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
Bosma A
(2017)
Outskirts of Galaxies
Brauer K
(2019)
The Origin of r -process Enhanced Metal-poor Halo Stars In Now-destroyed Ultra-faint Dwarf Galaxies
in The Astrophysical Journal
Breedt E
(2017)
Using large spectroscopic surveys to test the double degenerate model for Type Ia supernovae
in Monthly Notices of the Royal Astronomical Society
Buist H
(2017)
Behaviour of streams in angle and frequency spaces in different potentials
in Astronomy & Astrophysics
Burden A
(2017)
Mitigating the impact of the DESI fiber assignment on galaxy clustering
in Journal of Cosmology and Astroparticle Physics
Caffau E
(2019)
Systematic investigation of chemical abundances derived using IR spectra obtained with GIANO
in Astronomy & Astrophysics
Carrasco E
(2018)
The WEAVE observatory control system
Carrera R.
(2019)
Open clusters through the eyes of WEAVE
in Highlights on Spanish Astrophysics X
Casalta J
(2018)
The WEAVE prime focus correction: from design to integration
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
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 |