Fig. 7 from Dynamically Close Galaxy Pairs and Merger Rate Evolution in the CNOC2 Redshift Survey

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Dynamically Close Galaxy Pairs and Merger Rate Evolution in the CNOC2 Redshift Survey

Authors: D. R. Patton, C. J. Pritchet, R. G. Carlberg, R. O. Marzke, H. K. C. Yee, P. B. Hall, H. Lin, S. L. Morris, M. Sawicki, C. W. Shepherd, and G. D. Wirth

Patton et al. 2002 The Astrophysical Journal 565 208.

Provider: AAS Journals

Caption: Fig. 7.

Pair statistics are computed for a range in ﹩\Delta v^{\mathrm{max}\,}﹩, for both ﹩r^{\mathrm{max}\,}_{p}=20﹩ h⁻¹ kpc (left panels) and ﹩r^{\mathrm{max}\,}_{p}=50﹩ h⁻¹ kpc (right panels). Error bars are computed using the Jackknife technique. Both N_c and L_c are cumulative statistics; hence, measurements in successive bins are not independent.

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