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
Shipp N
(2019)
Proper Motions of Stellar Streams Discovered in the Dark Energy Survey
in The Astrophysical Journal
Salvadori S
(2019)
Probing the existence of very massive first stars
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
Walsh S
(2019)
Optimizing the choice of analysis method for all-sky searches for continuous gravitational waves with Einstein@Home
in Physical Review D
Hughes S
(2022)
Optimisation of the WEAVE target assignment algorithm
Carrera R.
(2019)
Open clusters through the eyes of WEAVE
in Highlights on Spanish Astrophysics X
Casamiquela L
(2019)
OCCASO - III. Iron peak and a elements of 18 open clusters. Comparison with chemical evolution models and field stars
in Monthly Notices of the Royal Astronomical Society
Koppelman H
(2019)
Multiple retrograde substructures in the Galactic halo: A shattered view of Galactic history
in Astronomy & Astrophysics
Cescutti G
(2022)
MINCE I. Presentation of the project and of the first year sample
in Astronomy & Astrophysics
Lodieu N
(2019)
Metallicity, temperature, and gravity scales of M subdwarfs ,
in Astronomy & Astrophysics
Sinigaglia F
(2022)
Mapping the Three-dimensional Lya Forest Large-scale Structure in Real and Redshift Space*
in The Astrophysical Journal
Conroy C
(2019)
Mapping the Stellar Halo with the H3 Spectroscopic Survey
in The Astrophysical Journal
Middleton K
(2018)
Low-level control software for the WEAVE spectrograph
Gürkan G
(2019)
LoTSS/HETDEX: Optical quasars I. Low-frequency radio properties of optically selected quasars
in Astronomy & Astrophysics
Mahatma V
(2019)
LoTSS DR1: Double-double radio galaxies in the HETDEX field
in Astronomy & Astrophysics
Hale C
(2019)
LOFAR observations of the XMM-LSS field
in Astronomy & Astrophysics
Schultheis Mathias
(2016)
Large surveys of Galactic populations with the new WEAVE faciligy
in Galactic Surveys: New Results on Formation, Evolution, Structure and Chemical Evolution of the Milky Way
Schultheis Mathias
(2016)
Large surveys of Galactic populations with the new WEAVE faciligy
in Galactic Surveys: New Results on Formation, Evolution, Structure and Chemical Evolution of the Milky Way
Cenarro A
(2019)
J-PLUS: The Javalambre Photometric Local Universe Survey
in Astronomy & Astrophysics
Ness M
(2019)
In the Galactic Disk, Stellar [Fe/H] and Age Predict Orbits and Precise [X/Fe]
in The Astrophysical Journal
Haines T
(2019)
Implications of a Time-varying Galactic Potential for Determinations of the Dynamical Surface Density
in The Astrophysical Journal
Garavito-Camargo N
(2019)
Hunting for the Dark Matter Wake Induced by the Large Magellanic Cloud
in The Astrophysical Journal
Khoperskov S
(2020)
Hic sunt dracones: Cartography of the Milky Way spiral arms and bar resonances with Gaia Data Release 2
in Astronomy & Astrophysics
Marasco A
(2019)
HALOGAS: the properties of extraplanar HI in disc galaxies
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 |