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Grism

From SharedSkies

A combination of transmission diffraction grating and wedge prism (GRISM) may be placed in the optical path of a telescope to form an image of a spectrum. We have designed one for use with the CDK125 and one of the Manta CCD video cameras. A schematic of the optical system is shown below.


Grism.jpg


On the left, a 140 mm focal length negative achromat collimates the beam from the CDK telescope before it reaches the focal plane. At f/6.8 the beam for a point source on axis is 20.5 mm in diameter at this lens. Immediately after the lens the beam enters an anti-reflection coated wedge prism that deflects it 6 degrees off axis. This approximately compensates for the diffraction angle of a 150 groove/mm grating blazed at 580 nm that is close to the second prism face. The prism and the grating are mounted in independent cells and are oriented so that the net deflection is minimized. In practice, the intense first order blaze wavelength is on axis and the weak zeroth order is at the edge of the field after diffraction. Following the grating, a 100 mm focal length positive achromat focuses the spectrum on a new focal plane that is coincident with the detector.


Grism assembly sm.jpg


We assembled this device from a modified 2-inch Barlow lens assembly, adding Thorlabs holders for the prism, grating, and positive lens by mounting cells on an interior stop. This makes a compact rugged unit that inserts in the optical system between the telescope and the camera with minimal changes in the focal plane configuration. With a Manta G033B camera the spectra cover 4.8 A/pixel (0.48 nm/pixel) and span the visible spectrum.

The test spectrum of Vega shown below is the sum of 60 frames from a Manta G033B CCD camera integrating for 0.1 seconds/frame. Red is on the right, and the hydrogen Balmer alpha line is the absorption feature on the right side. Other lines of the Balmer series extend into the blue on the left.


Vega.jpg


A sum across this image perpendicular to the direction of dispersion gives a quantitative spectrum. For this example the wavelength scale was calibrated from Balmer alpha and beta.


Vega spectrum sm.jpg