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The WASP Project and the SuperWASP Cameras

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Figure

Fig. 2.—SuperWASP-S instrument, with eight cameras mounted. The fieldof view of the instrument isfor a color version of this figure ∼482 deg2
Figure 4 is a plot ofragainstr, which reveals that for un-21blended stellar images, the two wing-to-core ratios are relatedby a constant scaling factor

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