<?xml version='1.0' encoding='UTF-8'?><codeBook xmlns="ddi:codebook:2_5" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="ddi:codebook:2_5 https://ddialliance.org/Specification/DDI-Codebook/2.5/XMLSchema/codebook.xsd" version="2.5" xml:lang="en"><docDscr><citation><titlStmt><titl xml:lang="en">Cobalt</titl><IDNo agency="DOI">doi:10.57979/08PIRG</IDNo></titlStmt><distStmt><distrbtr source="archive">POLEN DataHub</distrbtr><distDate>2026-03-30</distDate></distStmt><verStmt source="archive"><version date="2026-03-30" type="RELEASED">1</version></verStmt><biblCit>Guerra, Mauro; Machado, Jorge; Pinheiro, Daniel; Baptista, Gonçalo; Godinho, César; Fernandes, André; Amaro, Pedro; Sampaio, Jorge Miguel; Marques, José Pires; Parente, Fernando; Santos, José Paulo, 2026, "Cobalt", https://doi.org/10.57979/08PIRG, POLEN DataHub, V1</biblCit></citation></docDscr><stdyDscr><citation><titlStmt><titl xml:lang="en">Cobalt</titl><IDNo agency="DOI">doi:10.57979/08PIRG</IDNo></titlStmt><rspStmt><AuthEnty affiliation="Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa">Guerra, Mauro</AuthEnty><AuthEnty affiliation="Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa">Machado, Jorge</AuthEnty><AuthEnty affiliation="Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa">Pinheiro, Daniel</AuthEnty><AuthEnty affiliation="Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa">Baptista, Gonçalo</AuthEnty><AuthEnty affiliation="Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa">Godinho, César</AuthEnty><AuthEnty affiliation="Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa">Fernandes, André</AuthEnty><AuthEnty affiliation="Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa">Amaro, Pedro</AuthEnty><AuthEnty affiliation="Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa">Sampaio, Jorge Miguel</AuthEnty><AuthEnty affiliation="Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa">Marques, José Pires</AuthEnty><AuthEnty affiliation="Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa">Parente, Fernando</AuthEnty><AuthEnty affiliation="Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa">Santos, José Paulo</AuthEnty></rspStmt><prodStmt><prodDate>2026-03-27</prodDate><grantNo agency="Fundação para a Ciência e Tecnologia (FCT)">PTDC/FIS-AQM/31969/2017</grantNo></prodStmt><distStmt><distrbtr source="archive">POLEN DataHub</distrbtr><contact affiliation="Faculdade de Ciências e Tecnologia da Universidade Nova de Lisboa" email="mguerra@fct.unl.pt">Mauro Guerra</contact><depositr>Santos, Elis</depositr><depDate>2026-03-27</depDate></distStmt><holdings URI="https://doi.org/10.57979/08PIRG"/></citation><stdyInfo><subject><keyword xml:lang="en">Exact Sciences - Physical Sciences - Atomic Physics</keyword><keyword>X-ray interaction with matter</keyword><keyword>X-ray emission</keyword><keyword>Auger Emission</keyword><keyword>Fluorescence Yields</keyword><keyword>Line Energies</keyword><keyword>Line Widths</keyword><keyword>Spectral Shapes</keyword><keyword>Satellite Lines</keyword><keyword>Shake-Up</keyword><keyword>Shake-Off</keyword><keyword>Atomic spectra</keyword><topcClas vocab="PhySH - Physics Subject Headings" vocabURI="https://physh.org/concepts/30e65d01-6cd5-442b-889f-ddc0c3c28157">Atomic &amp; molecular structure</topcClas></subject><abstract date="2023-05-31" xml:lang="en">Cobalt</abstract><sumDscr/></stdyInfo><method><dataColl><sources/></dataColl><anlyInfo/></method><dataAccs><setAvail/><useStmt/><notes type="DVN:TOU" level="dv">&lt;a href="http://creativecommons.org/licenses/by/4.0">CC BY 4.0&lt;/a></notes></dataAccs><othrStdyMat><relStdy>Guerra, Mauro; Machado, Jorge; Pinheiro, Daniel; Baptista, Gonçalo; Godinho, César; Fernandes, André; Amaro, Pedro; Sampaio, Jorge Miguel; Marques, José Pires; Parente, Fernando; Santos, José Paulo, 2026, "Silver", &lt;a href="https://doi.org/10.57979/V8TQDW">https://doi.org/10.57979/V8TQDW&lt;/a></relStdy><relStdy>&lt;br>
