The following images show our progress in obtaining a spectrum. Each image from the Imaging CCD is paired with the correlating image from the Tracking CCD. Our final goal is to obtain a crisp spectra with the source centered on the slit in the tracking CCD.

An image of a star on the tracking CCD. The slit can be seen running vertically in the center of the image.

An image captured using the Imaging CCD. Note this looks nothing like a spectra.

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In this image the source was centered on the slit.

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The following is a progression of images captured by the spectrometer in conjunction with the sources position on the Tracking CCD. Note the change in quality of the spectrum due to the position of the source.

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The next sequence of images shows spectra of light passed through different color filters.

No Filter.

Blue Filter.

Green Filter.

Red Filter.

Yellow Filter.

These are not actually spectra gathered off of the diffraction reflector. They are instead patterns of diffuse light from within the spectrometer housing. It may look like the filters are creating different spectra, and that would be almost correct. The filters are blocking certain wavelengths from even entering the spectrometer thus there is no diffuse light of those wavelengths.

Position of source for filtered spectra.

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The following images were captured using a Helium-Neon Laser.

We finally have something that looks like a spectrum of an actual star. While this is not our ultimate goal, it is a step in the right direction. Now we must attach the spectrometer to the telescope and attempt to obtain a true spectra from a real star. If we can do this, then we will have corrected the problems that were in the spectrometer and can use it in scientific work.

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