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
Ditrani F
(2023)
Stellar metallicity from optical and UV spectral indices: Test case for WEAVE-StePS
in Astronomy & Astrophysics
Tabernero H
(2019)
STEPAR: an automatic code to infer stellar atmospheric parameters
in Astronomy & Astrophysics
Caffau E
(2019)
Systematic investigation of chemical abundances derived using IR spectra obtained with GIANO
in Astronomy & Astrophysics
Pittordis C
(2019)
Testing modified gravity with wide binaries in Gaia DR2
in Monthly Notices of the Royal Astronomical Society
Ted Mackereth J
(2017)
The age-metallicity structure of the Milky Way disc using APOGEE
in Monthly Notices of the Royal Astronomical Society
Majewski S
(2017)
The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
in The Astronomical Journal
Laverick M
(2019)
The Belgian repository of fundamental atomic data and stellar spectra (BRASS) II. Quality assessment of atomic data for unblended lines in FGK stars
in Astronomy & Astrophysics
Tortora C
(2022)
The Central Dark Matter Fraction of Massive Early-Type Galaxies
in Frontiers in Astronomy and Space Sciences
Thomas G
(2022)
The Cetus-Palca stream: A disrupted small dwarf galaxy A prequel to the science possible with WEAVE with precise spectro-photometric distances
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 |