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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

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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

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Salvadori S (2019) Probing the existence of very massive first stars in Monthly Notices of the Royal Astronomical Society

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Hale C (2019) LOFAR observations of the XMM-LSS field in Astronomy & Astrophysics

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Zavarygin E (2019) A search for cosmological anisotropy using the Lyman alpha forest from SDSS quasar spectra in Monthly Notices of the Royal Astronomical Society

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Lewis J. (2019) The WEAVE Core Processing System at CASU in Highlights on Spanish Astrophysics X

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Bianchini P (2019) Exploring the Outskirts of Globular Clusters: The Peculiar Kinematics of NGC 3201 in The Astrophysical Journal Letters

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Cenarro A (2019) J-PLUS: The Javalambre Photometric Local Universe Survey in Astronomy & Astrophysics

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Kushniruk I (2019) Disentangling the Arcturus stream in Astronomy & Astrophysics

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Xiang M (2019) Abundance Estimates for 16 Elements in 6 Million Stars from LAMOST DR5 Low-Resolution Spectra in The Astrophysical Journal Supplement Series

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Ting ? Y (2019) The Payne: Self-consistent ab initio Fitting of Stellar Spectra in The Astrophysical Journal

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Hayden M (2020) The GALAH survey: chemodynamics of the solar neighbourhood in Monthly Notices of the Royal Astronomical Society

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Everall A (2020) seestar: Selection functions for spectroscopic surveys of the Milky Way in Monthly Notices of the Royal Astronomical Society

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Veras D (2020) Constraining planet formation around 6-8 M? stars in Monthly Notices of the Royal Astronomical Society

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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

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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

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Manser C (2020) The frequency of gaseous debris discs around white dwarfs in Monthly Notices of the Royal Astronomical Society

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Tortora C (2022) The Central Dark Matter Fraction of Massive Early-Type Galaxies in Frontiers in Astronomy and Space Sciences

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Cescutti G (2022) MINCE I. Presentation of the project and of the first year sample in Astronomy & Astrophysics

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Esposito M (2022) Weighing cosmic structures with clusters of galaxies and the intergalactic medium in Monthly Notices of the Royal Astronomical Society

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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

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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

 
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