Fig 1 (IMAGE)

Kavli Institute for the Physics and Mathematics of the Universe

Fig 1

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Figure 1. Results from the observation of a field of NGC 1980. This is the ISR (instrument signature removal)-processed, sky-unsubtracted CCD image from a 300-second exposure of the red camera of the Spectrograph Module 1, clearly showing a number of spectra from the stars on and through the fibers.

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PFS Project

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