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dc.contributor.authorPinna, E.
dc.contributor.authorEsposito, S.
dc.contributor.authorHinz, P.
dc.contributor.authorAgapito, G.
dc.contributor.authorBonaglia, M.
dc.contributor.authorPuglisi, A.
dc.contributor.authorXompero, M.
dc.contributor.authorRiccardi, A.
dc.contributor.authorBriguglio, R.
dc.contributor.authorArcidiacono, C.
dc.contributor.authorCarbonaro, L.
dc.contributor.authorFini, L.
dc.contributor.authorMontoya, M.
dc.contributor.authorDurney, O.
dc.date.accessioned2017-01-20T18:59:49Z
dc.date.available2017-01-20T18:59:49Z
dc.date.issued2016-07-27
dc.identifier.citationE. Pinna ; S. Esposito ; P. Hinz ; G. Agapito ; M. Bonaglia ; A. Puglisi ; M. Xompero ; A. Riccardi ; R. Briguglio ; C. Arcidiacono ; L. Carbonaro ; L. Fini ; M. Montoya and O. Durney " SOUL: the Single conjugated adaptive Optics Upgrade for LBT ", Proc. SPIE 9909, Adaptive Optics Systems V, 99093V (July 27, 2016); doi:10.1117/12.2234444; http://dx.doi.org/10.1117/12.2234444en
dc.identifier.issn0277-786X
dc.identifier.doi10.1117/12.2234444
dc.identifier.urihttp://hdl.handle.net/10150/622050
dc.description.abstractWe present here SOUL: the Single conjugated adaptive Optics Upgrade for LBT. Soul will upgrade the wavefront sensors replacing the existing CCD detector with an EMCCD camera and the rest of the system in order to enable the closed loop operations at a faster cycle rate and with higher number of slopes. Thanks to reduced noise, higher number of pixel and framerate, we expect a gain (for a given SR) around 1.5-2 magnitudes at all wavelengths in the range 7.5 70% in I-band and 0.6asec seeing) and the sky coverage will be multiplied by a factor 5 at all galactic latitudes. Upgrading the SCAO systems at all the 4 focal stations, SOUL will provide these benefits in 2017 to the LBTI interferometer and in 2018 to the 2 LUCI NIR spectro-imagers. In the same year the SOUL correction will be exploited also by the new generation of LBT instruments: V-SHARK, SHARK-NIR and iLocater.
dc.language.isoenen
dc.publisherSPIE-INT SOC OPTICAL ENGINEERINGen
dc.relation.urlhttp://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.2234444en
dc.rights© 2016 SPIE.en
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectPyramid WFSen
dc.subjectAdaptive Secondaryen
dc.subjectSCAOen
dc.subjecteXAOen
dc.subjectLarge Binocular Telescopeen
dc.titleSOUL: the Single conjugated adaptive Optics Upgrade for LBTen
dc.typeArticleen
dc.contributor.departmentUniv Arizona, Steward Observen
dc.identifier.journalADAPTIVE OPTICS SYSTEMS Ven
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.institutionINAF - Osservatorio Astrofisico di Arcetri (Italy)
dc.contributor.institutionINAF - Osservatorio Astrofisico di Arcetri (Italy)
dc.contributor.institutionUniv. of Arizona (United States)
dc.contributor.institutionINAF - Osservatorio Astrofisico di Arcetri (Italy)
dc.contributor.institutionINAF - Osservatorio Astrofisico di Arcetri (Italy)
dc.contributor.institutionINAF - Osservatorio Astrofisico di Arcetri (Italy)
dc.contributor.institutionINAF - Osservatorio Astrofisico di Arcetri (Italy)
dc.contributor.institutionINAF - Osservatorio Astrofisico di Arcetri (Italy)
dc.contributor.institutionINAF - Osservatorio Astrofisico di Arcetri (Italy)
dc.contributor.institutionINAF – Osservatorio Astronomico di Bologna (Italy)
dc.contributor.institutionINAF - Osservatorio Astrofisico di Arcetri (Italy)
dc.contributor.institutionINAF - Osservatorio Astrofisico di Arcetri (Italy)
dc.contributor.institutionUniv. of Arizona (United States)
dc.contributor.institutionUniv. of Arizona (United States)
refterms.dateFOA2018-08-15T01:43:45Z
html.description.abstractWe present here SOUL: the Single conjugated adaptive Optics Upgrade for LBT. Soul will upgrade the wavefront sensors replacing the existing CCD detector with an EMCCD camera and the rest of the system in order to enable the closed loop operations at a faster cycle rate and with higher number of slopes. Thanks to reduced noise, higher number of pixel and framerate, we expect a gain (for a given SR) around 1.5-2 magnitudes at all wavelengths in the range 7.5 <mR <18. The correction at short wavelength will be greatly improved (SR>70% in I-band and 0.6asec seeing) and the sky coverage will be multiplied by a factor 5 at all galactic latitudes. Upgrading the SCAO systems at all the 4 focal stations, SOUL will provide these benefits in 2017 to the LBTI interferometer and in 2018 to the 2 LUCI NIR spectro-imagers. In the same year the SOUL correction will be exploited also by the new generation of LBT instruments: V-SHARK, SHARK-NIR and iLocater.


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