Share Email Print
cover

Proceedings Paper • new

Building the HARMONI engineering model
Author(s): T. Foster; J. Capone; A. Earle; A. Hidalgo; I. Lewis; J. Lynn; K. O'Brien; M. Rodrigues; I. Tosh; B. Watkins; F. Clarke; H. Schnetler; M. Tecza; N. Thatte
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper 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.

Paper Details

Date Published: 10 July 2018
PDF: 17 pages
Proc. SPIE 10702, Ground-based and Airborne Instrumentation for Astronomy VII, 10702A9 (10 July 2018); doi: 10.1117/12.2313747
Show Author Affiliations
T. Foster, Univ. of Oxford (United Kingdom)
J. Capone, Univ. of Oxford (United Kingdom)
A. Earle, STFC Rutherford Appleton Lab. (United Kingdom)
A. Hidalgo, Univ. of Oxford (United Kingdom)
I. Lewis, Univ. of Oxford (United Kingdom)
J. Lynn, Univ. of Oxford (United Kingdom)
K. O'Brien, Univ. of Oxford (United Kingdom)
M. Rodrigues, Univ. of Oxford (United Kingdom)
I. Tosh, STFC Rutherford Appleton Lab. (United Kingdom)
B. Watkins, Univ. of Oxford (United Kingdom)
F. Clarke, Univ. of Oxford (United Kingdom)
H. Schnetler, UK Astronomy Technology Ctr. (United Kingdom)
M. Tecza, Univ. of Oxford (United Kingdom)
N. Thatte, Univ. of Oxford (United Kingdom)


Published in SPIE Proceedings Vol. 10702:
Ground-based and Airborne Instrumentation for Astronomy VII
Christopher J. Evans; Luc Simard; Hideki Takami, Editor(s)

© SPIE. Terms of Use
Back to Top