WEAVE Detectors Completion

Lead Research Organisation: Liverpool John Moores University
Department Name: Astrophysics Research Institute

Abstract

This grant is to complete the production and commissioning of the detector system for the WEAVE spectrograph.

Planned Impact

ARI has a long tradition of strong industrial and PUS engagement. For this particular project we will continue our policy of engagement with engineering firms who will be commissioned to manufacture the structure of the instrument. In the past this has allowed firms working with us to upgrade their skills and machinery to deliver the high precision needed for astronomical instrumentation, allowing them to received grants and R&D tax credits in order to upgrade their precision machining capability and safeguarding a number of jobs at the time. In addition such firms have been able to use their work on astronomical instrumentation to enhance their reputation with other customers and has assisted them in gaining access to new markets (for example contracts with ING and CERN).

Publications

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Smith L (2018) VIRAC: the VVV Infrared Astrometric Catalogue in Monthly Notices of the Royal Astronomical Society

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Ċ½erjal M (2019) The GALAH Survey: lithium-strong KM dwarfs in Monthly Notices of the Royal Astronomical Society

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De Boer T (2018) The fall of the Northern Unicorn: tangential motions in the Galactic anticentre with SDSS and Gaia in Monthly Notices of the Royal Astronomical Society

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Kumari N (2018) O/H-N/O: the curious case of NGC 4670 in Monthly Notices of the Royal Astronomical Society

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Breedt E (2017) Using large spectroscopic surveys to test the double degenerate model for Type Ia supernovae in Monthly Notices of the Royal Astronomical Society

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Rendle B (2019) The K2 Galactic Caps Project - going beyond the Kepler field and ageing the Galactic disc in Monthly Notices of the Royal Astronomical Society

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Williams W (2018) LOFAR-Boötes: properties of high- and low-excitation radio galaxies at 0.5 < z < 2.0 in Monthly Notices of the Royal Astronomical Society

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Starkenburg E (2017) The Pristine survey - I. Mining the Galaxy for the most metal-poor stars in Monthly Notices of the Royal Astronomical Society

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Gonzalez-Perez V (2017) The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5 in Monthly Notices of the Royal Astronomical Society

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Venn K (2020) The Pristine survey - IX. CFHT ESPaDOnS spectroscopic analysis of 115 bright metal-poor candidate stars in Monthly Notices of the Royal Astronomical Society

 
Description The WEAVE detector system was successfully built to specification and is now in use at the WHT.
Exploitation Route Scientific Exploitation of WEAVE
Sectors Other

URL https://www.ing.iac.es/astronomy/instruments/weave/weaveinst.html