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
Ting Y
(2017)
Measuring 14 Elemental Abundances with R = 1800 LAMOST Spectra
in The Astrophysical Journal
Monreal-Ibero A
(2017)
Measuring diffuse interstellar bands with cool stars Improved line lists to model background stellar spectra?
in Astronomy & Astrophysics
Lodieu N
(2019)
Metallicity, temperature, and gravity scales of M subdwarfs ,
in Astronomy & Astrophysics
Cescutti G
(2022)
MINCE I. Presentation of the project and of the first year sample
in Astronomy & Astrophysics
Burden A
(2017)
Mitigating the impact of the DESI fiber assignment on galaxy clustering
in Journal of Cosmology and Astroparticle Physics
Thévenin F
(2017)
Modern Geometric Methods of Distance Determination
in Space Science Reviews
Koppelman H
(2019)
Multiple retrograde substructures in the Galactic halo: A shattered view of Galactic history
in Astronomy & Astrophysics
Kumari N
(2018)
O/H-N/O: the curious case of NGC 4670
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
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 |