Astro-Physics 1100GTOCP4 German...
Note u> that provides a spectrograph resolution of 0.1 Angstroms per pixel (pixel by 9 microns) then 10 times higher b> of the resolution offered by the best of spectroscopes Sbig.
LHIRES III therefore it offers potential results and much more professional. < p> With commercial telescopes (openings from about 25cm) you can get high resolution spectra of stars to the 9th magnitude.
Comes with grating 2400 lines (with telescope 8 "" f / 10, with pixel ccd 9 micron produces a resolution of 0.012nm 0.1Angstrom or in pixels) and the latter is easily replaceable (various models from 150ll / mm to 1200 ll / mm) to fit the resolution to the object type: planetary nebulae, comets, sun, etc.
The system can be connected to any type of refractor telescope is it, Mewlon, SCT or another and accepts as a CCD camera systems is that SLR cameras.
The walls of the slot are constituted by optical planes of precision and allow one side to position with accuracy the object of interest and the other to use the sides of the slit as optical driving off-axis.
E ' also installed a system for off-axis: the slit, mounted on a support, is polished so that the steel sides thereof become a mirror of re-sending of the light thus allowing an off-axis (for example during spectroscopy faint objects). Spectroscopy standard allows so to drive directly in the field of recovery, taking the object being analyzed by the gap that remains visible in the center of the field itself.
The result is a tool of the highest quality, without compromise, designed to spectroscopy visual or photographic of many celestial objects thanks to the interchangeable gratings and slits.
Main applications: b> Diffraction gratings and slits available: b> Features: < / b>
Diffraction gratings and slits available: b> Features: < / b>
Features: < / b>
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