WEAVE Detectors Completion
Lead Research Organisation:
Liverpool John Moores University
Department Name: Astrophysics Research Institute
Abstract
This grant is to complete the production and commissioning of 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 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
Figueras F
(2017)
Outskirts of Galaxies
Crnojevic D
(2017)
Outskirts of Galaxies
Walsh S
(2019)
Optimizing the choice of analysis method for all-sky searches for continuous gravitational waves with Einstein@Home
in Physical Review D
Hughes S
(2022)
Optimisation of the WEAVE target assignment algorithm
Carrera R.
(2019)
Open clusters through the eyes of WEAVE
in Highlights on Spanish Astrophysics X
Williams A
(2017)
On the run: mapping the escape speed across the Galaxy with SDSS
in Monthly Notices of the Royal Astronomical Society
Jean-Baptiste I
(2017)
On the kinematic detection of accreted streams in the Gaia era: a cautionary tale
in Astronomy & Astrophysics
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
Kalfountzou E
(2017)
Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power
in Monthly Notices of the Royal Astronomical Society
Storm N
(2023)
Observational constraints on the origin of the elements - VII. NLTE analysis of Y ii lines in spectra of cool stars and implications for Y as a Galactic chemical clock
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 | Scientific Exploitation of WEAVE |
Sectors | Other |
URL | https://www.ing.iac.es/astronomy/instruments/weave/weaveinst.html |