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WUVS simulator: detectability of spectral lines with the WSO-UV spectrographs

dc.contributor.authorMarcos-Arenal, P.
dc.contributor.authorGómez De Castro, Ana Inés
dc.contributor.authorAbarca, B. P.
dc.contributor.authorSachkov, Mikhail
dc.date.accessioned2023-06-17T22:07:56Z
dc.date.available2023-06-17T22:07:56Z
dc.date.issued2017
dc.description.abstractThe World Space Observatory Ultraviolet telescope is equipped with high dispersion (55,000) spectrographs working in the 1150 to 3100 angstrom spectral range. To evaluate the impact of the design on the scientific objectives of the mission, a simulation software tool has been developed. This simulator builds on the development made for the PLATO space mission and it is designed to generate synthetic time-series of images by including models of all important noise sources. We describe its design and performance. Moreover, its application to the detectability of important spectral features for star formation and exoplanetary research is addressed.
dc.description.departmentUnidad Deptal. de Astronomía y Geodesia
dc.description.facultyFac. de Ciencias Matemáticas
dc.description.refereedTRUE
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/44797
dc.identifier.doi10.1117/1.JATIS.3.2.025002
dc.identifier.issn2329-4124
dc.identifier.officialurlhttps://goo.gl/JDFp9P
dc.identifier.relatedurlhttps://www.spiedigitallibrary.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/18109
dc.issue.number2
dc.journal.titleJournal of Astronomical Telescopes, Instruments, and Systems
dc.language.isoeng
dc.page.final1
dc.page.initial025002
dc.publisherSociety of Photo-optical Instrumentation Engineers (SPIE)
dc.rights.accessRightsrestricted access
dc.subject.cdu510.6
dc.subject.keywordSpace missions
dc.subject.keywordUltraviolet detector
dc.subject.keywordUltraviolet spectrograph
dc.subject.keywordSimulations
dc.subject.keywordCCD
dc.subject.ucmLógica simbólica y matemática (Matemáticas)
dc.subject.unesco1102.14 Lógica Simbólica
dc.titleWUVS simulator: detectability of spectral lines with the WSO-UV spectrographs
dc.typejournal article
dc.volume.number3
dspace.entity.typePublication
relation.isAuthorOfPublication492947a5-78aa-4c19-bb69-3dd332bff97c
relation.isAuthorOfPublication.latestForDiscovery492947a5-78aa-4c19-bb69-3dd332bff97c

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