Project overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope

Gavin Dalton; Scott Trager; Don Carlos Abrams; Piercarlo Bonifacio; J. Alfonso López Aguerri; Kevin Middleton; Chris Benn; Kevin Dee; Frédéric Sayède; Ian Lewis; Johan Pragt; Sergio Pico; Nic Walton; Juerg Rey; Carlos Allende Prieto; José Peñate; Emilie Lhome; Tibor Agócs; José Alonso; David Terrett; Matthew Brock; James Gilbert; Andy Ridings; Isabelle Guinouard; Marc A.W. Verheijen; Ian Tosh; Kevin Rogers; Iain Steele; Remko Stuik; Neils Tromp; Attila Jasko; Jan Kragt; Dirk Lesman; Chris Mottram; Stuart Bates; Frank Gribbin; Luis Fernando Rodriguez; José M. Delgado; Carlos Martin; Diego Cano; Ramón Navarro; Mike Irwin; Jim Lewis; Eduardo Gonzalez Solares; Neil O'Mahony; Andrea Bianco; Christina Zurita; Rik ter Horst; Emilio Molinari; Marcello Lodi; José Guerra; Antonella Vallenari; Andrea Baruffolo

doi:10.1117/12.2055132

Project overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope

Gavin Dalton, Scott Trager, Don Carlos Abrams, Piercarlo Bonifacio, J. Alfonso López Aguerri, Kevin Middleton, Chris Benn, Kevin Dee, Frédéric Sayède, Ian Lewis, Johan Pragt, Sergio Pico, Nic Walton, Juerg Rey, Carlos Allende Prieto, José Peñate, Emilie Lhome, Tibor Agócs, José Alonso, David TerrettMatthew Brock, James Gilbert, Andy Ridings, Isabelle Guinouard, Marc A.W. Verheijen, Ian Tosh, Kevin Rogers, Iain Steele, Remko Stuik, Neils Tromp, Attila Jasko, Jan Kragt, Dirk Lesman, Chris Mottram, Stuart Bates, Frank Gribbin, Luis Fernando Rodriguez, José M. Delgado, Carlos Martin, Diego Cano, Ramón Navarro, Mike Irwin, Jim Lewis, Eduardo Gonzalez Solares, Neil O'Mahony, Andrea Bianco, Christina Zurita, Rik ter Horst, Emilio Molinari, Marcello Lodi, José Guerra, Antonella Vallenari, Andrea Baruffolo

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We present an overview of and status report on the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT). WEAVE principally targets optical ground-based follow up of upcoming ground-based (LOFAR) and space-based (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, 20 integral field units, or a single large IFU 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. The project is now in the final design and early procurement phase, with commissioning at the telescope expected in 2017.

Originele taal-2	English
Titel	Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series
Uitgeverij	SPIE
Pagina's	91470L
Volume	9147
DOI's	https://doi.org/10.1117/12.2055132
Status	Published - jul.-2014

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Dalton, G., Trager, S., Abrams, D. C., Bonifacio, P., López Aguerri, J. A., Middleton, K., Benn, C., Dee, K., Sayède, F., Lewis, I., Pragt, J., Pico, S., Walton, N., Rey, J., Allende Prieto, C., Peñate, J., Lhome, E., Agócs, T., Alonso, J., ... Baruffolo, A. (2014). Project overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope. In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series (Vol. 9147, blz. 91470L). SPIE. https://doi.org/10.1117/12.2055132

@inproceedings{47bf0037ec3849a09aa8874f73e254e5,

title = "Project overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope",

abstract = "We present an overview of and status report on the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT). WEAVE principally targets optical ground-based follow up of upcoming ground-based (LOFAR) and space-based (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, 20 integral field units, or a single large IFU 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. The project is now in the final design and early procurement phase, with commissioning at the telescope expected in 2017.",

author = "Gavin Dalton and Scott Trager and Abrams, {Don Carlos} and Piercarlo Bonifacio and {L{\'o}pez Aguerri}, {J. Alfonso} and Kevin Middleton and Chris Benn and Kevin Dee and Fr{\'e}d{\'e}ric Say{\`e}de and Ian Lewis and Johan Pragt and Sergio Pico and Nic Walton and Juerg Rey and {Allende Prieto}, Carlos and Jos{\'e} Pe{\~n}ate and Emilie Lhome and Tibor Ag{\'o}cs and Jos{\'e} Alonso and David Terrett and Matthew Brock and James Gilbert and Andy Ridings and Isabelle Guinouard and Verheijen, {Marc A.W.} and Ian Tosh and Kevin Rogers and Iain Steele and Remko Stuik and Neils Tromp and Attila Jasko and Jan Kragt and Dirk Lesman and Chris Mottram and Stuart Bates and Frank Gribbin and Rodriguez, {Luis Fernando} and Delgado, {Jos{\'e} M.} and Carlos Martin and Diego Cano and Ram{\'o}n Navarro and Mike Irwin and Jim Lewis and {Gonzalez Solares}, Eduardo and Neil O'Mahony and Andrea Bianco and Christina Zurita and {ter Horst}, Rik and Emilio Molinari and Marcello Lodi and Jos{\'e} Guerra and Antonella Vallenari and Andrea Baruffolo",

