Frédéric Sayède

TL;DR: WEAVE as mentioned in this paper is a multi-object and multi-IFU facility utilizing a new 2-degree prime focus field of view at the WHT, with a buffered pick-and-place positioner system hosting 1000 multiobject (MOS) fibres, 20 integral field units, or a single large IFU for each observation.

TL;DR: WEAVE as mentioned in this paper is a multi-object and multi-IFU facility utilizing a new 2-degree prime focus field of view at the WHT, with a buffered pick-and-place positioner system hosting 1000 multiobject (MOS) fibres, 20 integral field units, or a single large IFU for each observation.

TL;DR: In this paper, the authors present the final design of the WEAVE next-generation spectroscopy facility for the William Herschel Telescope (WHT), together with a status update on the details of manufacturing, integration and overall project schedule now that all the major fabrication contracts are in place.

TL;DR: In this paper, the authors proposed a multi-object 3D spectrograph with multi-conjugate adaptive optics in large fields to estimate the turbulent volume from sets of natural guide stars, by optimizing the correction to several and discrete small areas of few arcsec2 selected in a large field (Nasmyth field of 25 arcmin).

TL;DR: FALCON as discussed by the authors is a next generation spectrograph including multiple small integral field units (IFUs) which can be deployed within a large field of view such as that of VLT/GIRAFFE.