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import shift and param file for planck
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soliket/clusters/input_files/test_binned_classy_sz_evaluate_alice25sept24.yaml
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output: /Users/boris/Work/CLASS-SZ/SO-SZ/SOLikeT/soliket/chains/alice25sept24 | ||
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likelihood: | ||
bao.sdss_dr7_mgs: # SDSS MGS | ||
# path: /cosmo/moyer/Desktop/SOLikeT/cobaya_packages/data/ | ||
bao.sdss_dr12_consensus_bao: # Boss DR11 like likelihood | ||
# path: /cosmo/moyer/Desktop/SOLikeT/cobaya_packages/data/ | ||
bao.sixdf_2011_bao: #F. Beutler et al 6dF likelihood | ||
#soliket.sz_binned_cluster_counts.binned_cc.binned_cc_likelihood: | ||
soliket.BinnedClusterLikelihood : | ||
#tcat_file: 'SZ_cat.txt' | ||
#snrcut: 6. | ||
#experiment: 'Planck' | ||
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# bin_z_min_cluster_counts : 0.0 | ||
# bin_z_max_cluster_counts : 1.0 | ||
# bin_dz_cluster_counts : 0.1 | ||
# bin_dlog10_snr: 0.25 | ||
debug: True | ||
verbose: True | ||
stop_at_error: True | ||
theorypred: | ||
choose_theory: classy_sz | ||
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theory: | ||
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classy_szfast.classy_sz.classy_sz: | ||
use_class_sz_fast_mode : 1 | ||
stop_at_error: true | ||
extra_args: | ||
#cosmo_model : 3 # w cdm 0= Lambda cdm 1= nuCDM 2 = | ||
non_linear: 'halofit' | ||
output : 'sz_cluster_counts' | ||
mass function : 'T08M500c' | ||
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has_selection_function : 1 | ||
experiment : 0 # Planck | ||
y_m_relation : 0 | ||
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SZ_cat_file: /Users/boris/Work/CLASS-SZ/SO-SZ/class_sz/class-sz/class_sz_auxiliary_files/excludes/tsz/planck_szcounts/SZ_cat.txt | ||
sz_selection_function_ylims_file: /Users/boris/Work/CLASS-SZ/SO-SZ/class_sz/class-sz/class_sz_auxiliary_files/excludes/tsz/planck_szcounts/SZ_ylims.txt | ||
sz_selection_function_skyfracs_file: /Users/boris/Work/CLASS-SZ/SO-SZ/class_sz/class-sz/class_sz_auxiliary_files/excludes/tsz/planck_szcounts/SZ_skyfracs.txt | ||
sz_selection_function_thetas_file: /Users/boris/Work/CLASS-SZ/SO-SZ/class_sz/class-sz/class_sz_auxiliary_files/excludes/tsz/planck_szcounts/SZ_thetas.txt | ||
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#signal-to-noise_cut-off_for_survey_cluster_completeness: 6.0 | ||
#m_pivot_ym : 6e14 | ||
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signal-to-noise_cut-off_for_survey_cluster_completeness : 6.0 | ||
use_planck_binned_proba : 1 | ||
use_skyaveraged_noise : 0 # changer de 1 à 0 suite aux conseil de Boris | ||
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M_min : 5e11 | ||
M_max : 5e15 | ||
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z_min: 0. | ||
z_max: 1.0 | ||
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# bin_z_min_cluster_counts : 0. | ||
# bin_z_max_cluster_counts : 2. | ||
# bin_dz_cluster_counts : 0.1 | ||
# | ||
# | ||
tau_reio: 0.054 # planck 2018 value (in abstract of 1807.06209) | ||
