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hlasco
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###################
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# Global parameters
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###################
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# Virial velocity of the galaxy [km/s]
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v200 0.0
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# Virial mass of the galaxy [1e10 Msol]
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# Overrides the v200 parameter
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m200 112.127
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# Halo spin parameter
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lambda 0.04
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# Refinement level of the potential grid
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level_coarse 7
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# Refinement level of the plane plane density grid
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level_grid_mid_dens 7
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# Refinement level of the turbulence grid
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level_grid_turb 7
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# Refinement level of the gaussian field grid
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level_grid_dens_fluct 7
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# Size of the potential grid [kpc]
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boxsize1 320.0
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boxsize2 160.0
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boxsize3 80.0
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boxsize4 40.0
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boxsize5 20.0
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boxsize6 10.0
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boxsize7 5.0
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# Dispersion for the Gaussian field fluctuations
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dens_fluct_sigma 0.50
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# Physical injection scale of the random field fluctuations [kpc]
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dens_fluct_scale_inj 2.00
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# Physical dissipation scale of the random field fluctuations [kpc]
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dens_fluct_scale_diss 0.25
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dens_fluct_seed 1212
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# Seed for the random number generator
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seed 1246
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# Switch to MCMC ntry algorithm to position particles for a value > 1
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mcmc_ntry 1
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# Number of iterations to reach hydrostatic equilibrium (zero to deactivate)
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hydro_eq_niter 3
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#######################
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# Components parameters
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#######################
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#######################
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# Component 1: Halo
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#######################
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# Fraction of the virial mass in the component 1
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mass_frac1 0.9578424465115449
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# Number of particles for the component 1
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npart1 1000000
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# Target mass of individual particles [Msol]
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#part_mass1 2e6
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# Number of particles for the potential computation
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npart_pot1 2000000
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# Target mass of individual particles for potential computation [Msol]
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#part_mass_pot1 1e6
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# Component 1 density model
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# Available models:
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# 1 = Exponential disk + sech-z profile
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# 2 = Myamoto-Nagai profile
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# 3 = Exponential disk + exponential-z profile
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# 4 = Hernquist profile
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# 5 = Plummer profile
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# 6 = Jaffe profile
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# 7 = Isothermal profile
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# 8 = NFW profile
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# 9 = Burkert
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# 10 = Einasto profile
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# 11 = Mestel profile
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# 12 = Kalnajs profile
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# 13 = Sersic profile
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# 14 = Toomre-Kuzmin profile
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# 15 = Uniform profile
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# 16 = Pseudo-isothermal profile
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model1 8
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# Scale length of the density profile [kpc]
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scale_length1 1.0
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# Core radius in the density profile [kpc]
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rcore1 0.
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# Concentration parameter
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# if positive, the scale length is recomputed to match the concentration
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# the concentration parameter of an NFW halo with a mass M200*mass_frac
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concentration1 10
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# Gravitational softening for the poisson solver [kpc]
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softening1 0.3
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# Component 1 radial density cut [kpc]
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cut1 0.0
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# Component 1 thickness parameters
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flatx1 1.00
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flaty1 1.00
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flatz1 1.00
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# Gaussian step for the MCMC Metropolis-Hasting particle postionning algorithm,
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# expressed in units of the component scale length. Default value is 0.5.
