WEAVE Detectors Main Grant
Lead Research Organisation:
Liverpool John Moores University
Department Name: Astrophysics Research Institute
Abstract
This grant is to produce 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 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
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
Kraljic K
(2022)
Forecasts for WEAVE-QSO: 3D clustering and connectivity of critical points with Lyman- a tomography
in Monthly Notices of the Royal Astronomical Society
Hughes S
(2022)
Optimisation of the WEAVE target assignment algorithm
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
Cornwell D
(2022)
Forecasting the success of the WEAVE Wide-Field Cluster Survey on the extraction of the cosmic web filaments around galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Cescutti G
(2022)
MINCE I. Presentation of the project and of the first year sample
in Astronomy & Astrophysics
Osorio Y
(2022)
Accurate Metallicities for Very Metal-poor Stars from the Ca ii Infrared Triplet
in The Astrophysical Journal
Sinigaglia F
(2022)
Mapping the Three-dimensional Lya Forest Large-scale Structure in Real and Redshift Space*
in The Astrophysical Journal
Hughes S
(2022)
Calibration at elevation of the WEAVE fibre positioner
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
Tortora C
(2022)
The Central Dark Matter Fraction of Massive Early-Type Galaxies
in Frontiers in Astronomy and Space Sciences
Esposito M
(2022)
Weighing cosmic structures with clusters of galaxies and the intergalactic medium
in Monthly Notices of the Royal Astronomical Society
Koposov S
(2020)
Discovery of a nearby 1700 km s-1 star ejected from the Milky Way by Sgr A*
in Monthly Notices of the Royal Astronomical Society
Veras D
(2020)
Constraining planet formation around 6-8 M? stars
in Monthly Notices of the Royal Astronomical Society
Zwitter T
(2020)
The GALAH survey: chemodynamics of the solar neighbourhood
in Monthly Notices of the Royal Astronomical Society
Khoperskov S
(2020)
Hic sunt dracones: Cartography of the Milky Way spiral arms and bar resonances with Gaia Data Release 2
in Astronomy & Astrophysics
Youakim K
(2020)
The Pristine Survey - VIII. The metallicity distribution function of the Milky Way halo down to the extremely metal-poor regime
in Monthly Notices of the Royal Astronomical Society
Venn K
(2020)
The Pristine survey - IX. CFHT ESPaDOnS spectroscopic analysis of 115 bright metal-poor candidate stars
in Monthly Notices of the Royal Astronomical Society
Amard L
(2020)
The Impact of Metallicity on the Evolution of the Rotation and Magnetic Activity of Sun-like Stars
in The Astrophysical Journal
Das P
(2020)
seestar: Selection functions for spectroscopic surveys of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Manser C
(2020)
The frequency of gaseous debris discs around white dwarfs
in Monthly Notices of the Royal Astronomical Society
Japelj J
(2019)
Simulating MOS science on the ELT: Ly a forest tomography
in Astronomy & Astrophysics
Pittordis C
(2019)
Testing modified gravity with wide binaries in Gaia DR2
in Monthly Notices of the Royal Astronomical Society
Lodieu N
(2019)
Metallicity, temperature, and gravity scales of M subdwarfs ,
in Astronomy & Astrophysics
Lewis J.
(2019)
The WEAVE Core Processing System at CASU
in Highlights on Spanish Astrophysics X
Shimwell T
(2019)
The LOFAR Two-metre Sky Survey II. First data release
in Astronomy & Astrophysics
Mancera Piña P
(2019)
The evolution of ultra-diffuse galaxies in nearby galaxy clusters from the Kapteyn IAC WEAVE INT Clusters Survey
in Monthly Notices of the Royal Astronomical Society
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
Haines T
(2019)
Implications of a Time-varying Galactic Potential for Determinations of the Dynamical Surface Density
in The Astrophysical Journal
Hale C
(2019)
LOFAR observations of the XMM-LSS field
in Astronomy & Astrophysics
Harris A
(2019)
A study of full space motions of outer Galactic disc A and F stars in two deep pencil beams
in Monthly Notices of the Royal Astronomical Society
Morrison S
(2019)
Probing inhomogeneity in the helium ionizing UV background
in Monthly Notices of the Royal Astronomical Society
Sharma S
(2019)
The K2-HERMES Survey: age and metallicity of the thick disc
in Monthly Notices of the Royal Astronomical Society
Silk J
(2019)
Exploring a new definition of the green valley and its implications
in Monthly Notices of the Royal Astronomical Society: Letters
Laporte C
(2019)
Stellar disc streams as probes of the Galactic potential and satellite impacts
in Monthly Notices of the Royal Astronomical Society
Cenarro A
(2019)
J-PLUS: The Javalambre Photometric Local Universe Survey
in Astronomy & Astrophysics
Hardcastle M
(2019)
Radio-loud AGN in the first LoTSS data release The lifetimes and environmental impact of jet-driven sources
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
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
Peralta De Arriba L.
(2019)
The WEAVE Quick-Look GUI
in Highlights on Spanish Astrophysics X
Carrera R.
(2019)
Open clusters through the eyes of WEAVE
in Highlights on Spanish Astrophysics X
Brauer K
(2019)
The Origin of r -process Enhanced Metal-poor Halo Stars In Now-destroyed Ultra-faint Dwarf Galaxies
in The Astrophysical Journal
Croston J
(2019)
The environments of radio-loud AGN from the LOFAR Two-Metre Sky Survey (LoTSS)
in Astronomy & Astrophysics
Jofré P
(2019)
Accuracy and Precision of Industrial Stellar Abundances
in Annual Review of Astronomy and Astrophysics
Bieth M
(2019)
The gravitational force field of the Galaxy measured from the kinematics of RR Lyrae in Gaia
in Monthly Notices of the Royal Astronomical Society
Thomas G
(2019)
Dwarfs or Giants? Stellar Metallicities and Distances from ugrizG Multiband Photometry
in The Astrophysical Journal
Marasco A
(2019)
HALOGAS: the properties of extraplanar HI in disc galaxies
in Astronomy & Astrophysics
Gürkan G
(2019)
LoTSS/HETDEX: Optical quasars I. Low-frequency radio properties of optically selected quasars
in Astronomy & Astrophysics
| Description | The WEAVE detector system was successfully built to specification and is now in use at the WHT. |
| Exploitation Route | Science exploitation |
| Sectors | Other |
| URL | https://www.ing.iac.es/astronomy/instruments/weave/weaveinst.html |
| 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 |