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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Spatially resolved imaging of the inner Fomalhaut disk using JWST/MIRI · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2305.03789/</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/2305.03789/feed.xml" rel="self" type="application/rss+xml" /><item><title>Spatially resolved imaging of the inner Fomalhaut disk using JWST/MIRI — mentioned by sbierwagen</title><link>https://news.ycombinator.com/item?id=35883345</link><guid isPermaLink="false">urn:hackerpapers:mention:2305.03789:35883345</guid><pubDate>Wed, 10 May 2023 03:36:19 GMT</pubDate><description>&lt;p&gt;To be clear, they were using the coronagraph: https://arxiv.org/pdf/2305.03789.pdf &amp;gt;The 23.0 µm coronagraph of MIRI uses a classic Lyot mask to achieve high contrast imaging near bright sources. The mask is rather large, providing an inner working angle (IWA) of ∼ 3.3λ/D, i.e., ∼ 2. Our data is the first complete reference PSF subtracted set of observations taken with JWST using this mode. There&amp;#x27;s some residual light and diffraction effects around the Lyot mask which they have manually deleted.&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2305.03789/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.EP</category></item></channel></rss>
