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
Kushniruk I
(2017)
Kinematic structures of the solar neighbourhood revealed by Gaia DR1/TGAS and RAVE
in Astronomy & Astrophysics
Kushniruk I
(2019)
Disentangling the Arcturus stream
in Astronomy & Astrophysics
Kumari N
(2018)
O/H-N/O: the curious case of NGC 4670
in Monthly Notices of the Royal Astronomical Society
Kraljic K
(2022)
Forecasts for WEAVE-QSO: 3D clustering and connectivity of critical points with Lyman- a tomography
in Monthly Notices of the Royal Astronomical Society
Koppelman H
(2019)
Multiple retrograde substructures in the Galactic halo: A shattered view of Galactic history
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
Khoperskov S
(2020)
Hic sunt dracones: Cartography of the Milky Way spiral arms and bar resonances with Gaia Data Release 2
in Astronomy & Astrophysics
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
Johnston K
(2017)
Disk Heating, Galactoseismology, and the Formation of Stellar Halos
in Galaxies
Jofré P
(2019)
Accuracy and Precision of Industrial Stellar Abundances
in Annual Review of Astronomy and Astrophysics
| 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 |