&lt;br>Guerra, Mauro; Machado, Jorge; Pinheiro, Daniel; Baptista, Gonçalo; Godinho, César; Fernandes, André; Amaro, Pedro; Sampaio, Jorge Miguel; Marques, José Pires; Parente, Fernando; Santos, José Paulo, 2023, "Magnesium", &lt;a href="https://doi.org/10.57979/L2ERID">https://doi.org/10.57979/L2ERID&lt;/a></relStdy><relStdy>&lt;br>
&lt;br>Guerra, Mauro; Machado, Jorge; Pinheiro, Daniel; Baptista, Gonçalo; Godinho, César; Fernandes, André; Amaro, Pedro; Sampaio, Jorge Miguel; Marques, José Pires; Parente, Fernando; Santos, José Paulo, 2026, "Cadmium", &lt;a href="https://doi.org/10.57979/0K9RDJ">https://doi.org/10.57979/0K9RDJ&lt;/a></relStdy><relStdy>&lt;br>
&lt;br>Guerra, Mauro; Machado, Jorge; Pinheiro, Daniel; Baptista, Gonçalo; Godinho, César; Fernandes, André; Amaro, Pedro; Sampaio, Jorge Miguel; Marques, José Pires; Parente, Fernando; Santos, José Paulo, 2026, "Cuper", &lt;a href="https://doi.org/10.57979/BZA2WF">https://doi.org/10.57979/BZA2WF&lt;/a></relStdy><relStdy>&lt;br>
&lt;br>Guerra, Mauro; Machado, Jorge; Pinheiro, Daniel; Baptista, Gonçalo; Godinho, César; Fernandes, André; Amaro, Pedro; Sampaio, Jorge Miguel; Marques, José Pires; Parente, Fernando; Santos, José Paulo, 2026, "Palladium", &lt;a href="https://doi.org/10.57979/O47FWP">https://doi.org/10.57979/O47FWP&lt;/a></relStdy><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Ito et al., 2023.&lt;/strong>&lt;a href="https://www.mdpi.com/1422-0067/24/6/5570">Intensity Ratio of Kβ/Kα in Selected Elements from Mg to Cu, and the Chemical Effects of Cr Kα1,2 Diagram Lines and Cr Kβ/Kα Intensity Ratio in Cr Compounds&lt;/a>. &lt;i>International Journal of Molecular Sciences, 24(6), 5570.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.3390/ijms24065570</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Ito et al., 2023.&lt;/strong>&lt;a href="https://www.mdpi.com/1422-0067/24/6/5570">Intensity Ratio of Kβ/Kα in Selected Elements from Mg to Cu, and the Chemical Effects of Cr Kα1,2 Diagram Lines and Cr Kβ/Kα Intensity Ratio in Cr Compounds&lt;/a>. &lt;i>International Journal of Molecular Sciences, 24(6), 5570.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.3390/ijms24065570"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Pinheiro et al., 2023.&lt;/strong>
&lt;a href="https://doi.org/10.1016/j.radphyschem.2022.110595">Angular distribution of characteristic X-rays following electron impact ionization&lt;/a>. &lt;i>Radiation Physics and Chemistry, 203, 110595.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1016/j.radphyschem.2022.110595</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Pinheiro et al., 2023.&lt;/strong>
&lt;a href="https://doi.org/10.1016/j.radphyschem.2022.110595">Angular distribution of characteristic X-rays following electron impact ionization&lt;/a>. &lt;i>Radiation Physics and Chemistry, 203, 110595.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1016/j.radphyschem.2022.110595"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Pinheiro et al., 2023.&lt;/strong>&lt;a href="https://www.sciencedirect.com/science/article/pii/S0969806X22006569">K- and L-shell theoretical fluorescence yields for the Fe isonuclear sequence&lt;/a>.&lt;i>Radiation Physics and Chemistry, 203, 110594.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1016/j.radphyschem.2022.110594</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Pinheiro et al., 2023.&lt;/strong>&lt;a href="https://www.sciencedirect.com/science/article/pii/S0969806X22006569">K- and L-shell theoretical fluorescence yields for the Fe isonuclear sequence&lt;/a>.&lt;i>Radiation Physics and Chemistry, 203, 110594.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1016/j.radphyschem.2022.110594"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Hönicke et al., 2023.&lt;/strong>&lt;a href="https://doi.org/10.1016/j.radphyschem.2022.110501">Experimental and theoretical approaches for establishing the K-shell fluorescence yield of carbon&lt;/a>. &lt;i>Radiation Physics and Chemistry, 202, 110501.