LEADER 03591nam 22005895 450 001 9910254640103321 005 20200704100410.0 010 $a3-319-29400-8 024 7 $a10.1007/978-3-319-29400-1 035 $a(CKB)3710000000685972 035 $a(EBL)4530821 035 $a(DE-He213)978-3-319-29400-1 035 $a(MiAaPQ)EBC4530821 035 $a(PPN)194074153 035 $a(EXLCZ)993710000000685972 100 $a20160521d2016 u| 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 12$aA Far-Infrared Spectro-Spatial Space Interferometer $eInstrument Simulator and Testbed Implementation /$fby Roser Juanola-Parramon 205 $a1st ed. 2016. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2016. 215 $a1 online resource (166 p.) 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 300 $aDescription based upon print version of record. 311 $a3-319-29399-0 320 $aIncludes bibliographical references at the end of each chapters and index. 327 $aIntroduction -- Theoretical background -- Spectro-Spatial Interferometry Testbeds -- FIInS -- FIInS Data Processing and Verification -- Simulated Observations with FIInS -- Conclusions and Future Work. 330 $aThis thesis describes the physics and computational aspects of an end-to-end simulator to predict the performance of a Space-based Far Infrared Interferometer. The present thesis also includes, the science capabilities and instrumental state-of-the art. The latter is the ambitious next step which the Far-Infrared Astrophysical community needs to take to improve in anyway on the results of the most recent and current space telescopes in this wavelength region. This thesis outlines the requirements involved in such a mission and describes the most promising technique to capture most of the astrophysical information by combining spectroscopy to spatial interferometer. The simulation of such a system is extremely complex requiring multiple Fourier transforms each of which is subject to instrument non-idealities and appropriate optimization techniques. As a conclusion, the thesis provides an example of the basic performance achievable with such an instrument when targeting a young star formation region. 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aAstronomy$vObservations 606 $aAstronomy?Observations 606 $aEngineering design 606 $aComputer-aided engineering 606 $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014 606 $aEngineering Design$3https://scigraph.springernature.com/ontologies/product-market-codes/T17020 606 $aComputer-Aided Engineering (CAD, CAE) and Design$3https://scigraph.springernature.com/ontologies/product-market-codes/I23044 615 0$aAstronomy 615 0$aAstronomy?Observations. 615 0$aEngineering design. 615 0$aComputer-aided engineering. 615 14$aAstronomy, Observations and Techniques. 615 24$aEngineering Design. 615 24$aComputer-Aided Engineering (CAD, CAE) and Design. 676 $a530 700 $aJuanola-Parramon$b Roser$4aut$4http://id.loc.gov/vocabulary/relators/aut$0799812 906 $aBOOK 912 $a9910254640103321 996 $aA Far-Infrared Spectro-Spatial Space Interferometer$92523468 997 $aUNINA