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
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
Orenstein B
(2019)
The redshift distribution of infrared-faint radio sources
in Monthly Notices of the Royal Astronomical Society
Li T
(2019)
The southern stellar stream spectroscopic survey (S5): Overview, target selection, data reduction, validation, and early science
in Monthly Notices of the Royal Astronomical Society
Lewis J.
(2019)
The WEAVE Core Processing System at CASU
in Highlights on Spanish Astrophysics X
Famaey B.
(2016)
The WEAVE disk dynamics survey
in SF2A-2016: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics
Famaey B.
(2016)
The WEAVE disk dynamics survey
in SF2A-2016: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics
Carrasco E
(2018)
The WEAVE observatory control system
Canchado M
(2018)
The WEAVE prime focus correction: from design to integration
Peralta De Arriba L.
(2019)
The WEAVE Quick-Look GUI
in Highlights on Spanish Astrophysics X
Balcells M
(2015)
The WEAVE spectrograph on the WHT: plans for radial velocity and chemistry surveys of the northern and equatorial Milky Way
in EAS Publications Series
Balcells M
(2015)
The WEAVE spectrograph on the WHT: plans for radial velocity and chemistry surveys of the northern and equatorial Milky Way
in EAS Publications Series
Smith D
(2016)
The WEAVE-LOFAR Survey
Smith D
(2016)
The WEAVE-LOFAR Survey
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
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
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 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
Zanutta A
(2018)
VPHGs for WEAVE: design, manufacturing and characterization
Molinari E.
(2016)
WAS: Textures of the WEAVE Science Archive
in Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields
Molinari E.
(2016)
WAS: Textures of the WEAVE Science Archive
in Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields
Bonifacio P.
(2016)
WEAVE an overview and status update
in SF2A-2016: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics
Bonifacio P.
(2016)
WEAVE an overview and status update
in SF2A-2016: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics
Izazaga R
(2018)
WEAVE spectrograph cameras: the polishing of the spherical lenses
Dalton G.
(2016)
WEAVE: The Next Generation Spectroscopy Facility for the WHT
in Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields
Dalton G.
(2016)
WEAVE: The Next Generation Spectroscopy Facility for the WHT
in Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields
Esposito M
(2022)
Weighing cosmic structures with clusters of galaxies and the intergalactic medium
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
| 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 |