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
Oliva E
(2019)
Experimental characterization of modal noise in multimode fibers for astronomical spectrometers
in Astronomy & Astrophysics
Zwitter T
(2020)
The GALAH survey: chemodynamics of the solar neighbourhood
in Monthly Notices of the Royal Astronomical Society
Koposov S
(2020)
Discovery of a nearby 1700 km s-1 star ejected from the Milky Way by Sgr A*
in Monthly Notices of the Royal Astronomical Society
Veras D
(2020)
Constraining planet formation around 6-8 M? stars
in Monthly Notices of the Royal Astronomical Society
Manser C
(2020)
The frequency of gaseous debris discs around white dwarfs
in Monthly Notices of the Royal Astronomical Society
Amard L
(2020)
The Impact of Metallicity on the Evolution of the Rotation and Magnetic Activity of Sun-like Stars
in The Astrophysical Journal
Das P
(2020)
seestar: Selection functions for spectroscopic surveys of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Youakim K
(2020)
The Pristine Survey - VIII. The metallicity distribution function of the Milky Way halo down to the extremely metal-poor regime
in Monthly Notices of the Royal Astronomical Society
Khoperskov S
(2020)
Hic sunt dracones: Cartography of the Milky Way spiral arms and bar resonances with Gaia Data Release 2
in Astronomy & Astrophysics
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 |