<?xml version="1.0" encoding="UTF-8"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-10-18T23:57:06Z</responseDate><request verb="GetRecord" identifier="oai:ebyu-rdlopen.rawdatalibrary.net:ebyu/15813" metadataPrefix="oai_dc">https://ebyu-rdlopen.rawdatalibrary.net/oai/request</request><GetRecord><record><header><identifier>oai:ebyu-rdlopen.rawdatalibrary.net:ebyu/15813</identifier><datestamp>2026-10-18T20:36:48Z</datestamp><setSpec>openaire</setSpec><setSpec>driver</setSpec><setSpec>com_ebyu_10000</setSpec><setSpec>col_ebyu_10001</setSpec></header><metadata><oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" 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:title>Chemical shift and intensity ratio values of dyspersium, holmium and erbium L X-ray emission lines</dc:title><dc:creator>Porikli, Sevil</dc:creator><dc:subject>Chemical environment changes</dc:subject><dc:subject>Chemical shift</dc:subject><dc:subject>Intensity ratio</dc:subject><dc:subject>Line position</dc:subject><dc:subject>Line width</dc:subject><dc:subject>XRF</dc:subject><dc:subject>Chemical compounds</dc:subject><dc:subject>Chemical elements</dc:subject><dc:subject>Dysprosium compounds</dc:subject><dc:subject>Electromagnetic wave emission</dc:subject><dc:subject>Emission spectroscopy</dc:subject><dc:subject>Erbium</dc:subject><dc:subject>Erbium compounds</dc:subject><dc:subject>Holmium</dc:subject><dc:subject>Holmium compounds</dc:subject><dc:subject>Radioactivity</dc:subject><dc:subject>X ray scattering</dc:subject><dc:subject>X rays</dc:subject><dc:subject>americium 241</dc:subject><dc:subject>dyspersium</dc:subject><dc:subject>metal</dc:subject><dc:subject>unclassified drug</dc:subject><dc:subject>Chemical effect</dc:subject><dc:subject>Chemical environment</dc:subject><dc:subject>Heavy elements</dc:subject><dc:subject>L X-rays</dc:subject><dc:subject>Line positions</dc:subject><dc:subject>Radioactive sources</dc:subject><dc:subject>Relative intensity</dc:subject><dc:subject>Si detectors</dc:subject><dc:description>A systematic study of L X-ray spectrum has been made on the elements Dy, Ho and Er in the pure form elements and compounds to look into the influence of chemical effect. The vacancies were created by 59.54keV γ-rays from an 241Am radioactive source. The L X-ray emission spectra of heavy elements taken with the currently available Si(Li) detectors show four or five distinct peaks. Corrections for sample absorption and spectrometer efficiency were applied to the measured relative intensities. The results show agreement with the theoretical predictions of Scofield (Scofield, 1974a). © 2011 Elsevier Ltd.</dc:description><dc:publisher>PERGAMON-ELSEVIER SCIENCE LTD</dc:publisher><dc:date>2012</dc:date><dc:type>Article</dc:type><dc:identifier>https://rdlopen.rawdatalibrary.net/r/ebyu/15813</dc:identifier><dc:identifier>https://doi.org/10.1016/j.radphyschem.2011.10.003</dc:identifier><dc:identifier>1879-0895</dc:identifier><dc:language>en</dc:language><dc:relation>Radiation Physics and Chemistry</dc:relation><dc:rights>info:eu-repo/semantics/openAccess</dc:rights><dc:type>info:eu-repo/semantics/article</dc:type><dc:identifier>https://ebyu-rdlopen.rawdatalibrary.net/tr/items/ebyu/15813</dc:identifier></oai_dc:dc></metadata></record></GetRecord></OAI-PMH>