Raw Data, 1.0 micron
Jim Bell, Cornell University
This page contains calibration and test images for the paper "Compositional variability of the Serenitatis/Tranquillitatis region of the Moon from telescopic multispectral imaging and spectroscopy" , by Jim Bell and B. Ray Hawke, submitted to Icarus.
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Here are teeny-weeny previews of the available images. Click on the blue highlighted name of any one to see a full-resolution view...
First, here are examples of the raw data and the calibration data for the 1.0 micron filter observations...
Raw Data, 1.0 micron
Flatfield image at 1.0 micron
Sky image at 1.0 micron
(The striping is an artifact from shrinking this image down to this teeny weeny size; it does not show up in the full-
resolution view)
Dark (bias) image at 1.0 micron
(Again, the striping is an artifact)
Next, some examples of ratio images to examine possible problems with the 1.0 micron data by using the 0.96 micron image in ratios instead...
Ratio image: 1.0 / 0.4 microns (Fig. 2b)
Ratio image: 0.96 / 0.4 microns for comparison with previous
Ratio image: 1.0 / 0.73 microns (Fig. 2c)
Ratio image: 0.96 / 0.73 microns for comparison with previous
Ratio image: 1.0 / 0.9 microns (Fig. 2d)
Ratio image: 0.96 / 0.9 microns for comparison with previous
Last Modified by Jim Bell on 26 February 1996.