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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Multi-messenger Observations of a Binary Neutron Star Merger · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1710.05833/</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/1710.05833/feed.xml" rel="self" type="application/rss+xml" /><item><title>Multi-messenger Observations of a Binary Neutron Star Merger — mentioned by wlesieutre</title><link>https://news.ycombinator.com/item?id=28990045</link><guid isPermaLink="false">urn:hackerpapers:mention:1710.05833:28990045</guid><pubDate>Mon, 25 Oct 2021 16:49:23 GMT</pubDate><description>&lt;p&gt;https://arxiv.org/abs/1710.05833 &amp;gt; On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ∼1.7 s with respect to the merger time. So there is a delay between arrival of gravitational waves and accompanying gamma ray burst, but I couldn&amp;#x27;t tell you if that&amp;#x27;s purely because light travels slower than it would in a perfect vacuum…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1710.05833/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.HE</category></item><item><title>Multi-messenger Observations of a Binary Neutron Star Merger — mentioned by magicalhippo</title><link>https://news.ycombinator.com/item?id=23152884</link><guid isPermaLink="false">urn:hackerpapers:mention:1710.05833:23152884</guid><pubDate>Tue, 12 May 2020 11:38:47 GMT</pubDate><description>&lt;p&gt;&amp;gt; What&amp;#x27;s the breakthrough that another telescope at the cost of $Bs would achieve? Multi-messenger astronomy[1] seems to be the next big thing. Will we lose out if we don&amp;#x27;t have a good optical telescope &amp;quot;up there&amp;quot;? Or is the current crop of gamma/x-ray and IR satellite telescopes coupled with ground-based optical telescopes good enough? I understand adaptive optics and such has drastically improved the capabilities of ground-based telescopes, but for MMA (to hijack the acronym) are there any advantages of a space-based optical telescope? [1]: https://arxiv.org/abs/1710.05833&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1710.05833/"&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>
