WEAVE Detectors Interim
Lead Research Organisation:
Liverpool John Moores University
Department Name: Astrophysics Research Institute
Abstract
Start detector procurement for WEAVE
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 a 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
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
Williams W
(2019)
The LOFAR Two-metre Sky Survey III. First data release: Optical/infrared identifications and value-added catalogue
in Astronomy & Astrophysics
Howes L
(2019)
Estimating stellar ages and metallicities from parallaxes and broadband photometry: successes and shortcomings
in Astronomy & Astrophysics
Mints A
(2019)
Ensemble age inversions for large spectroscopic surveys
in Astronomy & Astrophysics
Gürkan G
(2019)
LoTSS/HETDEX: Optical quasars I. Low-frequency radio properties of optically selected quasars
in Astronomy & Astrophysics
Blomqvist M
(2019)
Baryon acoustic oscillations from the cross-correlation of Ly a absorption and quasars in eBOSS DR14
in Astronomy & Astrophysics
Kushniruk I
(2019)
Disentangling the Arcturus stream
in Astronomy & Astrophysics
Sabater J
(2019)
The LoTSS view of radio AGN in the local Universe The most massive galaxies are always switched on
in Astronomy & Astrophysics
Cescutti G
(2022)
MINCE I. Presentation of the project and of the first year sample
in Astronomy & Astrophysics
Shimwell T
(2019)
The LOFAR Two-metre Sky Survey II. First data release
in Astronomy & Astrophysics
Cenarro A
(2019)
J-PLUS: The Javalambre Photometric Local Universe Survey
in Astronomy & Astrophysics
Costantin L
(2019)
A few StePS forward in unveiling the complexity of galaxy evolution: light-weighted stellar ages of intermediate-redshift galaxies with WEAVE
in Astronomy & Astrophysics
Oliva E
(2019)
Experimental characterization of modal noise in multimode fibers for astronomical spectrometers
in Astronomy & Astrophysics
Hale C
(2019)
LOFAR observations of the XMM-LSS field
in Astronomy & Astrophysics
Mahatma V
(2019)
LoTSS DR1: Double-double radio galaxies in the HETDEX field
in Astronomy & Astrophysics
Gilbert James
(2015)
Verification of commercial motor performance for WEAVE at the William Herschel Telescope
in arXiv e-prints
Jofré P
(2019)
Accuracy and Precision of Industrial Stellar Abundances
in Annual Review of Astronomy and Astrophysics
Walton Nicholas
(2015)
Gaia, PLATO and WEAVE: A Powerful combination for Exoplanet Characterisation
in AAS/Division for Extreme Solar Systems Abstracts
Description | This is an interim grant to begin work on the development of detectors for the WEAVE spectrograph. The main element of this work is to come in the final work package now underway - this funding was used to develop the project to conceptual design and make a downpayment on array production. |
Exploitation Route | Experiments with pseudo-dummy and dummy CCD outputs to reduce common read house. |
Sectors | Digital/Communication/Information Technologies (including Software) |
Description | Collaboration with Isaac Newton Group |
Organisation | Isaac Newton Group of Telescopes (ING) |
Country | Spain |
Sector | Academic/University |
PI Contribution | Joint development of detector systems |
Collaborator Contribution | Expertise in operations and use |
Impact | Development in ongoing, with completion of the new system due in 2018. |
Start Year | 2014 |
Description | Collaboration with University of Oxford |
Organisation | University of Oxford |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Scientific Expertise, Access to telescope time |
Collaborator Contribution | Scientific Expertise, Financial Contribution |
Impact | Collaboration on followup of LOFAR radio transients starting in early 2014. |
Start Year | 2014 |