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
Sharma S
(2019)
The K2-HERMES Survey: age and metallicity of the thick disc
in Monthly Notices of the Royal Astronomical Society
Casamiquela L
(2019)
OCCASO - III. Iron peak and a elements of 18 open clusters. Comparison with chemical evolution models and field stars
in Monthly Notices of the Royal Astronomical Society
Esposito M
(2022)
Weighing cosmic structures with clusters of galaxies and the intergalactic medium
in Monthly Notices of the Royal Astronomical Society
Chabanier S
(2019)
The one-dimensional power spectrum from the SDSS DR14 Lya forests
in Journal of Cosmology and Astroparticle Physics
Carrera R.
(2019)
Open clusters through the eyes of WEAVE
in Highlights on Spanish Astrophysics X
Lewis J.
(2019)
The WEAVE Core Processing System at CASU
in Highlights on Spanish Astrophysics X
Peralta De Arriba L.
(2019)
The WEAVE Quick-Look GUI
in Highlights on Spanish Astrophysics X
Schultheis Mathias
(2016)
Large surveys of Galactic populations with the new WEAVE faciligy
in Galactic Surveys: New Results on Formation, Evolution, Structure and Chemical Evolution of the Milky Way
Schultheis Mathias
(2016)
Large surveys of Galactic populations with the new WEAVE faciligy
in Galactic Surveys: New Results on Formation, Evolution, Structure and Chemical Evolution of the Milky Way
Tortora C
(2022)
The Central Dark Matter Fraction of Massive Early-Type Galaxies
in Frontiers in Astronomy and Space Sciences
| 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 |