| A large, not to mention heavy, cryostat, from Pulse Ray Machining arrives at UVa - July 27, 2010. | ||
| John and Fred install "Fold 1" on an empty optical bench - August 30, 2010 (left). All optics installed but no fibers or arrays yet - October 28, 2010 (right) | ![]() |
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| Warm testing with a video rate InGaAs (H-band) camera - October 28, 2010. | ![]() |
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| Fiber installation - mid-December 2010. | ||
| Full system (left) and array mosaic installation (right) - December 24, 2010. | ||
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| Krypton lamp - January 17, 2011. Left image shows all three focal planes with red (1.7um) on the left, blue (1.5um) on the right. The right image zooms on a spectral line near the center of the array. | ![]() |
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| Solar spectrum - January 17, 2011. | ![]() |
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| Extracted solar spectrum. For comparison see this plot of absorption from atmospheric constituents. | ![]() |
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| Calibration setup: Integrating sphere, fiber bundles, telecentric coupling lens, and light sources. | ||
| Littrow ghost in krypton spectrum (left). Complete ThArNe spectrum (right) | ![]() |
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| A physically curved slit becomes straight in the images - with small curvature for each (physically linear) v-groove block. | ![]() |
John Wilson et al.
18 Jan 2011