Fig. 3 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. 3.

KL‐repaired spectra, linearly interpolated (solid line) and mean‐interpolated (dashed line), in the gap regions of the unmasked spectrum as in Fig. 2 (after 20 iterations). The inset is Tr(f^R(m)f⁰f^R(m)) as a function of iteration step for both cases.

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