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
Das P
(2020)
seestar: Selection functions for spectroscopic surveys of the Milky Way
in Monthly Notices of the Royal Astronomical Society
De Sainte Agathe V
(2019)
Baryon acoustic oscillations at z = 2.34 from the correlations of Ly a absorption in eBOSS DR14
in Astronomy & Astrophysics
Duncan K
(2019)
The LOFAR Two-metre Sky Survey IV. First Data Release: Photometric redshifts and rest-frame magnitudes
in Astronomy & Astrophysics
Esposito M
(2022)
Weighing cosmic structures with clusters of galaxies and the intergalactic medium
in Monthly Notices of the Royal Astronomical Society
Famaey B.
(2016)
The WEAVE disk dynamics survey
in SF2A-2016: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics
Fariña C
(2018)
Design of the observation queue scheduler for WEAVE on the WHT
Fratta M
(2023)
Spectroscopic follow-up of a subset of the Gaia /IPHAS catalogue of Ha-excess sources
in Monthly Notices of the Royal Astronomical Society
Garavito-Camargo N
(2019)
Hunting for the Dark Matter Wake Induced by the Large Magellanic Cloud
in The Astrophysical Journal
Geier S
(2019)
The population of hot subdwarf stars studied with Gaia II. The Gaia DR2 catalogue of hot subluminous stars
in Astronomy & Astrophysics
Gentile Fusillo N
(2019)
A Gaia Data Release 2 catalogue of white dwarfs and a comparison with SDSS
in Monthly Notices of the Royal Astronomical Society
Gilbert J.
(2016)
Verification of Commercial Motor Performance for WEAVE at the William Herschel Telescope
in Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields
Gilbert James
(2015)
Verification of commercial motor performance for WEAVE at the William Herschel Telescope
in arXiv e-prints
Gómez F
(2019)
Footprints of the Sagittarius dwarf galaxy in the Gaia data set
in Monthly Notices of the Royal Astronomical Society
Gürkan G
(2019)
LoTSS/HETDEX: Optical quasars I. Low-frequency radio properties of optically selected quasars
in Astronomy & Astrophysics
Haines T
(2019)
Implications of a Time-varying Galactic Potential for Determinations of the Dynamical Surface Density
in The Astrophysical Journal
Hale C
(2019)
LOFAR observations of the XMM-LSS field
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
Hardcastle M
(2019)
Radio-loud AGN in the first LoTSS data release The lifetimes and environmental impact of jet-driven sources
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
Howes L
(2019)
Estimating stellar ages and metallicities from parallaxes and broadband photometry: successes and shortcomings
in Astronomy & Astrophysics
Hughes S
(2022)
Calibration at elevation of the WEAVE fibre positioner
Hughes S
(2022)
Optimisation of the WEAVE target assignment algorithm
Japelj J
(2019)
Simulating MOS science on the ELT: Ly a forest tomography
in Astronomy & Astrophysics
Jofré P
(2019)
Accuracy and Precision of Industrial Stellar Abundances
in Annual Review of Astronomy and Astrophysics
Khoperskov S
(2020)
Hic sunt dracones: Cartography of the Milky Way spiral arms and bar resonances with Gaia Data Release 2
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 |