is only accurate enough to be used for stars within 100 light-years of Earth, which is approximately true. We have measurements of more distant stars, but they become increasingly inaccurate with distance. To be more precise, the relative error of a parallax distance measurement is proportional to both the measurement error and the distance. For example, the Hipparcos mission measured parallax with an accuract of roughly 0.001 arc-seconds. That…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1401.0484/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.IM</category></item></channel></rss>
