Fig. 2.
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Sample of mock images of galaxies at three different redshifts (z = 1.50, 1.15, and 0.80) is shown. The SDSS g-, r-, and i-band fluxes (mapped to blue, green, and red, respectively) are used to construct the color images. Based on stellar population and dust information, NEWCLUSTER successfully reproduces a wide variety of galaxy types.
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