YHe: BBN | ||
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# 1 massive neutrino (planck 2018 baseline) | ||
N_ur: 2.0328 | ||
N_ncdm: 1 | ||
m_ncdm: 0.06 | ||
T_ncdm: 0.71611 | ||
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# | ||
# #3 massive neutrinos | ||
# N_ur : 0.00641 | ||
# N_ncdm : 1 | ||
# deg_ncdm : 3 | ||
# m_ncdm : 0.02 | ||
# T_ncdm : 0.71611 | ||
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# | ||
# HMF_prescription_NCDM: 'CDM' | ||
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# verbose parameters for debugging | ||
input_verbose : 0 | ||
background_verbose: 0 | ||
perturbations_verbose: 0 | ||
# class_sz_verbose : 0 | ||
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# X ray mass bias (if applicable) | ||
# B : 1.25 | ||
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bin_z_min_cluster_counts : 0.0 | ||
bin_z_max_cluster_counts : 1.0 | ||
bin_dz_cluster_counts : 0.1 | ||
bin_dlog10_snr: 0.25 | ||
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dlny : 0.1 | ||
lnymin : -30 | ||
lnymax : -2 | ||
sigmaM_ym : 0.075 #dispersion intrinsèque relation d'échelle | ||
alpha_ym : 1.789 | ||
ystar_ym : -0.186 | ||
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dlnM_cluster_count_completeness_grid : 0.1 | ||
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cluster_count_completeness_grid_z_cutoff_low : 0.2 | ||
cluster_count_completeness_grid_z_cutoff_mid : 0.5 | ||
dz_cluster_count_completeness_grid_low_z : 0.01 | ||
dz_cluster_count_completeness_grid_mid_z : 0.01 | ||
dz_cluster_count_completeness_grid_high_z : 0.1 | ||
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#mass_epsrel_cluster_counts : 1e-3 | ||
#mass_epsabs_cluster_counts : 1e-30 | ||
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#redshift_epsrel_cluster_counts : 1e-3 | ||
#redshift_epsabs_cluster_counts : 1e-30 | ||
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# | ||
# | ||
# # tabulation of mass function: | ||
n_z_dndlnM : 80 | ||
n_m_dndlnM : 80 | ||
# | ||
# # computation of mass function | ||
# # (grid in mass and redshifts for sigma and dsigma) | ||
ndim_masses : 80 | ||
ndim_redshifts : 80 | ||
# | ||
# pk setup for computation of sigma and dsigma | ||
k_per_decade_class_sz : 20. | ||
k_min_for_pk_class_sz : 1e-3 | ||
k_max_for_pk_class_sz : 1e1 | ||
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P_k_max_h/Mpc : 1e1 | ||
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class_sz_verbose: 0 | ||
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params: | ||
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H0: | ||
prior: | ||
min: 50. | ||
max: 80. | ||
ref: | ||
dist: norm | ||
loc: 68 | ||
scale: 0.1 | ||
proposal: 0.1 | ||
logA: | ||
prior: | ||
min: 1.61 | ||
max: 4 | ||
ref: | ||
dist: norm | ||
loc: 2.87 | ||
scale: 0.01 | ||
proposal: 0.01 | ||
# drop: true | ||
latex: \log(10^{10} A_\mathrm{s}) | ||
# A_s: | ||
# value: 'lambda logA: 1e-10*np.exp(logA)' | ||
# latex: A_\mathrm{s} | ||
n_s: | ||
prior: | ||
min: 0.8 | ||
max: 1.2 | ||
ref: | ||
dist: norm | ||
loc: 0.964 | ||
