| HTML | ||
|---|---|---|
| ||
Instrument Page
The conceptual design of the instrument is driven by the WEAVE science requirements, as defined by the Science Team, and translated to technical requirements by the Project and Instrument Scientists. At the time of writing the requirements call for a dual-beam spectrograph with the following characteristics:
| HTML |
|---|
<center> |
| Borderless table | |||||||||||||||||||||||||||||||||||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
|
| HTML |
|---|
</center> |
The philosophy behind the construction of WEAVE is to keep it simple but effective. Thus the design exploits the use of COTS (Commercial Off-The Shelf) components which not only reduces project costs and risks but provides an attractive solution for maintaining the instrument throughout its lifecycle.
The Positioner
Pick-and-place technology will be used to position the fibre buttons onto a plate using a commercially available X-Y gantry. A computer simulation shows the complexity of weaving 920 960 fibres to acquire their targets. Each green line represents a single fibre and the purple beads are the magnetic buttons. In this particular example there are 8300 fibre crossings.
The solid circle shows the science field diameter, Green fibres are guide stars, yellow are calibration stars, blue are sky and black are targets.
At the edge of the field are the fibre retractors (originally designed for GYES) that tension and protect the individual fibres. Each retractor holds four six fibres and the buttons are seated at the entrance to the retractors as illustrated in the following pictures.
The fibre positioning mechanism is a twin-based system of fibres, retractors and buttons etc. The arrangement is s uch such that 1000 the fibre-assemblies are positioned at each end of the rotating assembly (blue) also known as the tumbler. This fits inside a gantry with a pair of robotic gripper grippers that places place the buttons on the plate. This arrangement allows for reconfiguration of the top plate whilst the bottom plate is used for observing.
The upper plate is configured by the robots while the lower plate sees the image plane of the telescope and diverts light from each target to the spectrograph. Fieldplate B also holds 20 small integral field units that feed an alternate input slit. A fourth slit is fed by a single large integral field unit (red box) that can be moved into the focal plane by the tumbler.
The Spectrograph
Fibres from the positioner are fed to the dual-beam spectrograph which incorporates a dichroic at ~600nm and has two volume phase holographic gratingsa grating exchange mechanism that provides either low- or high-resolution observations in each arm. The spectrograph will be housed in GHRIL.
