<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Radio Astronomy | A Quest After Perspectives</title><link>https://iphysresearch.github.io/blog/tag/radio-astronomy/</link><atom:link href="https://iphysresearch.github.io/blog/tag/radio-astronomy/index.xml" rel="self" type="application/rss+xml"/><description>Radio Astronomy</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Tue, 22 Jul 2025 00:00:00 +0000</lastBuildDate><image><url>https://iphysresearch.github.io/blog/media/sharing.png</url><title>Radio Astronomy</title><link>https://iphysresearch.github.io/blog/tag/radio-astronomy/</link></image><item><title>Real-Time Galactic Neutral Hydrogen Signals HI Detection: “Probing the 1.42 GHz, 21-cm Line” with Fabricated Conical Horn Radio Astronomy Telescope</title><link>https://iphysresearch.github.io/blog/mypublication/2025_hi_horn_telescope/</link><pubDate>Tue, 22 Jul 2025 00:00:00 +0000</pubDate><guid>https://iphysresearch.github.io/blog/mypublication/2025_hi_horn_telescope/</guid><description>&lt;p>The instrument combines a horn antenna, preamplification, and spectral measurements. The study focuses on an accessible setup for observing neutral-hydrogen emission and supporting educational radio astronomy.&lt;/p>
&lt;h2 id="sources">Sources&lt;/h2>
&lt;ul>
&lt;li>&lt;a href="https://www.techrxiv.org/doi/full/10.36227/techrxiv.175321744.43581339/v1" target="_blank" rel="noopener">TechRxiv record&lt;/a>&lt;/li>
&lt;li>&lt;a href="https://api.crossref.org/works/10.36227/techrxiv.175321744.43581339/v1" target="_blank" rel="noopener">Publisher metadata via Crossref&lt;/a>&lt;/li>
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