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The imaging and slitless spectroscopy instrument for surveys (ISSIS) for the world space observatory-ultraviolet (WSO-UV)

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dc.contributor.authorGómez De Castro, Ana Inés
dc.contributor.authorMaíz, Jesús
dc.contributor.authorRodríguez, Pablo
dc.contributor.authorGómez, Maite
dc.contributor.authorLarruquert, Juan A.
dc.contributor.authorMéndez, José A.
dc.contributor.authorBelenguer, Tomás
dc.contributor.authorRodrigo Gudiel, Víctor
dc.contributor.authorLópez Martinez, Fátima
dc.contributor.authorSestito, Paola
dc.date.accessioned2023-06-20T00:13:33Z
dc.date.available2023-06-20T00:13:33Z
dc.date.issued2011-09
dc.description.abstractISSIS is the Imaging and Slitless Spectroscopy Instrument for the World Space Observatory-Ultraviolet (WSO-UV) mission. ISSIS is a multipurpose instrument designed to carry out high resolution (< 0.1 arcsec) imaging in the far UV with fields of view a parts per thousand yen2x2 arcmin(2). ISSIS has two acquisition channels: the High Sensitivity Channel (HSC) and the Channel for Surveys (CfS). The HSC is equipped with an MCP-type detector to guarantee high sensitivity in the 1150-1750 range and high rejection of lower energy radiation. The CfS is equipped with a large CCD detector (4kx4k) to obtain images from the far UV to the red (1150-8500 ); the CfS is implemented to allow observing UV bright sources such as reflection nebulae or nearby massive star forming regions. The design drivers and the current status of the instrument are described in this contribution.en
dc.description.departmentUnidad Deptal. de Astronomía y Geodesia
dc.description.facultyFac. de Ciencias Matemáticas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Ciencia, Innovación y Universidades (España)
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/15857
dc.identifier.citationGómez de Castro, A.I., Maíz, J., Rodríguez, P. et al. «The Imaging and Slitless Spectroscopy Instrument for Surveys (ISSIS) for the World Space Observatory-Ultraviolet (WSO-UV)». Astrophysics and Space Science, vol. 335, n.o 1, septiembre de 2011, pp. 283-89. DOI.org (Crossref), https://doi.org/10.1007/s10509-011-0695-9.
dc.identifier.doi10.1007/s10509-011-0695-9
dc.identifier.issn0004-640X
dc.identifier.officialurlhttps//doi.org/10.1007/s10509-011-0695-9
dc.identifier.relatedurlhttp://www.springerlink.com/content/52174kx318718834/fulltext.pdf
dc.identifier.urihttps://hdl.handle.net/20.500.14352/42228
dc.issue.number1
dc.journal.titleAstrophysics and space science
dc.language.isoeng
dc.page.final289
dc.page.initial283
dc.publisherSpringer
dc.relation.projectIDAYA2008-06423-C03-01/ESP
dc.rights.accessRightsrestricted access
dc.subject.cdu52
dc.subject.keywordSpace astronomy
dc.subject.keywordInstrumentation
dc.subject.keywordUltraviolet astronomy
dc.subject.ucmAstronomía (Matemáticas)
dc.subject.unesco21 Astronomía y Astrofísica
dc.titleThe imaging and slitless spectroscopy instrument for surveys (ISSIS) for the world space observatory-ultraviolet (WSO-UV)en
dc.typejournal article
dc.volume.number335
dspace.entity.typePublication
relation.isAuthorOfPublication492947a5-78aa-4c19-bb69-3dd332bff97c
relation.isAuthorOfPublication.latestForDiscovery492947a5-78aa-4c19-bb69-3dd332bff97c

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