WEAVE Detectors Main Grant
Lead Research Organisation:
Liverpool John Moores University
Department Name: Astrophysics Research Institute
Abstract
This grant is to produce 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 a 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

Casalta J
(2018)
The WEAVE prime focus correction: from design to integration


Middleton K
(2018)
Low-level control software for the WEAVE spectrograph

Terlevich R
(2018)
WEAVE spectrograph cameras: the polishing of the spherical lenses

FariƱa C
(2018)
Design of the observation queue scheduler for WEAVE on the WHT

Middleton K
(2018)
Antireflective coatings for the red camera of WEAVE spectrograph

Leung H
(2018)
Deep learning of multi-element abundances from high-resolution spectroscopic data
in Monthly Notices of the Royal Astronomical Society

Terrett D
(2018)
First lab results of the WEAVE fibre positioner system


Zanutta A
(2018)
VPHGs for WEAVE: design, manufacturing and characterization
Description | Collaboration with Isaac Newton Group |
Organisation | Isaac Newton Group of Telescopes (ING) |
Country | Spain |
Sector | Academic/University |
PI Contribution | Joint development of detector systems |
Collaborator Contribution | Expertise in operations and use |
Impact | Development in ongoing, with completion of the new system due in 2018. |
Start Year | 2014 |
Description | Collaboration with University of Oxford |
Organisation | University of Oxford |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Scientific Expertise, Access to telescope time |
Collaborator Contribution | Scientific Expertise, Financial Contribution |
Impact | Collaboration on followup of LOFAR radio transients starting in early 2014. |
Start Year | 2014 |