The mechanical design of SOXS for the NTT

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dc.contributor.authorAliverti, M.
dc.contributor.authorHershko, O.
dc.contributor.authorDiner, O.
dc.contributor.authorBrucalassi, A.
dc.contributor.authorPignata, G.
dc.contributor.authorKuncarayakti, H.
dc.contributor.authorBianco, A.
dc.contributor.authorCampana, S.
dc.contributor.authorClaudi, R.
dc.contributor.authorSchipani, P.
dc.contributor.authorBaruffolo, A.
dc.contributor.authorBen-Ami, S.
dc.contributor.authorBiondi, F.
dc.contributor.authorCapasso, G.
dc.contributor.authorCosentino, R.
dc.contributor.authorD'Alessio, F.
dc.contributor.authorD'Avanzo, P.
dc.contributor.authorMunari, M.
dc.contributor.authorRubin, A.
dc.contributor.authorScuderi, S.
dc.contributor.authorVitali, F.
dc.contributor.authorAchrén, J.
dc.contributor.authorAraiza-Duran, J.A.
dc.contributor.authorArcavi, I.
dc.contributor.authorCappellaro, E.
dc.contributor.authorColapietro, M.
dc.contributor.authorDella Valle, M.
dc.contributor.authorD'Orsi, S.
dc.contributor.authorFantinel, D.
dc.contributor.authorFynbo, J.
dc.contributor.authorGal-Yam, A.
dc.contributor.authorGenoni, M.
dc.contributor.authorHirvonen, M.
dc.contributor.authorKotilainen, J.
dc.contributor.authorKumar, T.
dc.contributor.authorLandoni, M.
dc.contributor.authorLehti, J.
dc.contributor.authorLi Causi, G.
dc.contributor.authorMarafatto, L.
dc.contributor.authorMattila, S.
dc.contributor.authorPariani, G.
dc.contributor.authorRappaport, M.
dc.contributor.authorRicci, D.
dc.contributor.authorRiva, M.
dc.contributor.authorSalasnich, B.
dc.contributor.authorSmartt, S.
dc.contributor.authorTuratto, M.
dc.contributor.authorZanmar Sanchez, R.
dc.date.accessioned2022-09-27T19:16:33Z
dc.date.available2022-09-27T19:16:33Z
dc.date.issued2018-06
dc.descriptionIndexación: Scopuses
dc.description.abstractSOXS (Son of X-shooter) is a wide band, medium resolution spectrograph for the ESO NTT with a first light expected in early 2021. The instrument will be composed by five semi-independent subsystems: a pre-slit Common Path (CP), an Acquisition Camera (AC), a Calibration Unit (CU), the NIR spectrograph, and the UV-VIS spectrograph. In this paper, we present the mechanical design of the subsystems, the kinematic mounts developed to simplify the final integration procedure and the maintenance. The concept of the CP and NIR optomechanical mounts developed for a simple pre- alignment procedure and for the thermal compensation of reflective and refractive elements will be shown. © 2018 SPIE.es
dc.description.sponsorship4D TechnologyAndor Technology, Ltd.Astronomical Consultants and Equipment, Inc.et al.Giant Magellan TelescopeThe Society of Photo-Optical Instrumentation Engineers (SPIE) CODEN PSISDes
dc.description.uri//efaidnbmnnnibpcajpcglclefindmkaj/https://arxiv-org.recursosbiblioteca.unab.cl/ftp/arxiv/papers/1809/1809.01589.pdf
dc.identifier.doi10.1117/12.2313404
dc.identifier.issn0277-786X
dc.identifier.urihttps://repositorio.unab.cl/xmlui/handle/ria/24102
dc.language.isoenes
dc.publisherSPIEes
dc.rights.licenseAtribución 4.0 Internacional (CC BY 4.0)
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/deed.es
dc.subjectalignmentes
dc.subjectintegrationes
dc.subjectmechanical designes
dc.subjectNTTes
dc.subjectSOXSes
dc.titleThe mechanical design of SOXS for the NTTes
dc.typeArtículoes
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Proceedings of SPIE - The International Society for Optical Engineering Volume 107022018 Article number 1070231Ground-based and Airborne Instrumentation for Astronomy VII 2018Austin10 June 2018through 14 June 2018Code 138743
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