def plotcommand(cosmology='WMAP5', plotname=None): """pass""" xarray = 10 ** np.arange(1, 15, 0.2) yval = 'c' zarray = np.arange(0, 5, 0.5) xtitle = 'Halo Mass (M$_{sol}$)' ytitle = 'Concentration' linelabel = 'z=' fig = plt.figure() ax = fig.add_subplot(111) ax.set_xlabel(xtitle) ax.set_ylabel(ytitle) plt.ylim([2, 30]) colors = cm.rainbow(np.linspace(0, 1, len(zarray))) for zind, zval in enumerate(zarray): output = commah.run(cosmology=cosmology, zi=zval, Mi=xarray) yarray = output[yval].flatten() ax.plot(xarray, yarray, label=linelabel + str(zval), color=colors[zind]) ax.plot(xarray, commah.commah.cduffy(zval, xarray), color='black') ax.set_xscale('log') ax.set_yscale('log') leg = ax.legend(loc=1) leg.get_frame().set_alpha(0) leg.get_frame().set_edgecolor('white') for label in leg.get_texts(): label.set_fontsize('small') for label in leg.get_lines(): label.set_linewidth(4) if plotname: fig.tight_layout(pad=0.2) print("Plotting to '%s_CM_relation.png'" % plotname) fig.savefig(plotname + '_CM_relation.png', dpi=fig.dpi * 5) else: plt.show() xarray = 10 ** np.arange(0, 1, 0.05) - 1 yval = 'c' zarray = 10 ** np.arange(6, 14, 2) xtitle = 'Redshift' ytitle = 'NFW Concentration' linelabel = 'log$_{10}$ M$_{z}$(M$_{sol}$)=' fig = plt.figure() ax = fig.add_subplot(111) ax.set_xlabel(xtitle) ax.set_ylabel(ytitle) colors = cm.rainbow(np.linspace(0, 1, len(zarray))) for zind, zval in enumerate(zarray): output = commah.run(cosmology=cosmology, zi=xarray, Mi=zval) yarray = output[yval].flatten() ax.plot(xarray, yarray, label=linelabel + '{0:.1f}'.format(np.log10(zval)), color=colors[zind]) leg = ax.legend(loc=1) leg.get_frame().set_alpha(0) leg.get_frame().set_edgecolor('white') for label in leg.get_texts(): label.set_fontsize('small') for label in leg.get_lines(): label.set_linewidth(4) if plotname: fig.tight_layout(pad=0.2) print("Plotting to '%s_Cz_relation.png'" % plotname) fig.savefig(plotname + '_Cz_relation.png', dpi=fig.dpi * 5) else: plt.show() xarray = 10 ** np.arange(0, 1, 0.05) - 1 yval = 'zf' zarray = 10 ** np.arange(6, 14, 2) xtitle = 'Redshift' ytitle = 'Formation Redshift' linelabel = 'log$_{10}$ M$_{z}$(M$_{sol}$)=' fig = plt.figure() ax = fig.add_subplot(111) ax.set_xlabel(xtitle) ax.set_ylabel(ytitle) colors = cm.rainbow(np.linspace(0, 1, len(zarray))) for zind, zval in enumerate(zarray): output = commah.run(cosmology=cosmology, zi=xarray, Mi=zval) yarray = output[yval].flatten() ax.plot(xarray, yarray, label=linelabel + '{0:.1f}'.format(np.log10(zval)), color=colors[zind]) leg = ax.legend(loc=2) leg.get_frame().set_alpha(0) leg.get_frame().set_edgecolor('white') for label in leg.get_texts(): label.set_fontsize('small') for label in leg.get_lines(): label.set_linewidth(4) if plotname: fig.tight_layout(pad=0.2) print("Plotting to '%s_zfz_relation.png'" % plotname) fig.savefig(plotname + '_zfz_relation.png', dpi=fig.dpi * 5) else: plt.show() xarray = 10 ** np.arange(0, 1, 0.05) - 1 yval = 'dMdt' zarray = 10 ** np.arange(10, 14, 0.5) xtitle = 'log$_{10}$ (1+z)' ytitle = 'log$_{10}$ Accretion Rate M$_{sol}$ yr$^{-1}$' linelabel = 'log$_{10}$ M$_z$(M$_{sol}$)=' fig = plt.figure() ax = fig.add_subplot(111) ax.set_xlabel(xtitle) ax.set_ylabel(ytitle) colors = cm.rainbow(np.linspace(0, 1, len(zarray))) cosmo = commah.getcosmo(cosmology) for zind, zval in enumerate(zarray): output = commah.run(cosmology=cosmology, zi=xarray, Mi=zval, com=False, mah=True) yarray = output[yval].flatten() ax.plot(np.log10(xarray + 1.0), np.log10(yarray), label=linelabel + '{0:.1f}'.format(np.log10(zval)), color=colors[zind]) semianalytic_approx = 71.6 * (zval / 1000000000000.0) * (cosmo['h'] / 0.7) * (-0.24 + 0.75 * (xarray + 1)) * np.sqrt(cosmo['omega_M_0'] * (xarray + 1) ** 3 + cosmo['omega_lambda_0']) ax.plot(np.log10(xarray + 1), np.log10(semianalytic_approx), color='black') leg = ax.legend(loc=2) leg.get_frame().set_alpha(0) leg.get_frame().set_edgecolor('white') for label in leg.get_texts(): label.set_fontsize('small') for label in leg.get_lines(): label.set_linewidth(4) if