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
Carrera R.
(2019)
Open clusters through the eyes of WEAVE
in Highlights on Spanish Astrophysics X
Hughes S
(2022)
Optimisation of the WEAVE target assignment algorithm
Walsh S
(2019)
Optimizing the choice of analysis method for all-sky searches for continuous gravitational waves with Einstein@Home
in Physical Review D
Morrison S
(2019)
Probing inhomogeneity in the helium ionizing UV background
in Monthly Notices of the Royal Astronomical Society
Salvadori S
(2019)
Probing the existence of very massive first stars
in Monthly Notices of the Royal Astronomical Society
Shipp N
(2019)
Proper Motions of Stellar Streams Discovered in the Dark Energy Survey
in The Astrophysical Journal
Hardcastle M
(2019)
Radio-loud AGN in the first LoTSS data release The lifetimes and environmental impact of jet-driven sources
in Astronomy & Astrophysics
Mooney S
(2019)
Revisiting the Fanaroff-Riley dichotomy and radio-galaxy morphology with the LOFAR Two-Metre Sky Survey (LoTSS)
in Monthly Notices of the Royal Astronomical Society
Abbott R
(2022)
Search of the early O3 LIGO data for continuous gravitational waves from the Cassiopeia A and Vela Jr. supernova remnants
in Physical Review D
Miller J
(2019)
Searching for the shadows of giants: characterizing protoclusters with line of sight Lyman-a absorption
in Monthly Notices of the Royal Astronomical Society
Das P
(2020)
seestar: Selection functions for spectroscopic surveys of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Monari G
(2019)
Signatures of the resonances of a large Galactic bar in local velocity space
in Astronomy & Astrophysics
Japelj J
(2019)
Simulating MOS science on the ELT: Ly a forest tomography
in Astronomy & Astrophysics
Fratta M
(2023)
Spectroscopic follow-up of a subset of the Gaia /IPHAS catalogue of Ha-excess sources
in Monthly Notices of the Royal Astronomical Society
Laporte C
(2019)
Stellar disc streams as probes of the Galactic potential and satellite impacts
in Monthly Notices of the Royal Astronomical Society
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
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
Widmark A
(2019)
The dynamical matter density in the solar neighbourhood inferred from Gaia DR1
in Monthly Notices of the Royal Astronomical Society
Croston J
(2019)
The environments of radio-loud AGN from the LOFAR Two-Metre Sky Survey (LoTSS)
in Astronomy & Astrophysics
| 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 |