<?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>2026-06-27T16:06:57Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/8932" metadataPrefix="qdc">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/8932</identifier><datestamp>2024-07-11T16:23:03Z</datestamp><setSpec>com_20.500.14352_14</setSpec><setSpec>col_20.500.14352_20</setSpec></header><metadata><qdc:qualifieddc xmlns:qdc="http://dspace.org/qualifieddc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://purl.org/dc/elements/1.1/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dc.xsd http://purl.org/dc/terms/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dcterms.xsd http://dspace.org/qualifieddc/ http://www.ukoln.ac.uk/metadata/dcmi/xmlschema/qualifieddc.xsd">
   <dc:title>Field camera unit of the WSO-UV mission</dc:title>
   <dc:creator>Sachkov, Mikhail</dc:creator>
   <dc:creator>Sichevsky, Sergey</dc:creator>
   <dc:creator>Shustov, Boris</dc:creator>
   <dc:creator>Shugarov, Andrey</dc:creator>
   <dc:creator>Shmagin, Vladimir</dc:creator>
   <dc:creator>Iosipenko, Sergey</dc:creator>
   <dc:creator>Arkhangelsky, Roman</dc:creator>
   <dc:creator>Kanev, Evgeny</dc:creator>
   <dc:creator>Gómez De Castro, Ana Inés</dc:creator>
   <dc:creator>Vallejo, Juan Carlos</dc:creator>
   <dcterms:abstract>The main instrument of the space mission "Spectr-UF" (World Space Observatory-Ultraviolet) is a large space telescope to work in the UV wavelength domain (115 - 310 nm). The WSO-UV telescope feeds in its focal plane two main instruments: unit of spectrographs WUVS, and field camera unit FCU, as well as Fine Guidance System (FGS). The imaging instrument FCU onboard WSO-UV will be the first UV camera to be flown to a geosynchronous orbit. Here we provide a brief description on updated FCU instrument and its current status.</dcterms:abstract>
   <dcterms:dateAccepted>2023-06-17T10:14:11Z</dcterms:dateAccepted>
   <dcterms:available>2023-06-17T10:14:11Z</dcterms:available>
   <dcterms:created>2023-06-17T10:14:11Z</dcterms:created>
   <dcterms:issued>2020</dcterms:issued>
   <dc:type>conference paper</dc:type>
   <dc:identifier>https://hdl.handle.net/20.500.14352/8932</dc:identifier>
   <dc:identifier>XXXX-XXXX</dc:identifier>
   <dc:identifier>10.1117/12.2562962</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:relation>M. Sachkov, S. Sichevsky, B. Shustov, A. Shugarov, V. Shmagin, S. Iosipenko, R. Arkhangelsky, E. Kanev, A. I. Gomez de Castro, J. C. Vallejo, "Field camera unit of the WSO-UV mission," Proc. SPIE 11444, Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray, 1144474 (13 December 2020); doi: 10.1117/12.2562962</dc:relation>
   <dc:rights>https://creativecommons.org/licenses/by/3.0/es/</dc:rights>
   <dc:rights>open access</dc:rights>
   <dc:rights>Atribución 3.0 España</dc:rights>
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