Fig. 11 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. 11.

Means of all KL‐reconstructed spectra in different ranges of (﹩\phi ^{s}_{\mathrm{KL}\,},\,\phi ^{e}_{\mathrm{KL}\,},\,\theta ^{s}_{\mathrm{KL}\,},\,\theta ^{e}_{\mathrm{KL}\,}﹩) (the bounding boxes are the same as those in Fig. 9). The first three eigenspectra are used in the reconstruction. The continua and most of the line features are in excellent agreement with those of the mean spectra shown in Fig. 9.

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