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
Ham S. J.
(2016)
Towards an Integrated Model of the WEAVE Performance
in Multi-Object Spectroscopy in the Next Decade: Big Questions, Large Surveys, and Wide Fields
Smith D. J. B.
(2016)
The WEAVE-LOFAR Survey
in SF2A-2016: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics
Balcells M
(2015)
The WEAVE spectrograph on the WHT: plans for radial velocity and chemistry surveys of the northern and equatorial Milky Way
in EAS Publications Series
Peralta De Arriba L.
(2019)
The WEAVE Quick-Look GUI
in Highlights on Spanish Astrophysics X
Casalta J
(2018)
The WEAVE prime focus correction: from design to integration
Carrasco E
(2018)
The WEAVE observatory control system
Famaey B.
(2016)
The WEAVE disk dynamics survey
in SF2A-2016: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics
Lewis J.
(2019)
The WEAVE Core Processing System at CASU
in Highlights on Spanish Astrophysics X
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
Orenstein B
(2019)
The redshift distribution of infrared-faint radio sources
in Monthly Notices of the Royal Astronomical Society
| 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 |