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
Monreal-Ibero A
(2017)
Measuring diffuse interstellar bands with cool stars Improved line lists to model background stellar spectra?
in Astronomy & Astrophysics
Simpson C
(2017)
Extragalactic radio surveys in the pre-Square Kilometre Array era.
in Royal Society open science
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
Geier S
(2017)
The population of hot subdwarf stars studied with Gaia I. The catalog of known hot subdwarf stars?
in Astronomy & Astrophysics
Thévenin F
(2017)
Modern Geometric Methods of Distance Determination
in Space Science Reviews
Childress M
(2017)
OzDES multifibre spectroscopy for the Dark Energy Survey: 3-yr results and first data release
in Monthly Notices of the Royal Astronomical Society
Jofré P
(2017)
Gaia FGK benchmark stars: opening the black box of stellar element abundance determination
in Astronomy & Astrophysics
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
Sesar B
(2017)
Machine-learned Identification of RR Lyrae Stars from Sparse, Multi-band Data: The PS1 Sample
in The Astronomical Journal
Pato M
(2017)
galkin: A new compilation of Milky Way rotation curve data
in SoftwareX
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 |