<?xml version="1.0" encoding="UTF-8"?>
<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Atmospheric Cherenkov Gamma-ray Telescopes · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1510.05675/</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/1510.05675/feed.xml" rel="self" type="application/rss+xml" /><item><title>Atmospheric Cherenkov Gamma-ray Telescopes — mentioned by gattr</title><link>https://news.ycombinator.com/item?id=17519298</link><guid isPermaLink="false">urn:hackerpapers:mention:1510.05675:17519298</guid><pubDate>Thu, 12 Jul 2018 22:54:43 GMT</pubDate><description>&lt;p&gt;If anyone&amp;#x27;s interested in other unusual (i.e. other than an optical imaging telescope) detectors, have a look at Imaging Atmospheric Cherenkov Telescopes [0]. More details can be found e.g. in [1]. TL;DR: how to detect a very high-energy gamma-ray photon? Either with an orbital observatory (but these have limited size); or let the photon hit upper atmosphere (at a few tens of km), create (together with some atmospheric nucleus) a fast electron-positron pair, which through additional interactions eventually causes a narrow cone of Cherenkov light to shine all the way down to the ground (having…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1510.05675/"&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>
