WEAVE: The next generation wide-field spectroscopy facility for the William Herschel Telescope

Gavin Dalton; Scott C. Trager; Don Carlos Abrams; David Carter; Piercarlo Bonifacio; J. Alfonso L. Aguerri; Mike MacIntosh; Chris Evans; Ian Lewis; Ramon Navarro; Tibor Agocs; Kevin Dee; Sophie Rousset; Ian Tosh; Kevin Middleton; Johannes Pragt; David Terrett; Matthew Brock; Chris Benn; Marc Verheijen; Diego Cano Infantes; Craige Bevil; Iain Steele; Chris Mottram; Stuart Bates; Francis J. Gribbin; Jürg Rey; Luis Fernando Rodriguez; Jose Miguel Delgado; Isabelle Guinouard; Nic Walton; Michael J. Irwin; Pascal Jagourel; Remko Stuik; Gerrit Gerlofsma; Ronald Roelfsma; Ian Skillen; Andy Ridings; Marc Balcells; Jean-Baptiste Daban; Carole Gouvret; Lars Venema; Paul Girard

doi:10.1117/12.925950

WEAVE: The next generation wide-field spectroscopy facility for the William Herschel Telescope

Gavin Dalton, Scott C. Trager, Don Carlos Abrams, David Carter, Piercarlo Bonifacio, J. Alfonso L. Aguerri, Mike MacIntosh, Chris Evans, Ian Lewis, Ramon Navarro, Tibor Agocs, Kevin Dee, Sophie Rousset, Ian Tosh, Kevin Middleton, Johannes Pragt, David Terrett, Matthew Brock, Chris Benn, Marc VerheijenDiego Cano Infantes, Craige Bevil, Iain Steele, Chris Mottram, Stuart Bates, Francis J. Gribbin, Jürg Rey, Luis Fernando Rodriguez, Jose Miguel Delgado, Isabelle Guinouard, Nic Walton, Michael J. Irwin, Pascal Jagourel, Remko Stuik, Gerrit Gerlofsma, Ronald Roelfsma, Ian Skillen, Andy Ridings, Marc Balcells, Jean-Baptiste Daban, Carole Gouvret, Lars Venema, Paul Girard

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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 spacebased (Gaia) surveys. WEAVE is a multi-object and multi-IFU facility utilizing a new 2 degree prime focus field of view at the WHT, with a buffered pick and place positioner system hosting 1000 multi-object (MOS) fibres or up to 30 integral field units for each observation. The fibres are fed to a single spectrograph, with a pair of 8k(spectral) x 6k (spatial) pixel cameras, located within the WHT GHRIL enclosure on the telescope Nasmyth platform, supporting observations at R~5000 over the full 370-1000nm wavelength range in a single exposure, or a high resolution mode with limited coverage in each arm at R~20000.

Originele taal-2	English
Titel	Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series
Uitgeverij	SPIE.Digital Library
Aantal pagina's	12
Volume	8446
DOI's	https://doi.org/10.1117/12.925950
Status	Published - sep.-2012

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Dalton, G., Trager, S. C., Abrams, D. C., Carter, D., Bonifacio, P., Aguerri, J. A. L., 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., ... Girard, P. (2012). WEAVE: The next generation wide-field spectroscopy facility for the William Herschel Telescope. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series (Vol. 8446). Artikel 84460P SPIE.Digital Library. https://doi.org/10.1117/12.925950

@inproceedings{485b5c62fc064fceab370011bdb29bc0,

title = "WEAVE: The next generation wide-field spectroscopy facility for the William Herschel Telescope",

abstract = "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 spacebased (Gaia) surveys. WEAVE is a multi-object and multi-IFU facility utilizing a new 2 degree prime focus field of view at the WHT, with a buffered pick and place positioner system hosting 1000 multi-object (MOS) fibres or up to 30 integral field units for each observation. The fibres are fed to a single spectrograph, with a pair of 8k(spectral) x 6k (spatial) pixel cameras, located within the WHT GHRIL enclosure on the telescope Nasmyth platform, supporting observations at R~5000 over the full 370-1000nm wavelength range in a single exposure, or a high resolution mode with limited coverage in each arm at R~20000.",

author = "Gavin Dalton and Trager, {Scott C.} and Abrams, {Don Carlos} and David Carter and Piercarlo Bonifacio and Aguerri, {J. Alfonso L.} and Mike MacIntosh and Chris Evans and Ian Lewis and Ramon Navarro and Tibor Agocs and Kevin Dee and Sophie Rousset and Ian Tosh and Kevin Middleton and Johannes Pragt and David Terrett and Matthew Brock and Chris Benn and Marc Verheijen and {Cano Infantes}, Diego and Craige Bevil and Iain Steele and Chris Mottram and Stuart Bates and Gribbin, {Francis J.} and J{\"u}rg Rey and Rodriguez, {Luis Fernando} and Delgado, {Jose Miguel} and Isabelle Guinouard and Nic Walton and Irwin, {Michael J.} and Pascal Jagourel and Remko Stuik and Gerrit Gerlofsma and Ronald Roelfsma and Ian Skillen and Andy Ridings and Marc Balcells and Jean-Baptiste Daban and Carole Gouvret and Lars Venema and Paul Girard",

