WEAVE Detectors Interim
Lead Research Organisation:
Liverpool John Moores University
Department Name: Astrophysics Research Institute
Abstract
Start detector procurement for WEAVE
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
Walton Nicholas
(2015)
Gaia, PLATO and WEAVE: A Powerful combination for Exoplanet Characterisation
in AAS/Division for Extreme Solar Systems Abstracts
Jofré P
(2019)
Accuracy and Precision of Industrial Stellar Abundances
in Annual Review of Astronomy and Astrophysics
Gilbert James
(2015)
Verification of commercial motor performance for WEAVE at the William Herschel Telescope
in arXiv e-prints
Khoperskov S
(2020)
Hic sunt dracones: Cartography of the Milky Way spiral arms and bar resonances with Gaia Data Release 2
in Astronomy & Astrophysics
Hale C
(2019)
LOFAR observations of the XMM-LSS field
in Astronomy & Astrophysics
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
Gürkan G
(2019)
LoTSS/HETDEX: Optical quasars I. Low-frequency radio properties of optically selected quasars
in Astronomy & Astrophysics
Geier S
(2019)
The population of hot subdwarf stars studied with Gaia II. The Gaia DR2 catalogue of hot subluminous stars
in Astronomy & Astrophysics
Koppelman H
(2019)
Multiple retrograde substructures in the Galactic halo: A shattered view of Galactic history
in Astronomy & Astrophysics
Hardcastle M
(2019)
Radio-loud AGN in the first LoTSS data release The lifetimes and environmental impact of jet-driven sources
in Astronomy & Astrophysics
Description | This is an interim grant to begin work on the development of detectors for the WEAVE spectrograph. The main element of this work is to come in the final work package now underway - this funding was used to develop the project to conceptual design and make a downpayment on array production. |
Exploitation Route | Experiments with pseudo-dummy and dummy CCD outputs to reduce common read house. |
Sectors | Digital/Communication/Information Technologies (including Software) |
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 |