24 July 2014 The design of the WEAVE spectrograph
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WEAVE is the next-generation optical spectroscopy facility for the William Herschel Telescope and aims at spectroscopic follow-up of ground-based (LOFAR) and space-based (Gaia) surveys. WEAVE places in the re-fitted prime focus either 1000 fibres, 20 fibre-coupled mini-IFUs or a single large 600 fibre IFU. A spectrograph on the Nasmyth platform analyses the light and supports, in a single exposure, either R~5,000 observations over the full 366- 975 nm wavelength range or simultaneous R~20,000 observations over two out of three pre-specified bands within this wavelength range. This paper describes the requirements, optical design and mechanical design of the WEAVE spectrograph.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kevin Rogers, Kevin Rogers, Remko Stuik, Remko Stuik, Iain A. Steele, Iain A. Steele, Johan Pragt, Johan Pragt, Kevin F. Middleton, Kevin F. Middleton, Stuart Bates, Stuart Bates, Jan Kragt, Jan Kragt, Niels Tromp, Niels Tromp, Dirk Lesman, Dirk Lesman, Emilie Lhomé, Emilie Lhomé, Gavin Dalton, Gavin Dalton, Scott Trager, Scott Trager, Ramon Navarro, Ramon Navarro, Don Carlos Abrams, Don Carlos Abrams, Ian Tosh, Ian Tosh, Attila Jasko, Attila Jasko, Carlos Martin, Carlos Martin, Neil O'Mahony, Neil O'Mahony, Sergio Pico, Sergio Pico, Diego Cano Infantes, Diego Cano Infantes, Andrea Bianco, Andrea Bianco, Jose Delgado, Jose Delgado, Luis Fernando Rodríguez, Luis Fernando Rodríguez, "The design of the WEAVE spectrograph", Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 91476H (24 July 2014); doi: 10.1117/12.2055860; https://doi.org/10.1117/12.2055860

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