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dc.contributor.authorSablowski, D. P.
dc.contributor.authorWeber, M.
dc.contributor.authorWoche, M.
dc.contributor.authorIlyin, I.
dc.contributor.authorJärvinen, A.
dc.contributor.authorStrassmeier, K. G.
dc.contributor.authorGabor, P.
dc.date.accessioned2017-02-04T00:26:15Z
dc.date.available2017-02-04T00:26:15Z
dc.date.issued2016-07-22
dc.identifier.citationD. P. Sablowski ; M. Weber ; M. Woche ; I. Ilyin ; A. Järvinen ; K. G. Strassmeier and P. Gabor " PEPSI-feed: linking PEPSI to the Vatican Advanced Technology Telescope using a 450m long fibre ", Proc. SPIE 9912, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II, 99125H (July 22, 2016); doi:10.1117/12.2231874; http://dx.doi.org/10.1117/12.2231874en
dc.identifier.issn0277-786X
dc.identifier.doi10.1117/12.2231874
dc.identifier.urihttp://hdl.handle.net/10150/622429
dc.description.abstractLimited observing time at large telescopes equipped with the most powerful spectrographs makes it almost impossible to gain long and well-sampled time-series observations. Ditto, high-time-resolution observations of bright targets with high signal-to-noise are rare. By pulling an optical fibre of 450m length from the Vatican Advanced Technology Telescope (VATT) to the Large Binocular Telescope (LBT) to connect the Potsdam Echelle Polarimetric and Spectroscopic Instrument (PEPSI) to the VATT, allows for ultra-high resolution time-series measurements of bright targets. This article presents the fibre-link in detail from the technical point-of-view, demonstrates its performance from first observations, and sketches current applications.
dc.language.isoenen
dc.publisherSPIE-INT SOC OPTICAL ENGINEERINGen
dc.relation.urlhttp://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.2231874en
dc.rights© 2016 SPIE.en
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjecthigh-res spectroscopyen
dc.subjectfibre opticsen
dc.subjectfibre-feeden
dc.subjectPEPSIen
dc.titlePEPSI-feed: linking PEPSI to the Vatican Advanced Technology Telescope using a 450m long fibreen
dc.typeArticleen
dc.contributor.departmentUniv Arizona, Vatican Observen
dc.identifier.journalADVANCES IN OPTICAL AND MECHANICAL TECHNOLOGIES FOR TELESCOPES AND INSTRUMENTATION IIen
dc.description.noteSPIE grants to authors of papers published in an SPIE Journal or Proceedings the right to post an author-prepared version or an official version (preferred version) of the published paper on an internal or external server controlled exclusively by the author/employer, provided that (a) such posting is noncommercial in nature and the paper is made available to users without charge; (b) an appropriate copyright notice and full citation appear with the paper, and (c) a link to SPIE's official online version of the abstract is provided using the DOI (Document Object Identifier) link.en
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en
dc.eprint.versionFinal published versionen
dc.contributor.institutionLeibniz-Institute for Astrophysics Potsdam (Germany)
dc.contributor.institutionLeibniz-Institute for Astrophysics Potsdam (Germany)
dc.contributor.institutionLeibniz-Institute for Astrophysics Potsdam (Germany)
dc.contributor.institutionLeibniz-Institute for Astrophysics Potsdam (Germany)
dc.contributor.institutionLeibniz-Institute for Astrophysics Potsdam (Germany)
dc.contributor.institutionLeibniz-Institute for Astrophysics Potsdam (Germany)
dc.contributor.institutionVatican Observatory, The Univ. of Arizona (United States)
refterms.dateFOA2018-06-16T10:00:37Z
html.description.abstractLimited observing time at large telescopes equipped with the most powerful spectrographs makes it almost impossible to gain long and well-sampled time-series observations. Ditto, high-time-resolution observations of bright targets with high signal-to-noise are rare. By pulling an optical fibre of 450m length from the Vatican Advanced Technology Telescope (VATT) to the Large Binocular Telescope (LBT) to connect the Potsdam Echelle Polarimetric and Spectroscopic Instrument (PEPSI) to the VATT, allows for ultra-high resolution time-series measurements of bright targets. This article presents the fibre-link in detail from the technical point-of-view, demonstrates its performance from first observations, and sketches current applications.


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