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dc.rights.license© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE)-
dc.contributor.authorShipman, R. F.-
dc.contributor.authorVandenbussche, B.-
dc.contributor.authorCastillo Domínguez, E.-
dc.contributor.authorLabiano, Á.-
dc.contributor.authorJellema, W.-
dc.contributor.authorOrlando, A.-
dc.contributor.otherinfo:eu-repo/semantics/restrictedAccess-
dc.date.accessioned2022-02-15T14:12:53Z-
dc.date.available2022-02-15T14:12:53Z-
dc.date.issued2020-12-13-
dc.identifier.citationProceedings of Space Telescopes and Instrumentation, Optical, Infrared and Millimeter 11443: 114436L (2020)es
dc.identifier.issn0277-786X-
dc.identifier.otherhttps://www.spiedigitallibrary.org/conference-proceedings-of-spie/11443/2562071/The-calibration-strategy-for-the-SPICASAFARI-instrument/10.1117/12.2562071.short-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/574-
dc.description.abstractSPICA is a mid to far infra-red space mission to explore the processes that form galaxies, stars and planets. SPICA/SAFARI is the far infrared spectrometer that provides near-background limited observations between 34 and 230 micrometers. The core of SAFARI consists of 4 grating modules, dispersing light onto 5 arrays of TES detectors per module. The grating modules provide low resolution (250) instantaneous spectra over the entire wavelength range. The high resolution (1500 to 12000) mode is accomplished by placing a Fourier Transform Spectrometer (FTS) in front of the gratings. Each grating module detector sees an interferogram from which the high resolution spectrum can be constructed. SAFARI data will be a convolution of complex spectral, temporal and spatial information. Along with spectral calibration accuracy of < 1 %, a relative flux calibration of 1% and an absolute flux calibration accuracy of 10% are required. This paper will discuss the calibration strategy and its impact on the instrument design of SAFARIes
dc.description.sponsorshipR.S. thanks David Naylor for many useful discussions and his insight to the needs of an FTS. A.L. acknowledges the support from Comunidad de Madrid through the Atraccion de Talento grant 2017-T1/TIC-5213. This research has been partially funded by the Spanish State Research Agency (AEI) Project MDM-2017-0737 Unidad de Excelencia Maria de Maeztu-Centro de Astrobiologia (INTA-CSIC).es
dc.language.isoenges
dc.publisherSPIE Digital Libraryes
dc.titleCalibration strategy for the SPICA/SAFARI instrumentes
dc.typeinfo:eu-repo/semantics/conferenceObjectes
dc.contributor.orcidAngiola, O. [0000-0001-9464-3100]-
dc.identifier.doi10.1117/12.2562071-
dc.identifier.e-issn1996-756X-
dc.contributor.funderComunidad de Madrid-
dc.description.peerreviewedPeerreviewes
dc.identifier.funderhttp://dx.doi.org/10.13039/100012818-
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/restrictedAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_6670-
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