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
Fariña C
(2018)
Design of the observation queue scheduler for WEAVE on the WHT
Leung H
(2018)
Deep learning of multi-element abundances from high-resolution spectroscopic data
in Monthly Notices of the Royal Astronomical Society
Maiolino R
(2019)
De re metallica: the cosmic chemical evolution of galaxies
in The Astronomy and Astrophysics Review
Deason A
(2018)
Cresting the wave: proper motions of the Eastern Banded Structure
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
Jofré P
(2017)
Climbing the cosmic ladder with stellar twins in RAVE with Gaia
in Monthly Notices of the Royal Astronomical Society
Hughes S
(2022)
Calibration at elevation of the WEAVE fibre positioner
Buist H
(2017)
Behaviour of streams in angle and frequency spaces in different potentials
in Astronomy & Astrophysics
Blomqvist M
(2019)
Baryon acoustic oscillations from the cross-correlation of Ly a absorption and quasars in eBOSS DR14
in Astronomy & Astrophysics
Du Mas Des Bourboux H
(2017)
Baryon acoustic oscillations from the complete SDSS-III Ly a -quasar cross-correlation function at z = 2.4
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 |