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SOXS System engineering from design to installation: Challenges and results

  • Riccardo Claudi*
  • , Kalyan Radhakrishnan
  • , Federico Battaini
  • , Simone Di Filippo
  • , Lorenzo Cabona
  • , Sergio Campana
  • , Pietro Schipani
  • , Matteo Aliverti
  • , Josè Antonio Araiza-Duran
  • , Laura Asquini
  • , Andrea Baruffolo
  • , Sagi Ben-Ami
  • , Anna Brucalassi
  • , Rachel Bruch
  • , Giulio Capasso
  • , Mirko Colapietro
  • , Rosario Cosentino
  • , Francesco D'Alessio
  • , Paolo D'Avanzo
  • , Sergio D'Orsi
  • Matteo Genoni, Ofir Hershko, Hanindyo Kuncarayakti, Marco Landoni, Gianluca Li Causi, Luca Marafatto, Eugenio Martinetti, Antonio Miccichè, Matteo Munari, Gaetano Nicotra, Giuliano Pignata, Michael Rappaport, Davide Ricci, Adam Rubin, Bernardo Salasnich, Salvo Scuderi, Stephen Smartt, Fabrizio Vitali, David Young, Ricardo Zanmar Sanchez, Jani Achrén, Iair Arcavi, Enrico Cappellaro, Massimo Della Valle, Avishay Gal-Yam, Seppo Matila, Marco Riva
*Corresponding author for this work
  • Astronomical Observatory of Padua
  • Osservatorio Astronomico di Brera
  • Osservatorio Astronomico di Capodimonte
  • National Institute for Astrophysics
  • Weizmann Institute of Science
  • TNG
  • Osservatorio Astrofisico di Catania
  • Osservatorio Astronomico Roma
  • University of Turku
  • Universidad de Tarapacá
  • European Southern Observatory
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • Queen's University Belfast
  • Incident Angle Oy

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

4 Scopus citations

Abstract

SOXS (SOn of X-Shooter) is a high-efficiency spectrograph with a mean Resolution-Slit product of about 3500 over the entire band capable of simultaneously observing the complete spectral range 350-2000 nm. It consists of three scientific arms (the UV-VIS Spectrograph, the NIR Spectrograph, and the Acquisition Camera) connected by the Common Path system to the NTT, and the Calibration Unit. During the last year, we performed the instrument AIV at the integration site in Europe. It is still ongoing. We present an overview of the flow for validation of the scientific and technical requirements, after integration of the sub-systems with some results as highlights. Further, we give an overview of the methodologies used for planning and managing the assembly of the sub-systems, their integration, and tests before the acceptance of the instrument in Europe (PAE). SOXS could be used as an example for the system engineering of an instrument of moderate complexity, with a large geographic spread of the team.

Original languageEnglish
Title of host publicationModeling, Systems Engineering, and Project Management for Astronomy XI
EditorsSebastien E. Egner, Scott Roberts
PublisherSPIE
ISBN (Electronic)9781510675216
DOIs
StatePublished - 2024
EventModeling, Systems Engineering, and Project Management for Astronomy XI 2024 - Yokohama, Japan
Duration: 16 Jun 202418 Jun 2024

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume13099
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceModeling, Systems Engineering, and Project Management for Astronomy XI 2024
Country/TerritoryJapan
CityYokohama
Period16/06/2418/06/24

Funding

FundersFunder number
Science and Technology Facilities CouncilST/T000198/1

    Keywords

    • Astronomical Instrumentation
    • NIR
    • Spectrograph
    • Transients
    • VIS

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