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| Original file line number | Diff line number | Diff line change |
|---|---|---|
| @@ -0,0 +1,149 @@ | ||
| global: | ||
| { | ||
| #Output prefix. Output will be in prefix_<node ID>.<fits/txt> | ||
| prefix_out= "examples/simple/out"; | ||
| #Output format. Select HDF5, FITS or ASCII | ||
| output_format= "FITS"; | ||
| #Output Gaussian overdensity field at z=0? | ||
| output_density= true | ||
| #Path to power spectrum at z=0. Power spectrum file must | ||
| #be in CAMB format: k (h/Mpc), P(k) (Mpc/h)^3. | ||
| pk_filename= "examples/simple/Pk_CAMB_test.dat" | ||
| #This redshift range also defines the size of the box | ||
| z_min= 0.001 | ||
| z_max= 0.450 | ||
| #RNG seed note that output will depend on number of nodes, etc not only | ||
| #on the RNG seed | ||
| seed= 1003 | ||
| #Set to true if you want to generate the theory prediction for the 3D power spectrum | ||
| #of the different tracers. | ||
| write_pred=false | ||
| #Intervals of redshift at which the prediction will be produced. | ||
| pred_dz=0.1 | ||
| #If write_pred is true, set this to true if you just want to generate the prediction | ||
| #and then exit. This is also useful if you want to inspect the memory requirements | ||
| #before a run. | ||
| just_write_pred= true | ||
| } | ||
|
|
||
| field_par: | ||
| { | ||
| #Extra Gaussian smoothing scale [Mpc/h] (set to a | ||
| #negative value if you don't want any smoothing) | ||
| r_smooth= 5. | ||
| #Do you want to smooth the Newtonian potential as well? | ||
| smooth_potential= true | ||
| #Will use a Cartesian grid with n_grid^3 cells | ||
| n_grid= 256 | ||
| #Density field type | ||
| # 0-lognormal | ||
| # 1-1LPT | ||
| # 2-1LPT | ||
| dens_type= 1 | ||
| #If dens_type==1 or 2, buffer size (fraction per particle) | ||
| lpt_buffer_fraction= 0.6 | ||
| #If dens_type==1 or 2, scheme to interpolate particle | ||
| #positions into a grid | ||
| # 0-NGP | ||
| # 1-CIC | ||
| # 2-TSC | ||
| lpt_interp_type= 1 | ||
| #Set to 1 if you want to output the LPT particle positions | ||
| output_lpt= 0 | ||
| } | ||
|
|
||
| cosmo_par: | ||
| { | ||
| #Non-relativistic matter | ||
| omega_M= 0.3 | ||
| #Dark energy | ||
| omega_L= 0.7 | ||
| #Baryons | ||
| omega_B= 0.05 | ||
| #Hubble parameter (in units of 100 km/s/Mpc) | ||
| h= 0.7 | ||
| #Dark energy equation of state | ||
| w= -1.0 | ||
| #Primordial scalar spectral index, used only to extrapolate | ||
| #P(k) at low k end (-3 used at high k end) | ||
| ns= 0.96 | ||
| #Power spectrum normalization. The input power spectrum will be | ||
| #renormalized to this sigma8 | ||
| sigma_8= 0.803869 | ||
| } | ||
|
|
||
| #For each galaxy population, create a section called srcsX, starting with X=1 | ||
| srcs1: | ||
| { | ||
| #Path to N(z) file. Should contain two columns | ||
| # 1-> z, 2-> dN(z)/dz*dOmega | ||
| # with dN/dzdOmega in units of deg^-2 | ||
| nz_filename= "examples/simple/Nz_test.txt" | ||
| #Path to bias file. Should contain two columns | ||
| # 1-> z, 2-> b(z) | ||
| bias_filename= "examples/simple/Bz_test.txt" | ||
| #Do you want to include shear ellipticities? | ||
| include_shear= true | ||
| #Do you want to store line-of-sight skewers for each object? | ||
| store_skewers= true | ||
| #You can also store the Gaussian density field (instead of the non-Gaussian one) | ||
| #This is false by default. | ||
| gaussian_skewers= false | ||
| } | ||
|
|
||
| srcs2: | ||
| { | ||
| nz_filename= "examples/simple/Nz2_test.txt" | ||
| bias_filename= "examples/simple/Bz2_test.txt" | ||
| include_shear= false | ||
| store_skewers= true | ||
| } | ||
|
|
||
| #For each intensity mapping species, create a section called imapX, | ||
| #starting with X=1 | ||
| imap1: | ||
| { | ||
| #Tabulated background temperature as a function of redshift | ||
| tbak_filename= "examples/simple/Tz_test.txt" | ||
| #Tabulated linear bias as a function of redshift | ||
| bias_filename= "examples/simple/Bz_test.txt" | ||
| #Frequency bands in which to output maps. Should contain 2 columns: | ||
| # 1-> nu_ini, 2-> nu_end | ||
| freq_list= "examples/simple/nuTable.txt" | ||
| #Rest-frame frequency of this species (in the same units as the | ||
| #frequencies in freq_list). | ||
| freq_rest= 1420.405 | ||
| #HEALPix resolution parameter. | ||
| nside= 64 | ||
| } | ||
|
|
||
| #Include a section entitled kappa if you want to generate maps | ||
| #of the lensing convergence at specific redshifts. | ||
| kappa: | ||
| { | ||
| #Redshifts at which maps should be generated | ||
| z_out= [0.4] | ||
| nside= 64 | ||
| } | ||
|
|
||
| #Include a section entitled isw if you want to generate maps | ||
| #of the ISW effect (time derivative of the gravitational potential). | ||
| isw: | ||
| { | ||
| z_out= [0.4] | ||
| nside= 64 | ||
| } | ||
|
|
||
| #This section is needed if using the fast lensing method | ||
| lensing: | ||
| { | ||
| # Maximum Nside used for the lensing shells. | ||
| nside= 256 | ||
| # Select number of slices. | ||
| n_lensing= 11 | ||
| # Select spacing type ("r" or "log(1+z)"). | ||
| spacing_type= "r" | ||
| # Set to true if you want to output the different | ||
| # lensing shells. | ||
| write=false | ||
| } |
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