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
Jofré P
(2017)
Climbing the cosmic ladder with stellar twins in RAVE with Gaia
in Monthly Notices of the Royal Astronomical Society
Bosma A
(2017)
Outskirts of Galaxies
Catalán-Torrecilla C
(2017)
Star Formation in the Local Universe from the CALIFA Sample. II. Activation and Quenching Mechanisms in Bulges, Bars, and Disks
in The Astrophysical Journal
Crnojevic D
(2017)
Outskirts of Galaxies
Jean-Baptiste I
(2017)
On the kinematic detection of accreted streams in the Gaia era: a cautionary tale
in Astronomy & Astrophysics
Thévenin F
(2017)
Modern Geometric Methods of Distance Determination
in Space Science Reviews
González M
(2017)
Phase-space structures and stellar populations in the star-forming region NGC 2264
in Monthly Notices of the Royal Astronomical Society
González-Morales A
(2017)
Unbiased constraints on ultralight axion mass from dwarf spheroidal galaxies
in Monthly Notices of the Royal Astronomical Society
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
Buist H
(2017)
Behaviour of streams in angle and frequency spaces in different potentials
in Astronomy & 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 |