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
Terrett D
(2018)
First lab results of the WEAVE fibre positioner system
Thomas G
(2022)
The Cetus-Palca stream: A disrupted small dwarf galaxy A prequel to the science possible with WEAVE with precise spectro-photometric distances
in Astronomy & Astrophysics
Thomas G
(2019)
Dwarfs or Giants? Stellar Metallicities and Distances from ugrizG Multiband Photometry
in The Astrophysical Journal
Thygesen A
(2017)
An Investigation of the Formation and Line Properties of MgH in 3D Hydrodynamical Model Stellar Atmospheres
in The Astrophysical Journal
Thévenin F
(2017)
Modern Geometric Methods of Distance Determination
in Space Science Reviews
Ting Y
(2017)
Measuring 14 Elemental Abundances with R = 1800 LAMOST Spectra
in The Astrophysical Journal
Ting Y
(2019)
The Payne : Self-consistent ab initio Fitting of Stellar Spectra
in The Astrophysical Journal
Ting Y
(2017)
Prospects for Measuring Abundances of >20 Elements with Low-resolution Stellar Spectra
in The Astrophysical Journal
Tortora C
(2022)
The Central Dark Matter Fraction of Massive Early-Type Galaxies
in Frontiers in Astronomy and Space Sciences
Traven G
(2017)
The Galah Survey: Classification and Diagnostics with t-SNE Reduction of Spectral Information
in The Astrophysical Journal Supplement Series
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 |