WEAVE Detectors Interim
Lead Research Organisation:
Liverpool John Moores University
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
Kushniruk I
(2019)
Disentangling the Arcturus stream
in Astronomy & Astrophysics
Koposov S
(2020)
Discovery of a nearby 1700 km s-1 star ejected from the Milky Way by Sgr A*
in Monthly Notices of the Royal Astronomical Society
Fariña C
(2018)
Design of the observation queue scheduler for WEAVE on the WHT
Leung H
(2018)
Deep learning of multi-element abundances from high-resolution spectroscopic data
in Monthly Notices of the Royal Astronomical Society
Maiolino R
(2019)
De re metallica: the cosmic chemical evolution of galaxies
in The Astronomy and Astrophysics Review
Veras D
(2020)
Constraining planet formation around 6-8 M? stars
in Monthly Notices of the Royal Astronomical Society
Hughes S
(2022)
Calibration at elevation of the WEAVE fibre positioner
Blomqvist M
(2019)
Baryon acoustic oscillations from the cross-correlation of Ly a absorption and quasars in eBOSS DR14
in Astronomy & Astrophysics
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
| 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 |