<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="zh-Hans-CN">
	<id>http://202.127.29.3/~shen/wiki/index.php?action=history&amp;feed=atom&amp;title=UV_slope</id>
	<title>UV slope - 版本历史</title>
	<link rel="self" type="application/atom+xml" href="http://202.127.29.3/~shen/wiki/index.php?action=history&amp;feed=atom&amp;title=UV_slope"/>
	<link rel="alternate" type="text/html" href="http://202.127.29.3/~shen/wiki/index.php?title=UV_slope&amp;action=history"/>
	<updated>2026-04-21T09:29:10Z</updated>
	<subtitle>本wiki上该页面的版本历史</subtitle>
	<generator>MediaWiki 1.38.1</generator>
	<entry>
		<id>http://202.127.29.3/~shen/wiki/index.php?title=UV_slope&amp;diff=4063&amp;oldid=prev</id>
		<title>Shen：​创建页面，内容为“ arXiv:2405.20901 *This study&#039;s substantial sample size provides a benchmark for demonstrating that the rest-frame UV spectral slope correlates with stellar mass-dep…”</title>
		<link rel="alternate" type="text/html" href="http://202.127.29.3/~shen/wiki/index.php?title=UV_slope&amp;diff=4063&amp;oldid=prev"/>
		<updated>2024-06-03T08:22:30Z</updated>

		<summary type="html">&lt;p&gt;创建页面，内容为“ arXiv:2405.20901 *This study&amp;#039;s substantial sample size provides a benchmark for demonstrating that the rest-frame UV spectral slope correlates with stellar mass-dep…”&lt;/p&gt;
&lt;p&gt;&lt;b&gt;新页面&lt;/b&gt;&lt;/p&gt;&lt;div&gt; arXiv:2405.20901&lt;br /&gt;
*This study&amp;#039;s substantial sample size provides a benchmark for demonstrating that the rest-frame UV spectral slope correlates with stellar mass-dependent galaxy characteristics at z∼2−4, a relationship less discernible with smaller datasets typically available at higher redshifts.&lt;/div&gt;</summary>
		<author><name>Shen</name></author>
	</entry>
</feed>