Calibration at elevation of the WEAVE fibre positioner
Sarah Hughes, Gavin Dalton, Kevin Dee, Don Carlos Abrams, Kevin, Middleton, Ian Lewis, David Terrett, Alfonso L. Aguerri, Marc Balcells,, Georgia Bishop, Piercarlo Bonifacio, Esperanza Carrasco, Scott Trager,, Antonella Vallenari

TL;DR
This paper details the calibration procedures and recent maintenance of the WEAVE fibre positioner, ensuring precise fibre placement for the spectrograph at the William Herschel Telescope.
Contribution
It provides an overview of calibration, maintenance, and modifications to improve the accuracy and reliability of the WEAVE fibre positioner system.
Findings
Fibre systems inspected and repaired
Flexure modifications implemented
Calibration procedures updated
Abstract
WEAVE is the new wide-field spectroscopy facility for the prime focus of the William Herschel Telescope in La Palma, Spain. Its fibre positioner is essential for the accurate placement of the spectrograph's 960 fibre multiplex. We provide an overview of the recent maintenance, flexure modifications, and calibration measurements conducted at the observatory prior to the final top-end assembly. This work ensures that we have a complete understanding of the positioner's behaviour as it changes orientation during observations. All fibre systems have been inspected and repaired, and the tumbler structure contains new clamps to stiffen both the internal beam and the retractor support disk onto which the field plates attach. We present the updated metrology procedures and results that will be verified on-sky.
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