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        <identifier>oai:figshare.com:article/22240831</identifier>
        <datestamp>2023-09-28T10:28:55Z</datestamp>
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          <identifier identifierType="DOI">10.5522/04/22240831.v1</identifier>
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            <alternateIdentifier alternateIdentifierType="URL">https://figshare.com/articles/dataset/XAFS_IR_data_from_publication_entitled_A_High_Pressure_Operando_Spectroscopy_Examination_of_Bimetal_Interactions_in_Metal_Efficient_Palladium_In2O3_Al2O3_Catalysts_for_CO2_hydrogenation/22240831</alternateIdentifier>
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            <relatedIdentifier relatedIdentifierType="DOI" relationType="IsSupplementTo">10.1002/ange.202312645</relatedIdentifier>
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          <creators>
            <creator>
              <creatorName>Beale, Andrew</creatorName>
              <givenName>Andrew</givenName>
              <familyName>Beale</familyName>
            </creator>
            <creator>
              <creatorName>Potter, Matthew</creatorName>
              <givenName>Matthew</givenName>
              <familyName>Potter</familyName>
            </creator>
            <creator>
              <creatorName>Allen, Lisa</creatorName>
              <givenName>Lisa</givenName>
              <familyName>Allen</familyName>
            </creator>
            <creator>
              <creatorName>Vyas, Urvashi</creatorName>
              <givenName>Urvashi</givenName>
              <familyName>Vyas</familyName>
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          <titles>
            <title><![CDATA[XAFS & IR data from publication entitled: A High Pressure Operando Spectroscopy Examination of Bimetal Interactions in ‘Metal Efficient’ Palladium/In2O3/Al2O3 Catalysts for CO2 hydrogenation]]></title>
          </titles>
          <subjects>
            <subject>Analytical spectrometry</subject>
            <subject>Physical properties of materials</subject>
            <subject>Other chemical sciences not elsewhere classified</subject>
            <subject>Structural Chemistry and Spectroscopy</subject>
            <subject>Physical Chemistry of Materials</subject>
            <subject>Chemical Sciences not elsewhere classified</subject>
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          <dates>
            <date dateType="Created">2023-09-28</date>
            <date dateType="Updated">2023-09-28</date>
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          <publicationYear>2023</publicationYear>
          <publisher>University College London</publisher>
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            <description descriptionType="Abstract"><![CDATA[<p>.xlsx spreadsheets with ascii data recorded during reduction and reaction.</p>
<p><br></p>
<p> X-ray absorption spectroscopy was performed at Diamond Light Source, UK, at B18, through proposal SP30647 (August 2022) for the Pd/Al2O3, Pd/TiO2 and Pd/In2O3/Al2O3 species. Data was collected at the Pd and In K-edges in transmission mode using a QEXAFS setup with fast scanning Si(311) crystal monochromators. The time resolution here was roughly 90 seconds per spectrum. Samples were packed into an in-house custom-made capillary system designed and constructed by Diamond Light Source. 50 mg of 200-300 μm catalyst particles were packed between 3 cm of quartz wool.<br>
<br>
</p>
<p>DRIFTS measurements were performed on a Bruker VERTEX 80 system, with a custom-built high-pressure dome, capable of holding 25 bar of pressure within a high pressure chamber DiffusIRTM PIKE Technologies accessory. Argon and a 25% CO2/75% H2 mixture gas were delivered through high pressure EL-FLOW® Bronkhorst mass-flow controllers, into an in-house custom-made gas manifold. 30 mg of sample was used for the measurements. Initially, the sample was reduced in 25 mL/min of 25% H2 and 75 % Ar. The system was heated to 300 °C at a ramp rate of 5 °C/min and held for 1 hour. The samples were then cooled to 30 °C and either pressurised to 20 bar with 30 mL/min of 75% H2 and 25 % CO2 for the 20 bar measurements or kept at atmospheric pressure for the 1 bar measurements. Once the intended final pressure was reached, the system was heated at 10 °C/min, while holding at 50, 100, 150, 175, 200, 225, 250, 275 and 300 °C for 30 minutes for spectra to be collected. Mass-spectrometry data was collected throughout to observe the evolution of different species, using a Pfeiffer OmniStar.  </p>]]></description>
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