<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><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>2026-04-14T16:57:47Z</responseDate><request verb="GetRecord" identifier="oai:uvadoc.uva.es:10324/46258" metadataPrefix="mods">https://uvadoc.uva.es/oai/request</request><GetRecord><record><header><identifier>oai:uvadoc.uva.es:10324/46258</identifier><datestamp>2025-02-11T18:18:34Z</datestamp><setSpec>com_10324_1158</setSpec><setSpec>com_10324_931</setSpec><setSpec>com_10324_894</setSpec><setSpec>col_10324_1242</setSpec></header><metadata><mods:mods xmlns:mods="http://www.loc.gov/mods/v3" xmlns:doc="http://www.lyncode.com/xoai" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.loc.gov/mods/v3 http://www.loc.gov/standards/mods/v3/mods-3-1.xsd">
<mods:name>
<mods:namePart>Veneranda ., Marco</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>López Reyes, Guillermo Eduardo</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Manrique Martínez, José Antonio</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Medina García, Jesús</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Ruiz Galende, Patricia</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Torre Fernández, Imanol</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Castro, Kepa</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Lantz, Cateline</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Poulet, Francois</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Dypvik, Henning</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Werner, Stephanie C.</mods:namePart>
</mods:name>
<mods:name>
<mods:namePart>Rull Pérez, Fernando</mods:namePart>
</mods:name>
<mods:extension>
<mods:dateAvailable encoding="iso8601">2021-04-19T22:59:05Z</mods:dateAvailable>
</mods:extension>
<mods:extension>
<mods:dateAccessioned encoding="iso8601">2021-04-19T22:59:05Z</mods:dateAccessioned>
</mods:extension>
<mods:originInfo>
<mods:dateIssued encoding="iso8601">2020</mods:dateIssued>
</mods:originInfo>
<mods:identifier type="citation">Astrobiology, 2020, Vol. 20, n. 3, p. 349-363</mods:identifier>
<mods:identifier type="issn">1531-1074</mods:identifier>
<mods:identifier type="uri">http://uvadoc.uva.es/handle/10324/46258</mods:identifier>
<mods:identifier type="doi">10.1089/ast.2019.2095</mods:identifier>
<mods:identifier type="publicationfirstpage">349</mods:identifier>
<mods:identifier type="publicationissue">3</mods:identifier>
<mods:identifier type="publicationlastpage">363</mods:identifier>
<mods:identifier type="publicationtitle">Astrobiology</mods:identifier>
<mods:identifier type="publicationvolume">20</mods:identifier>
<mods:identifier type="essn">1557-8070</mods:identifier>
<mods:abstract>In the present work, NIR, LIBS, Raman and XRD techniques have been complementarily used to &#xd;
carry out a comprehensive characterization of a terrestrial analogue selected from the &#xd;
Chesapeake Bay Impact Structure (CBIS). The obtained data clearly highlight the key role of&#xd;
Raman spectroscopy in the detection of minor and trace compounds, through which inferences &#xd;
about geological processes occurred in the CBIS can be extrapolated. Beside the use of &#xd;
commercial systems, further Raman analyses were performed by the Raman Laser Spectrometer &#xd;
(RLS) ExoMars Simulator. This instrument representsthe most reliable tool to effectively predict &#xd;
the scientific capabilities of the ExoMars/Raman system that will be deployed on Mars in 2021.&#xd;
By emulating the analytical procedures and operational restrictions established by the ExoMars&#xd;
mission rover design, it was proved that the RLS ExoMars Simulator is able to detect the &#xd;
amorphization of quartz, which constitutes an analytical clue of the impact origin of craters. On &#xd;
the other hand, the detection of barite and siderite, compounds crystallizing under &#xd;
hydrothermal conditions, helps to indirectly confirm the presence of water in impact targets. &#xd;
Furthermore, the RLS ExoMars Simulator capability of performing smart molecular mappings&#xd;
was also evaluated. According to the obtained results, the algorithms developed for its &#xd;
operation provide a great analytical advantage over most of the automatic analysis systems &#xd;
employed by commercial Raman instruments, encouraging its application for many additional &#xd;
scientific and commercial purposes.</mods:abstract>
<mods:language>
<mods:languageTerm>eng</mods:languageTerm>
</mods:language>
<mods:accessCondition type="useAndReproduction">info:eu-repo/semantics/openAccess</mods:accessCondition>
<mods:titleInfo>
<mods:title>ExoMars Raman Laser Spectrometer: A Tool for the Potential Recognition of Wet-Target Craters on Mars</mods:title>
</mods:titleInfo>
<mods:genre>info:eu-repo/semantics/article</mods:genre>
</mods:mods></metadata></record></GetRecord></OAI-PMH>