Final design and progress of WEAVE: The next generation wide-field spectroscopy facility for the William Herschel Telescope

Gavin Dalton, Scott Trager, Don Carlos Abrams, Piercarlo Bonifacio, J. Alfonso L. Aguerri, Kevin Middleton, Chris Benn, Kevin Dee, Frédéric Sayède, Ian Lewis, Johannes Pragt, Sergio Pico, Nic Walton, Jeurg Rey, Carlos Allende Prieto, José Peñate, Emilie Lhome, Tibor Agócs, José Alonso, David TerrettMatthew Brock, James Gilbert, Ellen Schallig, Andy Ridings, Isabelle Guinouard, Marc Verheijen, Ian Tosh, Kevin Rogers, Martin Lee, Iain Steele, Remko Stuik, Niels Tromp, Attila Jaskó, Esperanza Carrasco, Szigfrid Farcas, Jan Kragt, Dirk Lesman, Gabby Kroes, Chris Mottram, Stuart Bates, Luis Fernando Rodriguez, Frank Gribbin, José Miguel Delgado, José Miguel Herreros, Carlos Martin, Diego Cano, Ramon Navarro, Mike Irwin, Jim Lewis, Eduardo Gonzalez Solares, David Murphy, Clare Worley, Richard Bassom, Neil O'Mahoney, Andrea Bianco, Christina Zurita, Rik ter Horst, Emilio Molinari, Marcello Lodi, José Guerra, Adrian Martin, Antonella Vallenari, Bernardo Salasnich, Andrea Baruffolo, Shoko Jin, Vanessa Hill, Dan Smith, Janet Drew, Bianca Poggianti, Mat Pieri, Lillian Dominquez Palmero, Cecilia Farina

OnderzoeksoutputAcademicpeer review

35 Citaten (Scopus)

Samenvatting

We present the Final Design of the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT), together with a status update on the details of manufacturing, integration and the overall project schedule now that all the major fabrication contracts are in place. We also present a summary of the current planning behind the 5-year initial phase of survey operations. WEAVE will provide optical ground-based follow up of 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 (dual-beam) spectrograph, with total of 16k spectral pixels, 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 manufacturing and integration phase with first light expected for early of 2018.
Originele taal-2English
TitelGround-based and Airborne Instrumentation for Astronomy VI, 99081G (August 4, 2016)
SubtitelPROCEEDINGS SPIE VOLUME 9908
RedacteurenChristopher J Evans, Luc Simard, Hideki Takami
UitgeverijSPIE.Digital Library
Pagina's99081G
ISBN van geprinte versie9781510601956
DOI's
StatusPublished - 4-aug-2016
EvenementSPIE Astronomical Telescopes + Instrumentation, 2016 - Edinburgh, United Kingdom
Duur: 26-jun-20161-jul-2016

Publicatie series

NaamProceedings SPIE
UitgeverijSPIE.Digital library
Volume9908

Conference

ConferenceSPIE Astronomical Telescopes + Instrumentation, 2016
LandUnited Kingdom
StadEdinburgh
Periode26/06/201601/07/2016

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