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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Limitations in timing precision due to single-pulse shape variability in millisecond pulsars · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1406.4716/</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/1406.4716/feed.xml" rel="self" type="application/rss+xml" /><item><title>Limitations in timing precision due to single-pulse shape variability in millisecond pulsars — mentioned by RedOrGreen</title><link>https://news.ycombinator.com/item?id=17465912</link><guid isPermaLink="false">urn:hackerpapers:mention:1406.4716:17465912</guid><pubDate>Thu, 05 Jul 2018 19:11:01 GMT</pubDate><description>&lt;p&gt;We can do even better some of the time - for example, we can get to ~few nanosecond timing precision for pulsars like J1909-3744 [1], which is equivalent to measuring (changes in) the path length to that pulsar to a few meters or better. [1] https://arxiv.org/abs/1406.4716&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1406.4716/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.SR</category></item></channel></rss>
