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
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
Thomas G
(2019)
Dwarfs or Giants? Stellar Metallicities and Distances from ugrizG Multiband Photometry
in The Astrophysical Journal
Ting Y
(2019)
The Payne : Self-consistent ab initio Fitting of Stellar Spectra
in The Astrophysical Journal
Tortora C
(2022)
The Central Dark Matter Fraction of Massive Early-Type Galaxies
in Frontiers in Astronomy and Space Sciences
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
Veras D
(2020)
Constraining planet formation around 6-8 M? stars
in Monthly Notices of the Royal Astronomical Society
Vos J
(2019)
Gaia Data Release 2 catalogue of extremely low-mass white dwarf candidates
in Monthly Notices of the Royal Astronomical Society
Walsh S
(2019)
Optimizing the choice of analysis method for all-sky searches for continuous gravitational waves with Einstein@Home
in Physical Review D
Walton N. A.
(2016)
Gaia and WEAVE/WxES: Supporting the PLATO Exoplanet Hunter
in Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields
Walton Nicholas
(2015)
Gaia, PLATO and WEAVE: A Powerful combination for Exoplanet Characterisation
in AAS/Division for Extreme Solar Systems Abstracts
Wang Y
(2019)
ATLAS probe: Breakthrough science of galaxy evolution, cosmology, Milky Way, and the Solar System
in Publications of the Astronomical Society of Australia
Widmark A
(2019)
The dynamical matter density in the solar neighbourhood inferred from Gaia DR1
in Monthly Notices of the Royal Astronomical Society
Williams W
(2019)
The LOFAR Two-metre Sky Survey III. First data release: Optical/infrared identifications and value-added catalogue
in Astronomy & Astrophysics
Xiang M
(2019)
Abundance Estimates for 16 Elements in 6 Million Stars from LAMOST DR5 Low-Resolution Spectra
in The Astrophysical Journal Supplement Series
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
Zanutta A
(2018)
VPHGs for WEAVE: design, manufacturing and characterization
Zavarygin E
(2019)
A search for cosmological anisotropy using the Lyman alpha forest from SDSS quasar spectra
in Monthly Notices of the Royal Astronomical Society
Zwitter T
(2020)
The GALAH survey: chemodynamics of the solar neighbourhood
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 | 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 |