<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>Darryl E. Granger</dc:contributor>
  <dc:contributor>William E. Odom</dc:contributor>
  <dc:contributor>Brody Conner</dc:contributor>
  <dc:contributor>Lan Luo</dc:contributor>
  <dc:creator>Xianmei Huang</dc:creator>
  <dc:date>2025</dc:date>
  <dc:description>&lt;p&gt;&lt;i&gt;In situ&lt;/i&gt;&lt;span&gt;-produced&amp;nbsp;&lt;/span&gt;&lt;sup&gt;10&lt;/sup&gt;&lt;span&gt;Be in quartz is widely used to constrain exposure ages and denudation rates, traditionally measured in sand-sized grains. Here we report a new method for isolating fine-grained quartz from shale and demonstrate its reliability for grain sizes down to single microns. Sequential dissolution tests and analyses of grain size separates show that meteoric&amp;nbsp;&lt;/span&gt;&lt;sup&gt;10&lt;/sup&gt;&lt;span&gt;Be is eliminated and that recoil losses during cosmogenic nuclide production are balanced by implantation from other mineral grains. High-temperature combustion leads to diffusion of meteoric&amp;nbsp;&lt;/span&gt;&lt;sup&gt;10&lt;/sup&gt;&lt;span&gt;Be into fine-grained quartz and must be used with caution.&lt;/span&gt;&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1016/j.nimb.2025.165913</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>Elsevier</dc:publisher>
  <dc:title>Measurement of in situ-produced cosmogenic nuclides in fine-grained quartz from shale</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>