Conference item
Building the HARMONI engineering model
- Abstract:
- HARMONI (High Angular Resolution MOnolithic Integral field spectrograph)1 is a planned first-light integral field spectrograph for the Extremely Large Telescope. The spectrograph sub-system is being designed, developed, and built by the University of Oxford. The project has just completed the Preliminary Design Review (PDR), with all major systems having nearly reached a final conceptual design. As part of the overall prototyping and assembly, integration, and testing (AIT) of the HARMONI spectrograph, we will be building a full-scale engineering model of the spectrograph. This will include all of the moving and mechanical systems, but without optics. Its main purpose is to confirm the AIT tasks before the availability of the optics, and the system will be tested at HARMONI cryogenic temperatures. By the time of the construction of the engineering model, all of the individual modules and mechanisms of the spectrograph will have been prototyped and cryogenically tested. The lessons learned from the engineering model will then be fed back into the overall design of the spectrograph modules ahead of their development.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
Actions
Access Document
- Files:
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(Preview, Accepted manuscript, pdf, 1.2MB, Terms of use)
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- Publisher copy:
- 10.1117/12.2313747
Authors
- Publisher:
- Society of Photo-optical Instrumentation Engineers
- Host title:
- Proceedings of SPIE
- Journal:
- Proceedings of SPIE More from this journal
- Volume:
- 10702
- Publication date:
- 2018-07-10
- DOI:
- EISSN:
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1996-756X
- ISSN:
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0277-786X
- ISBN:
- 9781510619579
- Keywords:
- Pubs id:
-
pubs:919116
- UUID:
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uuid:acb5e3b1-ab73-4f3d-921d-ad328664b74a
- Local pid:
-
pubs:919116
- Source identifiers:
-
919116
- Deposit date:
-
2019-07-01
Terms of use
- Copyright holder:
- Society of Photo-optical Instrumentation Engineers
- Copyright date:
- 2018
- Notes:
- © SPIE 2018. This paper was presented at Groube-based and Airborne Instrumentation for Astronomy VII, Austin, Texas, USA, June 2018. This is the accepted manuscript version of the paper. The final version is available online from the Society of Photo-optical Instrumentation Engineers at: http://doi.org/10.1117/12.2313747
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