Focal enlarger
In front of the device, at the Cassegrain focus, is mounted a small enlarger, transforming F/8 into
F/14.5; that is why each 100 µm fibre subtends 0.4" on the sky. This allows to take into account the focal ratio degradation within the fibres. At the exit, the beam is collected by the F/8 MOS collimator without additional optics. So, the spectral resolution for a given grism is about the same as could be obtained with a 100 µm width slit (0.7" on the sky) in classical mode. Since the sampling of the fibre's images by the CCD is correct, we did not attempt to conserve the "étendue" of the beam by adding more optics. Fibre bundle
This is the "heart" of the device, the part that changes the geometry of the focal image into a pseudo-slit. MOS/ARGUS slide
On the MOS/ARGUS slide, encoding by micro-switches is similar to those of other MOS slides, with 4 positions:
The bundle of fibres is spread into a sheet within the thickness of the slide and arranged to form a pseudo-slit. Then, a total reflection prism directs the output beam from this "slit" toward the MOS collimator. It is understandable that, in this configuration, the "slit" seen by the collimator must be horizontal.
The total reflection prism has dimensions 10 x 10 x 90 mm. The free aperture toward collimator is 6 x 85 mm. With a total of 622 fibres (594 active + spacers), the theoretical length of the "slit" is 77.75 mm and we do see some vignetting at its edges. The number of rows that can be safely used is 21; the field of view given above is for this number.