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<dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:invenio="http://invenio-software.org/elements/1.0" 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:identifier>doi:10.1016/j.nima.2025.171176</dc:identifier><dc:language>eng</dc:language><dc:creator>Quintana, A.</dc:creator><dc:creator>Castel, J.</dc:creator><dc:creator>Cebrián, S.</dc:creator><dc:creator>Dafni, T.</dc:creator><dc:creator>Díez-Ibáñez, D.</dc:creator><dc:creator>Ferrer-Ribas, E.</dc:creator><dc:creator>Ezquerro, A.</dc:creator><dc:creator>Galán, J.</dc:creator><dc:creator>García, J.A.</dc:creator><dc:creator>Giganon, A.</dc:creator><dc:creator>Goblin, C.</dc:creator><dc:creator>Goyal, N.</dc:creator><dc:creator>Iguaz, F.J.</dc:creator><dc:creator>García Irastorza, I.</dc:creator><dc:creator>Loiseau, C.</dc:creator><dc:creator>Luzón, G.</dc:creator><dc:creator>Margalejo, C.</dc:creator><dc:creator>Mirallas, H.</dc:creator><dc:creator>Obis, L.</dc:creator><dc:creator>Papaevangelou, T.</dc:creator><dc:creator>Pérez, O.</dc:creator><dc:creator>Porrón, J.</dc:creator><dc:creator>Jiménez Puyuelo, M.</dc:creator><dc:title>Spatial resolution studies with the BabyIAXO Micromegas prototype</dc:title><dc:identifier>ART-2025-146410</dc:identifier><dc:description>The spatial resolution of the Micromegas prototype developed for the BabyIAXO experiment was evaluated using a low-energy X-ray beam at the SOLEIL synchrotron facility. BabyIAXO, currently under construction, aims to search for hypothetical solar axions. A key component of the experiment is a low-background X-ray detector with high efficiency in the 1–10 keV energy range and stringent background rejection capabilities. Achieving a spatial resolution on the order of, or better than, 1 mm is critical for accurately reconstructing signal shapes and positions, and for effectively discriminating between signal and background events. Therefore, a precise characterization of the detector’s spatial resolution is essential to validate its suitability for the experiment. This study involved scanning the IAXO-D1 Micromegas detector under various beam energies, positions, and drift field configurations to evaluate their influence on spatial resolution. A resolution of approximately 100 µm at 6 keV was achieved, confirming the strong potential of this technology for application in the final BabyIAXO setup.</dc:description><dc:date>2025</dc:date><dc:source>http://zaguan.unizar.es/record/164210</dc:source><dc:doi>10.1016/j.nima.2025.171176</dc:doi><dc:identifier>http://zaguan.unizar.es/record/164210</dc:identifier><dc:identifier>oai:zaguan.unizar.es:164210</dc:identifier><dc:relation>info:eu-repo/grantAgreement/EC/H2020/788781/EU/Towards the detection of the axion with the International Axion Observatory/IAXOplus</dc:relation><dc:relation>This project has received funding from the European Union’s Horizon 2020 research and innovation program under grant agreement No H2020 788781-IAXOplus</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MICINN/PID2022-137268NB-C51</dc:relation><dc:identifier.citation>Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 1083 (2025), 171176 [8 pp.]</dc:identifier.citation><dc:rights>by</dc:rights><dc:rights>https://creativecommons.org/licenses/by/4.0/deed.es</dc:rights><dc:rights>info:eu-repo/semantics/openAccess</dc:rights></dc:dc>

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