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
Peralta De Arriba L.
(2019)
The WEAVE Quick-Look GUI
in Highlights on Spanish Astrophysics X
Casalta J
(2018)
The WEAVE prime focus correction: from design to integration
Carrasco E
(2018)
The WEAVE observatory control system
Lewis J.
(2019)
The WEAVE Core Processing System at CASU
in Highlights on Spanish Astrophysics X
Ciuca I
(2018)
The vertical metallicity gradients of mono-age stellar populations in the Milky Way with the RAVE and Gaia data
in Monthly Notices of the Royal Astronomical Society
Griv E
(2017)
The Spiral Arm Segments of the Galaxy within 3 kpc from the Sun: A Statistical Approach
in The Astrophysical Journal
Li T
(2019)
The southern stellar stream spectroscopic survey (S5): Overview, target selection, data reduction, validation, and early science
in Monthly Notices of the Royal Astronomical Society
Orenstein B
(2019)
The redshift distribution of infrared-faint radio sources
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
Cornwell D
(2023)
The probability of identifying the cosmic web environment of galaxies around clusters motivated by the Weave Wide Field Cluster Survey
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 |