A. Jeanneau, J. Kosmalski, E. Muslimov, E. Hugot, R. Bacon, J. Richard
{"title":"Curved detector-based optical design for the VLT/BlueMUSE instrument","authors":"A. Jeanneau, J. Kosmalski, E. Muslimov, E. Hugot, R. Bacon, J. Richard","doi":"10.1117/12.2561684","DOIUrl":null,"url":null,"abstract":"BlueMUSE (Blue Multi Unit Spectroscopic Explorer) is a blue-optimised, medium spectral resolution, panoramic integral field spectrograph proposed for the Very Large Telescope (VLT) and based on the MUSE concept. BlueMUSE will open up a new range of galactic and extragalactic science cases allowed by its specific capabilities in the 350 - 580 nm range: an optimised end-to-end transmission down to 350 nm, a larger FoV (up to 1.4 x 1.4 arcmin²) sampled at 0.3 arcsec, and a higher spectral resolution (λ/Δλ ~ 3500) compared to MUSE. To our knowledge, achieving such capabilities with a comparable mechanical footprint and an identical detector format (4k x 4k, 15 µm CCD) would not be possible with a conventional spectrograph design. \n\nIn this paper, we present the optomechanical architecture and design of BlueMUSE at pre-phase A level, with a particular attention to some original aspects such as the use of curved detectors.","PeriodicalId":215000,"journal":{"name":"Ground-based and Airborne Instrumentation for Astronomy VIII","volume":"6 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-12-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Ground-based and Airborne Instrumentation for Astronomy VIII","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2561684","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
BlueMUSE (Blue Multi Unit Spectroscopic Explorer) is a blue-optimised, medium spectral resolution, panoramic integral field spectrograph proposed for the Very Large Telescope (VLT) and based on the MUSE concept. BlueMUSE will open up a new range of galactic and extragalactic science cases allowed by its specific capabilities in the 350 - 580 nm range: an optimised end-to-end transmission down to 350 nm, a larger FoV (up to 1.4 x 1.4 arcmin²) sampled at 0.3 arcsec, and a higher spectral resolution (λ/Δλ ~ 3500) compared to MUSE. To our knowledge, achieving such capabilities with a comparable mechanical footprint and an identical detector format (4k x 4k, 15 µm CCD) would not be possible with a conventional spectrograph design.
In this paper, we present the optomechanical architecture and design of BlueMUSE at pre-phase A level, with a particular attention to some original aspects such as the use of curved detectors.