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
Erkal D
(2017)
A sharper view of Pal 5's tails: discovery of stream perturbations with a novel non-parametric technique
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
González M
(2017)
Phase-space structures and stellar populations in the star-forming region NGC 2264
in Monthly Notices of the Royal Astronomical Society
Monreal-Ibero A
(2017)
The Wolf-Rayet star population in the dwarf galaxy NGC 625
in Astronomy & Astrophysics
Traven G
(2017)
The Galah Survey: Classification and Diagnostics with t-SNE Reduction of Spectral Information
in The Astrophysical Journal Supplement Series
Majewski S
(2017)
The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
in The Astronomical Journal
Schönrich R
(2017)
Assessing distances and consistency of kinematics in Gaia/TGAS
in Monthly Notices of the Royal Astronomical Society
Ting Y
(2017)
Prospects for Measuring Abundances of >20 Elements with Low-resolution Stellar Spectra
in The Astrophysical Journal
Jean-Baptiste I
(2017)
On the kinematic detection of accreted streams in the Gaia era: a cautionary tale
in Astronomy & Astrophysics
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
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
González-Morales A
(2017)
Unbiased constraints on ultralight axion mass from dwarf spheroidal galaxies
in Monthly Notices of the Royal Astronomical Society
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
Gonzalez-Perez V
(2017)
The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5
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 |