plotname: fig.tight_layout(pad=0.2) print("Plotting to '%s_dMdtz_relation.png'" % plotname) fig.savefig(plotname + '_dMdtz_relation.png', dpi=fig.dpi * 5) else: plt.show() xarray = 10 ** np.arange(10, 14, 0.5) yval = 'dMdt' zarray = np.arange(0, 5, 0.5) xtitle = 'Halo Mass M$_{sol}$' ytitle = 'Accretion Rate M$_{sol}$ yr$^{-1}$' linelabel = 'z=' fig = plt.figure() ax = fig.add_subplot(111) ax.set_xlabel(xtitle) ax.set_ylabel(ytitle) colors = cm.rainbow(np.linspace(0, 1, len(zarray))) for zind, zval in enumerate(zarray): output = commah.run(cosmology=cosmology, zi=zval, Mi=xarray, com=False, mah=True) yarray = output[yval].flatten() ax.plot(xarray, yarray, label=linelabel + str(zval), color=colors[zind]) ax.set_xscale('log') ax.set_yscale('log') leg = ax.legend(loc=2) leg.get_frame().set_alpha(0) leg.get_frame().set_edgecolor('white') for label in leg.get_texts(): label.set_fontsize('small') for label in leg.get_lines(): label.set_linewidth(4) if plotname: fig.tight_layout(pad=0.2) print("Plotting to '%s_MAH_M_relation.png'" % plotname) fig.savefig(plotname + '_MAH_M_relation.png', dpi=fig.dpi * 5) else: plt.show() xarray = 10 ** np.arange(10, 14, 0.5) yval = 'dMdt' zarray = np.arange(0, 5, 0.5) xtitle = 'Halo Mass M$_{sol}$' ytitle = 'Specific Accretion Rate yr$^{-1}$' linelabel = 'z=' fig = plt.figure() ax = fig.add_subplot(111) ax.set_xlabel(xtitle) ax.set_ylabel(ytitle) colors = cm.rainbow(np.linspace(0, 1, len(zarray))) for zind, zval in enumerate(zarray): output = commah.run(cosmology=cosmology, zi=zval, Mi=xarray, mah=True, com=False) yarray = output[yval].flatten() ax.plot(xarray, yarray / xarray, label=linelabel + str(zval), color=colors[zind]) ax.set_xscale('log') ax.set_yscale('log') leg = ax.legend(loc=1) leg.get_frame().set_alpha(0) leg.get_frame().set_edgecolor('white') for label in leg.get_texts(): label.set_fontsize('small') for label in leg.get_lines(): label.set_linewidth(4) if plotname: fig.tight_layout(pad=0.2) print("Plotting to '%s_specificMAH_M_relation.png'" % plotname) fig.savefig(plotname + '_specificMAH_M_relation.png', dpi=fig.dpi * 5) else: plt.show() xarray = 10 ** np.arange(0, 1, 0.05) - 1 yval = 'Mz' zarray = 10 ** np.arange(10, 14, 0.5) xtitle = 'Redshift' ytitle = 'M(z) (M$_{sol}$)' linelabel = 'log$_{10}$ M$_{0}$(M$_{sol}$)=' fig = plt.figure() ax = fig.add_subplot(111) ax.set_xlabel(xtitle) ax.set_ylabel(ytitle) colors = cm.rainbow(np.linspace(0, 1, len(zarray))) for zind, zval in enumerate(zarray): output = commah.run(cosmology=cosmology, zi=0, Mi=zval, z=xarray) yarray = output[yval].flatten() ax.plot(xarray, yarray, label=linelabel + '{0:.1f}'.format(np.log10(zval)), color=colors[zind]) ax.set_yscale('log') leg = ax.legend(loc=1) leg.get_frame().set_alpha(0) leg.get_frame().set_edgecolor('white') for label in leg.get_texts(): label.set_fontsize('small') for label in leg.get_lines(): label.set_linewidth(4) if plotname: fig.tight_layout(pad=0.2) print("Plotting to '%s_Mzz_relation.png'" % plotname) fig.savefig(plotname + '_Mzz_relation.png', dpi=fig.dpi * 5) else: plt.show() xarray = 10 ** np.arange(0, 1, 0.02) - 1 yval = 'Mz' zarray = 10 ** np.arange(10, 14, 0.5) xtitle = 'Redshift' ytitle = 'log$_{10}$ M(z)/M$_{0}$' linelabel = 'log$_{10}$ M$_{0}$(M$_{sol}$)=' fig = plt.figure() ax = fig.add_subplot(111) ax.set_xlabel(xtitle) ax.set_ylabel(ytitle) colors = cm.rainbow(np.linspace(0, 1, len(zarray))) for zind, zval in enumerate(zarray): output = commah.run(cosmology=cosmology, zi=0, Mi=zval, z=xarray) yarray = output[yval].flatten() ax.plot(xarray, np.log10(yarray / zval), label=linelabel + '{0:.1f}'.format(np.log10(zval)), color=colors[zind]) leg = ax.legend(loc=3) leg.get_frame().set_alpha(0) leg.get_frame().set_edgecolor('white') for label in leg.get_texts(): label.set_fontsize('small') for label in leg.get_lines(): label.set_linewidth(4) if plotname: fig.tight_layout(pad=0.2) print("Plotting to '%s_MzM0z_relation.png'" % plotname) fig.savefig(plotname + '_MzM0z_relation.png', dpi=fig.dpi * 5) else: plt.show() return 'Done'