Fig. 9 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. 9.

Mean of all the observed spectra in different ranges of (﹩\phi ^{s}_{\mathrm{KL}\,},\,\phi ^{e}_{\mathrm{KL}\,},\,\theta ^{s}_{\mathrm{KL}\,},\,\theta ^{e}_{\mathrm{KL}\,}﹩), with the classification angles being (a) (7.5, 20, 86, 92), (b) (5, 6, 80, 100), (c) (0, 2, 80, 100), (d) (−12, −8, 80, 100), (e) (−40, −30, 80, 100), and (f) (−60, −40, 120, 135).

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