<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Photometric Redshifts | Dr. Kevin Hainline</title><link>https://kevinhainline.github.io/tags/photometric-redshifts/</link><atom:link href="https://kevinhainline.github.io/tags/photometric-redshifts/index.xml" rel="self" type="application/rss+xml"/><description>Photometric Redshifts</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Thu, 14 May 2026 00:00:00 +0000</lastBuildDate><image><url>https://kevinhainline.github.io/media/icon_hu13005498772911772797.png</url><title>Photometric Redshifts</title><link>https://kevinhainline.github.io/tags/photometric-redshifts/</link></image><item><title>Understanding EAZY-py</title><link>https://kevinhainline.github.io/post/eazy_py_guide/</link><pubDate>Thu, 14 May 2026 00:00:00 +0000</pubDate><guid>https://kevinhainline.github.io/post/eazy_py_guide/</guid><description>&lt;p>
, the photometric redshift code developed by
, is very commonly used in the extragalactic community for its speed and reliability. I&amp;rsquo;ve used it for years as a member of
, performing photometric redshift analysis on the catalog sources and
. Over the years, I&amp;rsquo;ve talked with many, many folks about the use cases for EAZY, and I decided to collect my thoughts into a website that guides folks through how to run EAZY, update templates and filters, and how to understand the output.&lt;/p>
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&lt;p>I&amp;rsquo;m sure there are probably errors and parts that are still confusing. Please let me know if you have any questions!&lt;/p></description></item></channel></rss>