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
Middleton K
(2018)
Antireflective coatings for the red camera of WEAVE spectrograph
Fariña C
(2018)
Design of the observation queue scheduler for WEAVE on the WHT
Carrasco E
(2018)
The WEAVE observatory control system
Middleton K
(2018)
The polishing of WEAVE spectrograph collimator mirror
Terlevich R
(2018)
WEAVE spectrograph cameras: the polishing of the spherical lenses
Leung H
(2018)
Deep learning of multi-element abundances from high-resolution spectroscopic data
in Monthly Notices of the Royal Astronomical Society
Zanutta A
(2018)
VPHGs for WEAVE: design, manufacturing and characterization
Terrett D
(2018)
First lab results of the WEAVE fibre positioner system
Casalta J
(2018)
The WEAVE prime focus correction: from design to integration
Middleton K
(2018)
Low-level control software for the WEAVE spectrograph
Aguado D
(2019)
The Pristine survey - VI. The first three years of medium-resolution follow-up spectroscopy of Pristine EMP star candidates
in Monthly Notices of the Royal Astronomical Society
Bianchini P
(2019)
Exploring the Outskirts of Globular Clusters: The Peculiar Kinematics of NGC 3201
in The Astrophysical Journal
Garavito-Camargo N
(2019)
Hunting for the Dark Matter Wake Induced by the Large Magellanic Cloud
in The Astrophysical Journal
Xiang M
(2019)
Abundance Estimates for 16 Elements in 6 Million Stars from LAMOST DR5 Low-Resolution Spectra
in The Astrophysical Journal Supplement Series
Oliva E
(2019)
Experimental characterization of modal noise in multimode fibers for astronomical spectrometers
in Astronomy & Astrophysics
Carrera R.
(2019)
Open clusters through the eyes of WEAVE
in Highlights on Spanish Astrophysics X
Ting Y
(2019)
The Payne : Self-consistent ab initio Fitting of Stellar Spectra
in The Astrophysical Journal
Duncan K
(2019)
The LOFAR Two-metre Sky Survey IV. First Data Release: Photometric redshifts and rest-frame magnitudes
in Astronomy & Astrophysics
Gómez F
(2019)
Footprints of the Sagittarius dwarf galaxy in the Gaia data set
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
Gentile Fusillo N
(2019)
A Gaia Data Release 2 catalogue of white dwarfs and a comparison with SDSS
in Monthly Notices of the Royal Astronomical Society
| 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 |