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
Sabater J
(2019)
The LoTSS view of radio AGN in the local Universe The most massive galaxies are always switched on
in Astronomy & Astrophysics
Chabanier S
(2019)
The one-dimensional power spectrum from the SDSS DR14 Lya forests
in Journal of Cosmology and Astroparticle Physics
Brauer K
(2019)
The Origin of r -process Enhanced Metal-poor Halo Stars In Now-destroyed Ultra-faint Dwarf Galaxies
in The Astrophysical Journal
Ting Y
(2019)
The Payne : Self-consistent ab initio Fitting of Stellar Spectra
in The Astrophysical Journal
Padilla C
(2019)
The Physics of the Accelerating Universe Camera
in The Astronomical Journal
Middleton K
(2018)
The polishing of WEAVE spectrograph collimator mirror
Geier S
(2019)
The population of hot subdwarf stars studied with Gaia II. The Gaia DR2 catalogue of hot subluminous stars
in Astronomy & Astrophysics
Venn K
(2020)
The Pristine survey - IX. CFHT ESPaDOnS spectroscopic analysis of 115 bright metal-poor candidate stars
in Monthly Notices of the Royal Astronomical Society
Aguado D
(2019)
The Pristine survey - VI. The first three years of medium-resolution follow-up spectroscopy of Pristine EMP star candidates
in Monthly Notices of the Royal Astronomical Society
Youakim K
(2020)
The Pristine Survey - VIII. The metallicity distribution function of the Milky Way halo down to the extremely metal-poor regime
in Monthly Notices of the Royal Astronomical Society
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 |