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Subaru Laser Guide Star System Upgrade and On-sky Characterization

dc.contributor.authorMinowa, Yosukeen
dc.contributor.authorOno, Yoshitoen
dc.contributor.authorDoi, Yoshiyukien
dc.contributor.authorTanaka, Yokoen
dc.contributor.authorBando, Takamasaen
dc.contributor.authorYoshida, Hiroshigeen
dc.contributor.authorTerao, Kokien
dc.contributor.authorOkita, Hirofumien
dc.contributor.authorWung, Matthewen
dc.contributor.authorRamos, Lucioen
dc.contributor.authorOgane, Hajimeen
dc.contributor.authorOjika, Akimasaen
dc.contributor.authorAkiyama, Masayukien
dc.date.accessioned2025-05-23T15:23:09Z
dc.date.available2025-05-23T15:23:09Z
dc.date.issued2024en
dc.description.abstractThe Subaru laser guide star system has been upgraded by implementing the TOPTICA/MPBC guide-star laser and a new mirror-based laser relay system. The upgrade is to replace the aged laser and its transfer system and provide the improved performance for stable science operation. The increased laser return photon can also bring a new capability of generating multiple laser guide stars (LGSs) by splitting the laser beam. The new laser guide star system was installed on the Subaru telescope in December 2021 and commissioning observations were conducted in 2022. The LGSAO mode with the new laser guide star system has been offered for science open use program since 2023. The new laser guide star system provides more stable LGS than the previous system with respect to the laser power and pointing. The LGS spot size is ∼1.0 arcsec in FWHM under median seeing condition. The LGS photon return is more than 10 times brighter than the previous system. By utilizing the increased brightness, further upgrade of the Laser Launching Telescope (LLT) is being implemented to generate the asterism of four LGSs with the diameter variable between 10 and 40 arcsec for the new Laser Tomography Adaptive Optics (LTAO) system.en
dc.description.sponsorshipWe would like to thank all the staff at Subaru Telescope for their support, which made the upgrade of the laser guide star system realized. We are especially grateful to Dr. Yutaka Hayano for his advice in designing the new laser guide star system, to Dr. Etsuko Mieda for initial experiments to validate the selected design, to Ms. Morris Marita for her contribution in optical assembly and tolerance analysis, to Mr. Michael Lemmen for assembling the cooling system, and to Dr. Yuhei Takagi for his support in commissioning the new laser guide star system. This work is partly supported by the the Japanese Ministry of Education, Culture, Sports, Science and Technology (MEXT) as a prototype activity for the Gruond Layer Adaptive Optics (GLAO) system for the ULTIMATE-Subaru project. This work is also supported by JSPS Grant-in-Aid for Scientific Research (KAKENHI) grant number JP17H06129.en
dc.description.statusPeer-revieweden
dc.identifier.isbn9781510675179en
dc.identifier.issn0277-786Xen
dc.identifier.otherORCID:/0000-0002-7760-7703/work/184104122en
dc.identifier.scopus85205567836en
dc.identifier.urihttp://www.scopus.com/inward/record.url?scp=85205567836&partnerID=8YFLogxKen
dc.identifier.urihttps://hdl.handle.net/1885/733752545
dc.language.isoenen
dc.publisherSPIEen
dc.relation.ispartofAdaptive Optics Systems IXen
dc.relation.ispartofseriesAdaptive Optics Systems IX 2024en
dc.relation.ispartofseriesProceedings of SPIE - The International Society for Optical Engineeringen
dc.rightsPublisher Copyright: © 2024 SPIE.en
dc.subjectadaptive opticsen
dc.subjectlaser guide staren
dc.subjectlaser tomographyen
dc.titleSubaru Laser Guide Star System Upgrade and On-sky Characterizationen
dc.typeConference paperen
dspace.entity.typePublicationen
local.contributor.affiliationMinowa, Yosuke; National Institutes of Natural Sciences - National Astronomical Observatory of Japanen
local.contributor.affiliationOno, Yoshito; National Institutes of Natural Sciences - National Astronomical Observatory of Japanen
local.contributor.affiliationDoi, Yoshiyuki; National Institutes of Natural Sciences - National Astronomical Observatory of Japanen
local.contributor.affiliationTanaka, Yoko; National Institutes of Natural Sciences - National Astronomical Observatory of Japanen
local.contributor.affiliationBando, Takamasa; National Institutes of Natural Sciences - National Astronomical Observatory of Japanen
local.contributor.affiliationYoshida, Hiroshige; National Institutes of Natural Sciences - National Astronomical Observatory of Japanen
local.contributor.affiliationTerao, Koki; National Institutes of Natural Sciences - National Astronomical Observatory of Japanen
local.contributor.affiliationOkita, Hirofumi; National Institutes of Natural Sciences - National Astronomical Observatory of Japanen
local.contributor.affiliationWung, Matthew; National Institutes of Natural Sciences - National Astronomical Observatory of Japanen
local.contributor.affiliationRamos, Lucio; National Institutes of Natural Sciences - National Astronomical Observatory of Japanen
local.contributor.affiliationOgane, Hajime; Advanced Instrumentation and Technology Centre, Research School of Astronomy & Astrophysics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationOjika, Akimasa; Kwansei Gakuin Universityen
local.contributor.affiliationAkiyama, Masayuki; Tohoku Universityen
local.identifier.doi10.1117/12.3018789en
local.identifier.essn1996-756Xen
local.identifier.pure4bf9fdaa-cdec-4af4-b229-76a2c06bd2b9en
local.identifier.urlhttps://www.scopus.com/pages/publications/85205567836en
local.type.statusPublisheden

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