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1016/j.radphyschem.2022.110501</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Hönicke et al., 2023.&lt;/strong>&lt;a href="https://doi.org/10.1016/j.radphyschem.2022.110501">Experimental and theoretical approaches for establishing the K-shell fluorescence yield of carbon&lt;/a>. &lt;i>Radiation Physics and Chemistry, 202, 110501.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1016/j.radphyschem.2022.110501"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Guerra et al., 2021.&lt;/strong>&lt;a href="https://www.mdpi.com/2218-2004/9/1/8">Fundamental Parameters Related to Selenium Kα and Kβ Emission X-ray Spectra&lt;/a>. &lt;i>Atoms, 9(1), 8.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.3390/atoms9010008</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Guerra et al., 2021.&lt;/strong>&lt;a href="https://www.mdpi.com/2218-2004/9/1/8">Fundamental Parameters Related to Selenium Kα and Kβ Emission X-ray Spectra&lt;/a>. &lt;i>Atoms, 9(1), 8.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.3390/atoms9010008"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Ito et al., 2020.&lt;/strong>&lt;a href="https://doi.org/10.1103/PhysRevA.102.052820">Structure of Kα1,2- and Kβ1,3-emission x-ray spectra for Se, Y, and Zr&lt;/a>. &lt;i>Physical Review A, 102(5), 052820.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1103/PhysRevA.102.052820</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Ito et al., 2020.&lt;/strong>&lt;a href="https://doi.org/10.1103/PhysRevA.102.052820">Structure of Kα1,2- and Kβ1,3-emission x-ray spectra for Se, Y, and Zr&lt;/a>. &lt;i>Physical Review A, 102(5), 052820.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1103/PhysRevA.102.052820"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Martins et al., 2020.&lt;/strong>&lt;a href="https://doi.org/10.1002/xrs.3123">Overview and calculation of X-ray K-shell transition yields for comprehensive data libraries&lt;/a>. &lt;i>X-Ray Spectrometry, 49(3), 398–423.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1002/xrs.3123</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Martins et al., 2020.&lt;/strong>&lt;a href="https://doi.org/10.1002/xrs.3123">Overview and calculation of X-ray K-shell transition yields for comprehensive data libraries&lt;/a>. &lt;i>X-Ray Spectrometry, 49(3), 398–423.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1002/xrs.3123"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Ménesguen et al., 2019.&lt;/strong>&lt;a href="https://doi.org/10.1016/j.jqsrt.2019.106585">Precise x-ray energies of gadolinium determined by a combined experimental and theoretical approach&lt;/a>. &lt;i>Journal of Quantitative Spectroscopy and Radiative Transfer, 236, 106585.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1016/j.jqsrt.2019.106585</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Ménesguen et al., 2019.&lt;/strong>&lt;a href="https://doi.org/10.1016/j.jqsrt.2019.106585">Precise x-ray energies of gadolinium determined by a combined experimental and theoretical approach&lt;/a>. &lt;i>Journal of Quantitative Spectroscopy and Radiative Transfer, 236, 106585.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1016/j.jqsrt.2019.106585"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Martins et al., 2020.&lt;/strong>&lt;a href="https://doi.org/10.1002/xrs.3089"> Multiconfiguration Dirac-Fock calculations of Zn K-shell radiative and nonradiative transtitions&lt;/a>. &lt;i> X-ray Spectrom. 49, 192-199.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1002/xrs.3089</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Martins et al., 2020.&lt;/strong>&lt;a href="https://doi.org/10.1002/xrs.3089"> Multiconfiguration Dirac-Fock calculations of Zn K-shell radiative and nonradiative transtitions&lt;/a>. &lt;i> X-ray Spectrom. 