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mcmc_step1 0.50
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# Maximum velocity for the component 1 particles in expressed in units of escape velocity
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vmax_esc1 5.0
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# Particles type (GADGET format -- 0=Gas,1=Halo,2=Disk,3=Bulge,4=Stars)
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type1 1
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# Radius at which the density profile should have the exact same
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# value as the NFW profile with the previously defined concentration
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# and with a mass M200*mass_frac [kpc]
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radius_nfw1 -1.0
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# Cut the density function in the Jeans equation integration
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jeans_mass_cut1 0
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# Compute component velocity (debug option)
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compute_vel1 1
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# Number of integral of motion for the Jeans equations
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# 0 = Do not use Jeans equation for sigma_r and sigma_z (model specidifed by sigmar_model and sigmaz_model)
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# 1 = Spherically symmetric Jeans equation
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# 2 = Jeans equations with 2 integrals of motion
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# 3 = Jeans equations with 3 integrals of motion (solved on a 2D grid in the r-z plane)
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jeans_dim1 1
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# Method for streaming velocity computation
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# 0 = - User defined fixed fraction of the circular velocity profile (stream_fraction keyword)
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# 1 = Bullock 2001 - Streaming velocity profile following the cumulative mass profile
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# 2 = Springel 1999 - Streaming velocity profile following is a fixed fraction of the rotation curve
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# 3 = - Solid Body rotation
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stream_method1 1
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# Streaming fraction of the component 1 (only for steam_method=4)
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stream_fraction1 0.00
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# Alpha coefficient for the generalized normal distribution [Gaussian=2.0]
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# for the random generation of velocities
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ggd_beta1 2.0
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# Minimum acceptance for the MCMC chain
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accept_min1 0.95
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# Maximum acceptance for the MCMC chain
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accept_max1 0.99
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################################
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# Component 2: Thin stellar disk
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################################
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mass_frac2 0.03066166043860979
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npart2 1000000
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npart_pot2 2000000
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model2 3
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# If the value is zero and the particle type is not 1 the size is determined using the spin conservation
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# (Fitting formula from Mo, Mao & White 1998)
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scale_length2 3.43218
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cut2 30.
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flatz2 0.1
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mcmc_step2 0.3
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type2 1
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stream_fraction2 1.00
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# Epicycle approximation in the Jeans equations
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epicycle2 1
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# Minimal value for the Toomre parameter
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Q_lim2 1.5
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# Fixed value for the Toomre parameter
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Q_fixed2 0.0
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# Additional term for the Toomre parameter
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Q_boost2 0.0
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# Past constant Star Formation Rate [Msol/yr]
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# Negative value recomptes the SFR according to Bouché et al. 2010
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SFR2 -1.
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# Minimum age of the stars [Myr]
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min_age2 50.
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# Metallicity of the stars [Zsolar]
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metal2 0.02041
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# Gaussian fluctuations in the density field
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dens_fluct2 0
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# Use the density cut during the Jeans equation integration
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jeans_mass_cut2 1
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compute_vel2 1
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###########################
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# Component 3: Gaseous disk
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###########################
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mass_frac3 0.007663631417945721
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npart3 1000000
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npart_pot3 2000000
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model3 3
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scale_length3 3.43218
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cut3 30.
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flatz3 0.1
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mcmc_step3 0.15
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type3 0
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stream_fraction3 1.00
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metal3 0.02041
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# Metallicity follows density gradient
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metal_gradient3 0
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# Temperature of the gas particles [K]
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t_init3 1e4
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# Turbulent velocity dispersion [km/s]
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turb_sigma3 10.0
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# Turbulence injection scale [kpc]
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turb_scale_inj3 0.34
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# Turbulence dissipation scale [kpc]
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turb_scale_diss3 0.005
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# Seed for the turbulent gaussian field
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turb_seed3 1234
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# Compute hydrostatic equilibrium
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hydro_eq3 0
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# Gaussian step for the MCMC Metropolis-Hasting particle postionning algorithm
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# within the hydro equilibrium algorithm
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mcmc_step_hydro3 0.3
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compute_vel3 1
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# Polytropic index for the gas (1 = isothermal)
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gamma_poly3 1.0
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############################
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# Component 4: Stellar bulge
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############################
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mass_frac4 0.0038322616318995422
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npart4 125000
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npart_pot4 250000
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model4 4
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scale_length4 0.343218
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flatz4 0.80
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mcmc_step4 0.3
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type4 1
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stream_fraction4 1.
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min_age4 50.
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metal4 0.02041
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Q_lim4 1.5
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epicycle4 1
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compute_vel4 1
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