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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Understanding extreme quasar optical variability with CRTS: II. Changing-state quasars · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1905.02262/</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/1905.02262/feed.xml" rel="self" type="application/rss+xml" /><item><title>Understanding extreme quasar optical variability with CRTS: II. Changing-state quasars — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=37248590</link><guid isPermaLink="false">urn:hackerpapers:mention:1905.02262:37248590</guid><pubDate>Thu, 24 Aug 2023 13:34:45 GMT</pubDate><description>&lt;p&gt;Your question about pulsars is a good one and I&amp;#x27;ll answer it first, but the study at the top is about quasars, and I&amp;#x27;ll address that further below. With one exception all known pulsars are in the Milky Way; they are too intrinsically dim (and obscured by dust, much of which is local to them, produced in their progenitor star&amp;#x27;s explosive demise) to see them at extragalactic distances. The exception is PSR J0540-6919 in the Large Magellanic Cloud (the LMC, a satellite galaxy to the Milky Way), which is atypically bright in gamma rays and so is visible to the Fermi-GLAST telescope in low Earth…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1905.02262/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.GA</category></item></channel></rss>