49, 192-199.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1002/xrs.3089"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Zeeshan et al., 2019.&lt;/strong>&lt;a href="https://doi.org/10.1002/xrs.3019">Diagram, valence-to-core and hypersatellite Kβ X-ray transitions in metallic chromium&lt;/a>. &lt;i>X-Ray Spectrometry, 48(5), 351–359.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1002/xrs.3019</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Zeeshan et al., 2019.&lt;/strong>&lt;a href="https://doi.org/10.1002/xrs.3019">Diagram, valence-to-core and hypersatellite Kβ X-ray transitions in metallic chromium&lt;/a>. &lt;i>X-Ray Spectrometry, 48(5), 351–359.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1002/xrs.3019"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Ménesguen et al., 2018.&lt;/strong>&lt;a href="https://doi.org/10.1002/xrs.2948">A combined experimental and theoretical approach to determine X-ray atomic fundamental quantities of tin&lt;/a>. &lt;i>X-Ray Spectrometry, 47(5), 341–351.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1002/xrs.2948</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Ménesguen et al., 2018.&lt;/strong>&lt;a href="https://doi.org/10.1002/xrs.2948">A combined experimental and theoretical approach to determine X-ray atomic fundamental quantities of tin&lt;/a>. &lt;i>X-Ray Spectrometry, 47(5), 341–351.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1002/xrs.2948"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Ito et al., 2018.&lt;/strong>&lt;a href="https://doi.org/10.1103/PhysRevA.97.052505">Structure of high-resolution K β 1 , 3 x-ray emission spectra for the elements from Ca to Ge&lt;/a>. &lt;i>Physical Review A, 97(5), 052505.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1103/PhysRevA.97.052505</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Ito et al., 2018.&lt;/strong>&lt;a href="https://doi.org/10.1103/PhysRevA.97.052505">Structure of high-resolution K β 1 , 3 x-ray emission spectra for the elements from Ca to Ge&lt;/a>. &lt;i>Physical Review A, 97(5), 052505.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1103/PhysRevA.97.052505"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Ménesguen et al., 2018.&lt;/strong>&lt;a href="https://doi.org/10.1088/1681-7575/aad1d6">Experimental and theoretical determination of the L-fluorescence yields of bismuth&lt;/a>. &lt;i>Metrologia, 55(5), 621–630.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1088/1681-7575/aad1d6"</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Ménesguen et al., 2018.&lt;/strong>&lt;a href="https://doi.org/10.1088/1681-7575/aad1d6">Experimental and theoretical determination of the L-fluorescence yields of bismuth&lt;/a>. &lt;i>Metrologia, 55(5), 621–630.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1088/1681-7575/aad1d6"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Guerra et al., 2018.&lt;/strong>&lt;a href="https://doi.org/10.1103/PhysRevA.97.042501">Theoretical and experimental determination of K- and L-shell X-ray relaxation parameters in Ni&lt;/a>. &lt;i>Physical Review A, 97(4), 042501.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1103/PhysRevA.97.042501</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Guerra et al., 2018.&lt;/strong>&lt;a href="https://doi.org/10.1103/PhysRevA.97.042501">Theoretical and experimental determination of K- and L-shell X-ray relaxation parameters in Ni&lt;/a>. &lt;i>Physical Review A, 97(4), 042501.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1103/PhysRevA.97.042501"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Guerra et al., 2017.&lt;/strong>&lt;a href="https://doi.org/10.1016/j.adt.2017.01.001">Relativistic calculations of screening parameters and atomic radii of neutral atoms&lt;/a>. &lt;i>Atomic Data and Nuclear Data Tables, 117–118, 439–457.