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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. 18.

Frequency distribution of φKL. The three modeled Gaussian populations are shown (dotted lines), with the peaks corresponding to early late‐type through to intermediate late‐type. The solid line is the sum of the three modeled populations.

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