Frequently Asked Questions

Type IV aberration corrected flat field & imaging gratings provide much better light collection efficiency and signal to noise ratio than traditional Type I Rowland circle concave gratings due to their large optical numerical aperture and correction from aberrations.

When an area detector such as a CCD is utilized, it is often possible to focus multiple sources onto the entrance slit and independently evaluate the spectrum from each source.

The dispersion range and wavelength range vary depending on the reference number, but they range from 4 to 36 nm/mm and 200 to 1170 nm, respectively.

They are designed to focus a spectrum onto a plane surface, making them ideal for use with linear or 2-D array detectors.

Yes, these gratings are interchangeable (same geometry of use).

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