year = "2014",

month = jul,

doi = "10.1117/12.2055132",

language = "English",

volume = "9147",

pages = "91470L",

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

publisher = "SPIE",

}

Dalton, G, Trager, S, Abrams, DC, Bonifacio, P, López Aguerri, JA, Middleton, K, Benn, C, Dee, K, Sayède, F, Lewis, I, Pragt, J, Pico, S, Walton, N, Rey, J, Allende Prieto, C, Peñate, J, Lhome, E, Agócs, T, Alonso, J, Terrett, D, Brock, M, Gilbert, J, Ridings, A, Guinouard, I, Verheijen, MAW, Tosh, I, Rogers, K, Steele, I, Stuik, R, Tromp, N, Jasko, A, Kragt, J, Lesman, D, Mottram, C, Bates, S, Gribbin, F, Rodriguez, LF, Delgado, JM, Martin, C, Cano, D, Navarro, R, Irwin, M, Lewis, J, Gonzalez Solares, E, O'Mahony, N, Bianco, A, Zurita, C, ter Horst, R, Molinari, E, Lodi, M, Guerra, J, Vallenari, A & Baruffolo, A 2014, Project overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope. in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series. vol. 9147, SPIE, blz. 91470L. https://doi.org/10.1117/12.2055132

TY - GEN

T1 - Project overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope

AU - Dalton, Gavin

AU - Trager, Scott

AU - Abrams, Don Carlos

AU - Bonifacio, Piercarlo

AU - López Aguerri, J. Alfonso

AU - Middleton, Kevin

AU - Benn, Chris

AU - Dee, Kevin

AU - Sayède, Frédéric

AU - Lewis, Ian

AU - Pragt, Johan

AU - Pico, Sergio

AU - Walton, Nic

AU - Rey, Juerg

AU - Allende Prieto, Carlos

AU - Peñate, José

AU - Lhome, Emilie

AU - Agócs, Tibor

AU - Alonso, José

AU - Terrett, David

AU - Brock, Matthew

AU - Gilbert, James

AU - Ridings, Andy

AU - Guinouard, Isabelle

AU - Verheijen, Marc A.W.

AU - Tosh, Ian

AU - Rogers, Kevin

AU - Steele, Iain

AU - Stuik, Remko

AU - Tromp, Neils

AU - Jasko, Attila

AU - Kragt, Jan

AU - Lesman, Dirk

AU - Mottram, Chris

AU - Bates, Stuart

AU - Gribbin, Frank

AU - Rodriguez, Luis Fernando

AU - Delgado, José M.

AU - Martin, Carlos

AU - Cano, Diego

AU - Navarro, Ramón

AU - Irwin, Mike

AU - Lewis, Jim

AU - Gonzalez Solares, Eduardo

AU - O'Mahony, Neil

AU - Bianco, Andrea

AU - Zurita, Christina

AU - ter Horst, Rik

AU - Molinari, Emilio

AU - Lodi, Marcello

AU - Guerra, José

AU - Vallenari, Antonella

AU - Baruffolo, Andrea

PY - 2014/7

Y1 - 2014/7

N2 - We present an overview of and status report on the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT). WEAVE principally targets optical ground-based follow up of upcoming ground-based (LOFAR) and space-based (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, 20 integral field units, or a single large IFU 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. The project is now in the final design and early procurement phase, with commissioning at the telescope expected in 2017.

AB - We present an overview of and status report on the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT). WEAVE principally targets optical ground-based follow up of upcoming ground-based (LOFAR) and space-based (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, 20 integral field units, or a single large IFU 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. The project is now in the final design and early procurement phase, with commissioning at the telescope expected in 2017.

UR - http://adsabs.harvard.edu/abs/2014SPIE.9147E..0LD

U2 - 10.1117/12.2055132

DO - 10.1117/12.2055132

M3 - Conference contribution

VL - 9147

SP - 91470L

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

PB - SPIE

ER -

Project overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel Telescope

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