scale: 0.01 | ||
proposal: 0.01 | ||
latex: n_\mathrm{s} | ||
B: | ||
prior: | ||
min: 1.0 | ||
max: 2.0 | ||
ref: | ||
dist: norm | ||
loc: 1.25 | ||
scale: 0.02 | ||
proposal: 0.02 | ||
latex: B | ||
# sigmaM_ym : | ||
# prior: | ||
# min: 0 | ||
# max: 1 | ||
# ref: | ||
# dist: norm | ||
# loc: 0.075 | ||
# scale: 0.1 | ||
# proposal: 0.1 | ||
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# alpha_ym : | ||
# prior: | ||
# min: 1 | ||
# max: 3 | ||
# ref: | ||
# dist: norm | ||
# loc: 1.789 | ||
# scale: 0.1 | ||
# proposal: 0.1 | ||
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# ystar_ym : | ||
# prior: | ||
# min: -1 | ||
# max: 0 | ||
# ref: | ||
# dist: norm | ||
# loc: -0.186 | ||
# scale: 0.1 | ||
# proposal: 0.1 | ||
#B: | ||
# prior: | ||
# min: 1. | ||
# max: 2. | ||
# ref: | ||
# dist: norm | ||
# loc: 1.71 | ||
# scale: 0.02 | ||
# proposal: 0.02 | ||
# latex: B | ||
omega_b: | ||
prior: | ||
min: 0.005 #avant 0.01933 | ||
max: 0.02533 # avanr 0.02533 | ||
ref: | ||
dist: norm | ||
loc: 0.0224 | ||
scale: 0.005 | ||
proposal: 0.005 | ||
latex: \Omega_\mathrm{b}h^2 | ||
omega_cdm: | ||
prior: | ||
min: 0.001 #avant 0.08 | ||
max: 0.99 # avant 0.2 | ||
ref: | ||
dist: norm | ||
loc: 0.125 | ||
scale: 0.005 | ||
proposal: 0.005 | ||
latex: \Omega_\mathrm{c}h^2 | ||
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# F_sz: | ||
# derived: 'lambda sigma8, Omega_m, B, H0: (sigma8/0.8)*(Omega_m/0.3)**0.35*(B/1.25)**-0.35*(H0/70.)**-0.20' | ||
# latex: F_\mathrm{sz} | ||
#sigma8: | ||
# latex: \sigma_8 | ||
Omega_m: | ||
latex: \Omega_\mathrm{m} | ||
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prior: | ||
omega_b_prior: 'lambda omega_b: stats.norm.logpdf(omega_b, loc=0.022, scale=0.002)' | ||
n_s_prior: 'lambda n_s: stats.norm.logpdf(n_s, loc=0.964, scale=0.014)' | ||
B_prior: 'lambda B: stats.norm.logpdf(B, loc=1.2820,scale=0.17)' | ||
# sigmaM_ym_prior : 'lambda sigmaM_ym: stats.norm.logpdf(sigmaM_ym, loc=0.075, scale=0.01)' | ||
# alpha_ym_prior : 'lambda alpha_ym: stats.norm.logpdf(alpha_ym, loc=1.789, scale=0.08)' | ||
# ystar_ym_prior : 'lambda ystar_ym: stats.norm.logpdf(ystar_ym, loc=-0.186, scale=0.02)' | ||
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sampler: | ||
#settings for covmat see https://cobaya.readthedocs.io/en/latest/sampler_mcmc.html | ||
# mcmc: | ||
# #covmat: /archeops/moyer/Desktop/cosmopo/class_sz_unbinned_cluster_counts_planck.covmat | ||
# #remettre la bonne covmat de cette analyse plus tard? | ||
# Rminus1_stop: 0.5 # remettre à 0.01 apres? | ||
# #Rminus1_cl_stop : 0.4 | ||
# burn_in: 100 | ||
# # drag: true | ||
# proposal_scale: 1.2 | ||
# learn_proposal: True | ||
# #learn_every: 40 | ||
# learn_proposal_Rminus1_max: 2. | ||
# learn_proposal_Rminus1_max_early: 80.0 | ||
# max_tries : 1000 | ||
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evaluate: | ||
override: | ||
# #parameter values: | ||
omega_cdm: 0.125 | ||
omega_b: 0.0224 | ||
logA: 2.95 | ||
n_s: 0.96 | ||
H0: 69. | ||
B: 1.25 | ||
# theta_MC_100: 1.043612 | ||
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debug : False | ||
timing: true |