Fig. 23 from Distributions of Galaxy Spectral Types in the Sloan Digital Sky Survey

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Distributions of Galaxy Spectral Types in the Sloan Digital Sky Survey

Authors: C. W. Yip, A. J. Connolly, A. S. Szalay, T. Budavári, M. SubbaRao, J. A. Frieman, R. C. Nichol, A. M. Hopkins, D. G. York, S. Okamura, J. Brinkmann, I. Csabai, A. R. Thakar, M. Fukugita, and Ž. Ivezić

Yip et al. 2004 The Astronomical Journal 128 585.

Provider: AAS Journals

Caption: Fig. 23.

Difference in the classification for the whole galaxy and the inner 3^{﹩\arcsec﹩} region as a function of ﹩z/ z_{\mathrm{max}\,}﹩ from the reddest (a) to the bluest (f) galaxies. In each subfigure the galaxies are of sizes 0–100 kpc (solid line), 10–15 kpc (dotted line) and 30–35 kpc (dashed line).

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