WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope
We present the preliminary design of the WEAVE next generation spectroscopy facility for the William Herschel Telescope (WHT), principally targeting optical ground-based follow up of upcoming ground-based (LOFAR) and space-based (Gaia) surveys. WEAVE is a multi-object and multi-IFU facility utilizin...
Prif Awduron: | Dalton, G, Trager, S, Abrams, D, Carter, D, Bonifacio, P, Aguerri, J, MacIntosh, M, Evans, C, Lewis, I, Navarro, R, Agocs, T, Dee, K, Rousset, S, Tosh, I, Middleton, K, Pragt, J, Terrett, D, Brock, M, Benn, C, Verheijen, M, Cano, D, Bevil, C, Steele, I, Mottram, C, Bates, S |
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Fformat: | Journal article |
Iaith: | English |
Cyhoeddwyd: |
2012
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Eitemau Tebyg
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Manufacturing process for the WEAVE Prime Focus Corrector optics for the 4.2m William Herschel Telescope
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The hardware control system for WEAVE at the William Herschel telescope
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Developments in fibre positioning technology for the WEAVE instrument for the William Herschel Telescope
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Integration and early testing of WEAVE: the next-generation spectroscopy facility for the William Herschel Telescope
gan: Dalton, G, et al.
Cyhoeddwyd: (2020) -
Testing process for the WEAVE prime focus corrector lenses for the William Herschel Telescope
gan: Bogunivic, D, et al.
Cyhoeddwyd: (2018)