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
Das P
(2020)
seestar: Selection functions for spectroscopic surveys of the Milky Way
in Monthly Notices of the Royal Astronomical Society
De Boer T
(2018)
The fall of the Northern Unicorn: tangential motions in the Galactic anticentre with SDSS and Gaia
in Monthly Notices of the Royal Astronomical Society
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
Deason A
(2018)
Cresting the wave: proper motions of the Eastern Banded Structure
in Monthly Notices of the Royal Astronomical Society
Debattista V
(2017)
Separation of stellar populations by an evolving bar: implications for the bulge of the Milky Way
in Monthly Notices of the Royal Astronomical Society
DomÃnguez-Tenreiro R
(2017)
The Radial Distribution of Mono-metallicity Populations in the Galactic Disk as Evidence for Two-phase Disk Formation
in The Astrophysical Journal
Du Mas Des Bourboux H
(2017)
Baryon acoustic oscillations from the complete SDSS-III Ly a -quasar cross-correlation function at z = 2.4
in Astronomy & Astrophysics
Duncan K
(2018)
Photometric redshifts for the next generation of deep radio continuum surveys - I. Template fitting
in Monthly Notices of the Royal Astronomical Society
Duncan K
(2019)
The LOFAR Two-metre Sky Survey IV. First Data Release: Photometric redshifts and rest-frame magnitudes
in Astronomy & Astrophysics