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
Orenstein B
(2019)
The redshift distribution of infrared-faint radio sources
in Monthly Notices of the Royal Astronomical Society
Everall A
(2020)
seestar: Selection functions for spectroscopic surveys of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Veras D
(2020)
Constraining planet formation around 6-8 M? stars
in Monthly Notices of the Royal Astronomical Society
Rendle B
(2019)
The K2 Galactic Caps Project - going beyond the Kepler field and ageing the Galactic disc
in Monthly Notices of the Royal Astronomical Society
Miller J
(2019)
Searching for the shadows of giants: characterizing protoclusters with line of sight Lyman-a absorption
in Monthly Notices of the Royal Astronomical Society
Laporte C
(2019)
Stellar disc streams as probes of the Galactic potential and satellite impacts
in Monthly Notices of the Royal Astronomical Society
Gómez F
(2019)
Footprints of the Sagittarius dwarf galaxy in the Gaia data set
in Monthly Notices of the Royal Astronomical Society
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
Minchev I
(2019)
Yule-Simpson's paradox in Galactic Archaeology
in Monthly Notices of the Royal Astronomical Society
Žerjal M
(2019)
The GALAH Survey: lithium-strong KM dwarfs
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 |