The design of the WEAVE spectrograph

Kevin Rogers; Remko Stuik; Iain A. Steele; Johan Pragt; Kevin F. Middleton; Stuart Bates; Jan Kragt; Niels Tromp; Dirk Lesman; Emilie Lhomé; Gavin Dalton; Scott Trager; Ramon Navarro; Don C. Abrams; Ian Tosh; Attila Jasko; Carlos Martin; Neil O'Mahony; Sergio Pico; Diego Cano Infantes; Andrea Bianca; Jose Delgado; Luis F. Rodríguez

doi:10.1117/12.2055860

The design of the WEAVE spectrograph

Kevin Rogers, Remko Stuik, Iain A. Steele, Johan Pragt, Kevin F. Middleton, Stuart Bates, Jan Kragt, Niels Tromp, Dirk Lesman, Emilie Lhomé, Gavin Dalton, Scott Trager, Ramon Navarro, Don C. Abrams, Ian Tosh, Attila Jasko, Carlos Martin, Neil O'Mahony, Sergio Pico, Diego Cano InfantesAndrea Bianca, Jose Delgado, Luis F. Rodríguez

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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.

Originele taal-2	English
Titel	Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series
Pagina's	91476H
Volume	9147
DOI's	https://doi.org/10.1117/12.2055860
Status	Published - 1-jul.-2014

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http://adsabs.harvard.edu/abs/2014SPIE.9147E..6HR

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Rogers, K., Stuik, R., Steele, I. A., Pragt, J., Middleton, K. F., Bates, S., Kragt, J., Tromp, N., Lesman, D., Lhomé, E., Dalton, G., Trager, S., Navarro, R., Abrams, D. C., Tosh, I., Jasko, A., Martin, C., O'Mahony, N., Pico, S., ... Rodríguez, L. F. (2014). The design of the WEAVE spectrograph. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series (Vol. 9147, blz. 91476H) https://doi.org/10.1117/12.2055860

@inproceedings{c4387e57f23a44168ea963cc478ec631,

title = "The design of the WEAVE spectrograph",

abstract = "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.",

author = "Kevin Rogers and Remko Stuik and Steele, {Iain A.} and Johan Pragt and Middleton, {Kevin F.} and Stuart Bates and Jan Kragt and Niels Tromp and Dirk Lesman and Emilie Lhom{\'e} and Gavin Dalton and Scott Trager and Ramon Navarro and Abrams, {Don C.} and Ian Tosh and Attila Jasko and Carlos Martin and Neil O'Mahony and Sergio Pico and {Cano Infantes}, Diego and Andrea Bianca and Jose Delgado and Rodr{\'i}guez, {Luis F.}",

year = "2014",

month = jul,

day = "1",

doi = "10.1117/12.2055860",

language = "English",

volume = "9147",

pages = "91476H",

booktitle = "Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series",

}

Rogers, K, Stuik, R, Steele, IA, Pragt, J, Middleton, KF, Bates, S, Kragt, J, Tromp, N, Lesman, D, Lhomé, E, Dalton, G, Trager, S, Navarro, R, Abrams, DC, Tosh, I, Jasko, A, Martin, C, O'Mahony, N, Pico, S, Cano Infantes, D, Bianca, A, Delgado, J & Rodríguez, LF 2014, The design of the WEAVE spectrograph. in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. vol. 9147, blz. 91476H. https://doi.org/10.1117/12.2055860

TY - GEN

T1 - The design of the WEAVE spectrograph

AU - Rogers, Kevin

AU - Stuik, Remko

AU - Steele, Iain A.

AU - Pragt, Johan

AU - Middleton, Kevin F.

AU - Bates, Stuart

AU - Kragt, Jan

AU - Tromp, Niels

AU - Lesman, Dirk

AU - Lhomé, Emilie

AU - Dalton, Gavin

AU - Trager, Scott

AU - Navarro, Ramon

AU - Abrams, Don C.

AU - Tosh, Ian

AU - Jasko, Attila

AU - Martin, Carlos

AU - O'Mahony, Neil

AU - Pico, Sergio

AU - Cano Infantes, Diego

AU - Bianca, Andrea

AU - Delgado, Jose

AU - Rodríguez, Luis F.

PY - 2014/7/1

Y1 - 2014/7/1

N2 - 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.

AB - 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.

U2 - 10.1117/12.2055860

DO - 10.1117/12.2055860

M3 - Conference contribution

VL - 9147

SP - 91476H

BT - Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series

ER -

The design of the WEAVE spectrograph

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