| def runcommand(cosmology='WMAP5'): |
| """pass""" |
| Mi = [100000000.0, 1000000000.0, 10000000000.0] |
| zi = 0 |
| print('Concentrations for haloes of mass %s at z=%s' % (Mi, zi)) |
| output = commah.run(cosmology=cosmology, zi=zi, Mi=Mi) |
| print(output['c'].flatten()) |
| Mi = [100000000.0, 1000000000.0, 10000000000.0] |
| zi = 0 |
| print('Concentrations for haloes of mass %s at z=%s' % (Mi, zi)) |
| output, cosmo = commah.run(cosmology=cosmology, zi=zi, Mi=Mi, retcosmo=True) |
| print(output['c'].flatten()) |
| print(cosmo) |
| Mi = 2000000000000.0 |
| z = [0, 0.5, 1, 1.5, 2, 2.5] |
| output = commah.run(cosmology=cosmology, zi=0, Mi=Mi, z=z) |
| for zval in z: |
| print('M(z=0)=%s has c(z=%s)=%s' % (Mi, zval, output[output['z'] == zval]['c'].flatten())) |
| Mi = 2000000000000.0 |
| zi = [0, 0.5, 1, 1.5, 2, 2.5] |
| output = commah.run(cosmology=cosmology, zi=zi, Mi=Mi) |
| for zval in zi: |
| print('M(z=%s)=%s has concentration %s' % (zval, Mi, output[(output['zi'] == zval) & (output['z'] == zval)]['c'].flatten())) |
| Mi = 200000000000000.0 |
| zi = 6 |
| output = commah.run(cosmology=cosmology, zi=zi, Mi=Mi) |
| print('Concentrations for haloes of mass %s at z=%s' % (Mi, zi)) |
| print(output['c'].flatten()) |
| print('Mass variance sigma of haloes of mass %s at z=%s' % (Mi, zi)) |
| print(output['sig'].flatten()) |
| print('Fluctuation for haloes of mass %s at z=%s' % (Mi, zi)) |
| print(output['nu'].flatten()) |
| Mi = [100000000.0, 1000000000.0, 10000000000.0] |
| zi = [0] |
| z = [0, 0.5, 1, 1.5, 2, 2.5] |
| output = commah.run(cosmology=cosmology, zi=zi, Mi=Mi, z=z) |
| for Mval in Mi: |
| print('dM/dt for halo of mass %s at z=%s across redshift %s is: ' % (Mval, zi, z)) |
| print(output[output['Mi'] == Mval]['dMdt'].flatten()) |
| M = [100000000.0] |
| z = [0, 0.5, 1, 1.5, 2, 2.5] |
| print('Halo Mass History for z=0 mass of %s across z=%s' % (M, z)) |
| output = commah.run(cosmology=cosmology, zi=0, Mi=M, z=z) |
| print(output['Mz'].flatten()) |
| M = [100000000.0, 1000000000.0, 10000000000.0] |
| z = [0] |
| print('Formation Redshifts for haloes of mass %s at z=%s' % (M, z)) |
| output = commah.run(cosmology=cosmology, zi=0, Mi=M, z=z) |
| for Mval in M: |
| print(output[output['Mi'] == Mval]['zf'].flatten()) |
| return 'Done' |