note = "ISBN: 9780819491473 M1 - Conference Proceedings",

year = "2012",

month = sep,

doi = "10.1117/12.925950",

language = "English",

volume = "8446",

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

publisher = "SPIE.Digital Library",

}

Dalton, G, Trager, SC, Abrams, DC, Carter, D, Bonifacio, P, Aguerri, JAL, 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 Infantes, D, Bevil, C, Steele, I, Mottram, C, Bates, S, Gribbin, FJ, Rey, J, Rodriguez, LF, Delgado, JM, Guinouard, I, Walton, N, Irwin, MJ, Jagourel, P, Stuik, R, Gerlofsma, G, Roelfsma, R, Skillen, I, Ridings, A, Balcells, M, Daban, J-B, Gouvret, C, Venema, L & Girard, P 2012, WEAVE: The next generation wide-field spectroscopy facility for the William Herschel Telescope. in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. vol. 8446, 84460P, SPIE.Digital Library. https://doi.org/10.1117/12.925950

TY - GEN

T1 - WEAVE

T2 - The next generation wide-field spectroscopy facility for the William Herschel Telescope

AU - Dalton, Gavin

AU - Trager, Scott C.

AU - Abrams, Don Carlos

AU - Carter, David

AU - Bonifacio, Piercarlo

AU - Aguerri, J. Alfonso L.

AU - MacIntosh, Mike

AU - Evans, Chris

AU - Lewis, Ian

AU - Navarro, Ramon

AU - Agocs, Tibor

AU - Dee, Kevin

AU - Rousset, Sophie

AU - Tosh, Ian

AU - Middleton, Kevin

AU - Pragt, Johannes

AU - Terrett, David

AU - Brock, Matthew

AU - Benn, Chris

AU - Verheijen, Marc

AU - Cano Infantes, Diego

AU - Bevil, Craige

AU - Steele, Iain

AU - Mottram, Chris

AU - Bates, Stuart

AU - Gribbin, Francis J.

AU - Rey, Jürg

AU - Rodriguez, Luis Fernando

AU - Delgado, Jose Miguel

AU - Guinouard, Isabelle

AU - Walton, Nic

AU - Irwin, Michael J.

AU - Jagourel, Pascal

AU - Stuik, Remko

AU - Gerlofsma, Gerrit

AU - Roelfsma, Ronald

AU - Skillen, Ian

AU - Ridings, Andy

AU - Balcells, Marc

AU - Daban, Jean-Baptiste

AU - Gouvret, Carole

AU - Venema, Lars

AU - Girard, Paul

N1 - ISBN: 9780819491473 M1 - Conference Proceedings

PY - 2012/9

Y1 - 2012/9

N2 - 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 spacebased (Gaia) surveys. WEAVE is a multi-object and multi-IFU facility utilizing a new 2 degree prime focus field of view at the WHT, with a buffered pick and place positioner system hosting 1000 multi-object (MOS) fibres or up to 30 integral field units for each observation. The fibres are fed to a single spectrograph, with a pair of 8k(spectral) x 6k (spatial) pixel cameras, located within the WHT GHRIL enclosure on the telescope Nasmyth platform, supporting observations at R~5000 over the full 370-1000nm wavelength range in a single exposure, or a high resolution mode with limited coverage in each arm at R~20000.

AB - 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 spacebased (Gaia) surveys. WEAVE is a multi-object and multi-IFU facility utilizing a new 2 degree prime focus field of view at the WHT, with a buffered pick and place positioner system hosting 1000 multi-object (MOS) fibres or up to 30 integral field units for each observation. The fibres are fed to a single spectrograph, with a pair of 8k(spectral) x 6k (spatial) pixel cameras, located within the WHT GHRIL enclosure on the telescope Nasmyth platform, supporting observations at R~5000 over the full 370-1000nm wavelength range in a single exposure, or a high resolution mode with limited coverage in each arm at R~20000.

UR - http://adsabs.harvard.edu/abs/2012SPIE.8446E..0PD

U2 - 10.1117/12.925950

DO - 10.1117/12.925950

M3 - Conference contribution

VL - 8446

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

PB - SPIE.Digital Library

ER -

WEAVE: The next generation wide-field spectroscopy facility for the William Herschel Telescope

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