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
Kumari N
(2018)
O/H-N/O: the curious case of NGC 4670
in Monthly Notices of the Royal Astronomical Society
Middleton K
(2018)
The polishing of WEAVE spectrograph collimator mirror
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
Bosma A
(2017)
Outskirts of Galaxies
Burden A
(2017)
Mitigating the impact of the DESI fiber assignment on galaxy clustering
in Journal of Cosmology and Astroparticle Physics
DomÃnguez-Tenreiro R
(2017)
The Radial Distribution of Mono-metallicity Populations in the Galactic Disk as Evidence for Two-phase Disk Formation
in The Astrophysical Journal
Ichikawa K
(2017)
Foreground effect on the J-factor estimation of classical dwarf spheroidal galaxies
in Monthly Notices of the Royal Astronomical Society
Conrad C
(2017)
A RAVE investigation on Galactic open clusters II. Open cluster pairs, groups and complexes?
in Astronomy & Astrophysics
Thygesen A
(2017)
An Investigation of the Formation and Line Properties of MgH in 3D Hydrodynamical Model Stellar Atmospheres
in The Astrophysical Journal
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 |