WEAVE Detectors Completion

Lead Research Organisation: Liverpool John Moores University
Department Name: Astrophysics Research Institute

Abstract

This grant is to complete the production and commissioning of 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 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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Miller J (2019) Searching for the shadows of giants: characterizing protoclusters with line of sight Lyman-a absorption in Monthly Notices of the Royal Astronomical Society

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Gómez F (2019) Footprints of the Sagittarius dwarf galaxy in the Gaia data set in Monthly Notices of the Royal Astronomical Society

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Childress M (2017) OzDES multifibre spectroscopy for the Dark Energy Survey: 3-yr results and first data release in Monthly Notices of the Royal Astronomical Society

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Rosslowe C (2017) A deep near-infrared spectroscopic survey of the Scutum-Crux arm for Wolf-Rayet stars? in Monthly Notices of the Royal Astronomical Society

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Morabito L (2017) Investigating the unification of LOFAR-detected powerful AGN in the Boötes field in Monthly Notices of the Royal Astronomical Society

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Pittordis C (2019) Testing modified gravity with wide binaries in Gaia DR2 in Monthly Notices of the Royal Astronomical Society

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Mateu C (2017) Predictions for the detection of tidal streams with Gaia using great-circle methods in Monthly Notices of the Royal Astronomical Society

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

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Morrison S (2019) Probing inhomogeneity in the helium ionizing UV background 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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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

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

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Sharma S (2019) The K2-HERMES Survey: age and metallicity of the thick disc 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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Minchev I (2019) Yule-Simpson's paradox in Galactic Archaeology in Monthly Notices of the Royal Astronomical Society

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

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Ichikawa K (2017) Foreground effect on the J-factor estimation of classical dwarf spheroidal galaxies in Monthly Notices of the Royal Astronomical Society

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Laporte C (2019) Stellar disc streams as probes of the Galactic potential and satellite impacts in Monthly Notices of the Royal Astronomical Society

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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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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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Duncan K (2018) Photometric redshifts for the next generation of deep radio continuum surveys - I. Template fitting 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 Scientific Exploitation of WEAVE
Sectors Other

URL https://www.ing.iac.es/astronomy/instruments/weave/weaveinst.html