Erratum: The build-up of the colour-magnitude relation as a function of environment
Masaomi Tanaka, T. Kodama, N. Arimoto, Sadanori Okamura, Keiichi Umetsu, Kazuhiro Shimasaku, Ichi Tanaka, Takatoshi Yamada · Monthly Notices of the Royal Astronomical Society · 2006
Total LFs in RXJ0153 (top), CL0016 (middle), and SDSS (bottom). Note that no contamination subtraction is performed here. The left-hand panels show the error ellipse for each LF. The solid and dashed contours show 1σ and 2σ errors. The right-hand panels show LFs along with the best-fitting Schechter functions. The error bars are based on the Poisson statistics only. Rest-frame LFs in various environments in RXJ0153 (top left), CL0016 (top right), and the SDSS (bottom). The left-hand panels in each plot show the 1σ error ellipses of the Schechter fits. The solid and dashed lines represent red and blue galaxies defined in Fig. 8 (of the original paper). The filled points and open squares show the best-fitting parameters for red and blue LFs, respectively. The right-hand panels show LFs. The filled and open symbols represent red and blue galaxies. The solid and dashed lines, respectively, show the best-fitting Schechter functions for red and blue galaxies. The statistical contamination subtraction is carried out here.