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1016/j.adt.2017.01.001</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Guerra et al., 2017.&lt;/strong>&lt;a href="https://doi.org/10.1016/j.adt.2017.01.001">Relativistic calculations of screening parameters and atomic radii of neutral atoms&lt;/a>. &lt;i>Atomic Data and Nuclear Data Tables, 117–118, 439–457.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1016/j.adt.2017.01.001"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Kup Aylikci et al., 2017.&lt;/strong>&lt;a href="https://doi.org/10.1002/xrs.2763"> The investigation of K-shell fluorescence parameters of Zn-Fe alloys with different grain size and microstrain values&lt;/a>. &lt;i>X-Ray Spectrometry, 46(4), 242–251.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1002/xrs.2763</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Kup Aylikci et al., 2017.&lt;/strong>&lt;a href="https://doi.org/10.1002/xrs.2763"> The investigation of K-shell fluorescence parameters of Zn-Fe alloys with different grain size and microstrain values&lt;/a>. &lt;i>X-Ray Spectrometry, 46(4), 242–251.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1002/xrs.2763"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Sampaio et al., 2016.&lt;/strong>&lt;a href="https://doi.org/10.1016/j.jqsrt.2016.05.012">Relativistic Calculations of K-, L- and M-shell X-ray production cross-sections by electron impact for Ne, Ar, Kr, Xe, Rn and Uuo&lt;/a>. &lt;i>Journal of Quantitative Spectroscopy and Radiative Transfer, 182, 87–93. &lt;/i>&lt;/p></titl><IDNo agency="doi">10.1016/j.jqsrt.2016.05.012</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Sampaio et al., 2016.&lt;/strong>&lt;a href="https://doi.org/10.1016/j.jqsrt.2016.05.012">Relativistic Calculations of K-, L- and M-shell X-ray production cross-sections by electron impact for Ne, Ar, Kr, Xe, Rn and Uuo&lt;/a>. &lt;i>Journal of Quantitative Spectroscopy and Radiative Transfer, 182, 87–93. &lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1016/j.jqsrt.2016.05.012"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Sampaio et al., 2016.&lt;/strong>&lt;a href="https://doi.org/10.1016/j.adt.2016.02.001">Calculations of Photo-Induced X-ray Production Cross-sections in the energy range 1-150 keV and Average Fluorescence Yields for Zn, Cd and Hg&lt;/a>. &lt;i>Atomic Data and Nuclear Data Tables, 111–112, 67–86.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1016/j.adt.2016.02.001</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Sampaio et al., 2016.&lt;/strong>&lt;a href="https://doi.org/10.1016/j.adt.2016.02.001">Calculations of Photo-Induced X-ray Production Cross-sections in the energy range 1-150 keV and Average Fluorescence Yields for Zn, Cd and Hg&lt;/a>. &lt;i>Atomic Data and Nuclear Data Tables, 111–112, 67–86.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1016/j.adt.2016.02.001"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Sampaio et al., 2015.&lt;/strong>&lt;a href="https://doi.org/10.1088/1742-6596/635/9/092095"> Relativistic calculations of atomic parameters in Ununoctium&lt;/a>. &lt;i>Journal of Physics: Conference Series, 635(9), 092095.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1088/1742-6596/635/9/092095</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Sampaio et al., 2015.&lt;/strong>&lt;a href="https://doi.org/10.1088/1742-6596/635/9/092095"> Relativistic calculations of atomic parameters in Ununoctium&lt;/a>. &lt;i>Journal of Physics: Conference Series, 635(9), 092095.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1088/1742-6596/635/9/092095"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Marques et al., 2015.&lt;/strong>&lt;a href="https://doi.org/10.1088/1742-6596/635/9/092094">K-shell width, fluorescence yield, and Kβ/Kα intensity ratio calculation for Fe in the Dirac-Fock approach&lt;/a>. &lt;i>Journal of Physics: Conference Series, 635(9), 092094.