# StepWise Maximum Likelihood estimates of the # galaxy stellar mass function. # # As shown in Fig. 18 of "2dFGRS: Near-Infrared Galaxy Luminosity Functions" # Cole etal (The 2dFGRS Team) 2001, MNRAS in press (astro-ph/0012429). # # The first column is the log_10 of the Mass locked up in stars # and stellar remnants in units of Msol/h^2 # # The second column, Phi(M), is the number density of galaxies with # this stellar mass and has units of number per (Mpc/h)^3 per log_10 Mass. # # The third column is the uncertainty in Phi in the same units. # # 1) Kennicutt IMF # log M Phi(M) error # 8.963 0.01172 0.01663 9.063 0.04243 0.02623 9.163 0.03416 0.01801 9.263 0.03006 0.01314 9.363 0.03334 0.01107 9.463 0.04205 0.01038 9.563 0.02753 0.00668 9.663 0.02702 0.00549 9.763 0.02305 0.004226 9.863 0.02196 0.003532 9.963 0.02213 0.003068 10.06 0.01774 0.002278 10.16 0.01913 0.001972 10.26 0.0177 0.001561 10.36 0.01459 0.001167 10.46 0.01111 0.0008403 10.56 0.00815 0.0006107 10.66 0.005617 0.0004308 10.76 0.003393 0.0002895 10.86 0.00208 0.0001994 10.96 0.001067 0.0001245 11.06 0.0005946 8.223e-05 11.16 0.0002745 4.872e-05 11.26 0.0001046 2.594e-05 11.36 2.766e-05 1.108e-05 11.46 9.505e-06 5.653e-06 11.56 2.047e-06 2.379e-06 11.66 6.87e-07 1.355e-06 # # 2) Salpeter IMF # log M Phi(M) error # 9.057 0.01367 0.01045 9.157 0.02413 0.01345 9.257 0.02055 0.01131 9.357 0.03005 0.01127 9.457 0.03252 0.009202 9.557 0.02869 0.006723 9.657 0.03099 0.005559 9.757 0.03298 0.004724 9.857 0.02673 0.003427 9.957 0.02509 0.002733 10.06 0.02028 0.002023 10.16 0.0193 0.001701 10.26 0.01862 0.001447 10.36 0.01618 0.001124 10.46 0.01494 0.0008945 10.56 0.01608 0.0007676 10.66 0.01303 0.0005685 10.76 0.0106 0.0004226 10.86 0.007398 0.0002969 10.96 0.005502 0.0002189 11.06 0.00329 0.0001454 11.16 0.002024 9.999e-05 11.26 0.001131 6.568e-05 11.36 0.0005555 4.016e-05 11.46 0.0002899 2.568e-05 11.56 9.868e-05 1.258e-05 11.66 3.729e-05 6.63e-06 11.76 8.455e-06 2.578e-06 11.86 2.215e-06 1.198e-06 11.96 5.571e-07 5.839e-07