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
Jofré P
(2019)
Accuracy and Precision of Industrial Stellar Abundances
in Annual Review of Astronomy and Astrophysics
Japelj J
(2019)
Simulating MOS science on the ELT: Ly a forest tomography
in Astronomy & Astrophysics
Hughes S
(2022)
Calibration at elevation of the WEAVE fibre positioner
Hughes S
(2022)
Optimisation of the WEAVE target assignment algorithm
Howes L
(2019)
Estimating stellar ages and metallicities from parallaxes and broadband photometry: successes and shortcomings
in Astronomy & Astrophysics
Harris A
(2019)
A study of full space motions of outer Galactic disc A and F stars in two deep pencil beams
in Monthly Notices of the Royal Astronomical Society
Hardcastle M
(2019)
Radio-loud AGN in the first LoTSS data release The lifetimes and environmental impact of jet-driven sources
in Astronomy & Astrophysics
Ham S. J.
(2016)
Towards an Integrated Model of the WEAVE Performance
in Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields
Hale C
(2019)
LOFAR observations of the XMM-LSS field
in Astronomy & Astrophysics
Haines T
(2019)
Implications of a Time-varying Galactic Potential for Determinations of the Dynamical Surface Density
in The Astrophysical Journal
Description | The WEAVE detector system was successfully built to specification and is now in use at the WHT. |
Exploitation Route | Science exploitation |
Sectors | Other |
URL | https://www.ing.iac.es/astronomy/instruments/weave/weaveinst.html |
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 |