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1088/1742-6596/635/9/092094</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Marques et al., 2015.&lt;/strong>&lt;a href="https://doi.org/10.1088/1742-6596/635/9/092094">K-shell width, fluorescence yield, and Kβ/Kα intensity ratio calculation for Fe in the Dirac-Fock approach&lt;/a>. &lt;i>Journal of Physics: Conference Series, 635(9), 092094.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1088/1742-6596/635/9/092094"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Guerra et al., 2015.&lt;/strong>&lt;a href="https://doi.org/10.1103/PhysRevA.92.022507">Theoretical and experimental determination of L-shell decay rates, linewidths and fluorescence yields in Ge&lt;/a>. &lt;i>Physical Review A, 92(2), 022507.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1103/PhysRevA.92.022507</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Guerra et al., 2015.&lt;/strong>&lt;a href="https://doi.org/10.1103/PhysRevA.92.022507">Theoretical and experimental determination of L-shell decay rates, linewidths and fluorescence yields in Ge&lt;/a>. &lt;i>Physical Review A, 92(2), 022507.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1103/PhysRevA.92.022507"/></relPubl><relPubl><citation><titlStmt><titl>&lt;br>
&lt;p>&lt;strong>Sampaio et al., 2015.&lt;/strong>&lt;a href="https://doi.org/10.1103/PhysRevA.91.052507">Dirac-Fock calculations of K-, L-, and M-shell fluorescence and Coster-Kronig yields for Ne, Ar, Kr, Xe, Rn, and Uuo&lt;/a>. &lt;i>Physical Review A, 91(5), 052507.&lt;/i>&lt;/p></titl><IDNo agency="doi">10.1103/PhysRevA.91.052507</IDNo></titlStmt><biblCit>&lt;br>
&lt;p>&lt;strong>Sampaio et al., 2015.&lt;/strong>&lt;a href="https://doi.org/10.1103/PhysRevA.91.052507">Dirac-Fock calculations of K-, L-, and M-shell fluorescence and Coster-Kronig yields for Ne, Ar, Kr, Xe, Rn, and Uuo&lt;/a>. &lt;i>Physical Review A, 91(5), 052507.&lt;/i>&lt;/p></biblCit></citation><ExtLink URI="https://doi.org/10.1103/PhysRevA.91.052507"/></relPubl></othrStdyMat></stdyDscr><otherMat ID="f287" URI="https://datahub.polen.fccn.pt/api/access/datafile/287" level="datafile"><labl>Co_rates_auger.txt</labl><notes level="file" type="DATAVERSE:CONTENTTYPE" subject="Content/MIME Type">text/plain</notes></otherMat><otherMat ID="f284" URI="https://datahub.polen.fccn.pt/api/access/datafile/284" level="datafile"><labl>Co_rates_radiative.txt</labl><notes level="file" type="DATAVERSE:CONTENTTYPE" subject="Content/MIME Type">text/plain</notes></otherMat><otherMat ID="f288" URI="https://datahub.polen.fccn.pt/api/access/datafile/288" level="datafile"><labl>Co_rates_sums.txt</labl><notes level="file" type="DATAVERSE:CONTENTTYPE" subject="Content/MIME Type">text/plain</notes></otherMat><otherMat ID="f286" URI="https://datahub.polen.fccn.pt/api/access/datafile/286" level="datafile"><labl>Co_rates_sums_sat.txt</labl><notes level="file" type="DATAVERSE:CONTENTTYPE" subject="Content/MIME Type">text/plain</notes></otherMat><otherMat ID="f285" URI="https://datahub.polen.fccn.pt/api/access/datafile/285" level="datafile"><labl>Co_spectrum_auger.txt</labl><notes level="file" type="DATAVERSE:CONTENTTYPE" subject="Content/MIME Type">text/plain</notes></otherMat><otherMat ID="f289" URI="https://datahub.polen.fccn.pt/api/access/datafile/289" level="datafile"><labl>Co_spectrum_diagram.txt</labl><notes level="file" type="DATAVERSE:CONTENTTYPE" subject="Content/MIME Type">text/plain</notes></otherMat><otherMat ID="f290" URI="https://datahub.polen.fccn.pt/api/access/datafile/290" level="datafile"><labl>Co_spectrum_sat.txt</labl><notes level="file" type="DATAVERSE:CONTENTTYPE" subject="Content/MIME Type">text/plain</notes></otherMat><otherMat ID="f291" URI="https://datahub.polen.fccn.pt/api/access/datafile/291" level="datafile"><labl>readme.pdf</labl><txt>Readme file for all the files on this dataset.</txt><notes level="file" type="DATAVERSE:CONTENTTYPE" subject="Content/MIME Type">application/pdf</notes></otherMat></codeBook>