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Merge pull request #87 from joezuntz/act-dr6-lens
Act DR6 lensing likelihood
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[cosmological_parameters] | ||
ombh2 = normal 0.02233 0.00036 | ||
n_s = normal 0.96 0.02 |
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[cosmological_parameters] | ||
omch2 = 0.08 0.12 0.16 | ||
ombh2 = 0.01 0.02233 0.03 | ||
log1e10As = 2.9 3.0448 3.2 | ||
n_s = 0.86 0.96 1.06 | ||
cosmomc_theta = 0.009 0.0104 0.012 | ||
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omega_k = 0.0 ;spatial curvature | ||
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;neutrinos | ||
mnu = 0.06 | ||
nnu = 3.046 | ||
num_massive_neutrinos = 3 | ||
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;helium | ||
yhe = 0.245341 ;helium mass fraction | ||
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;reionization | ||
tau = 0.0543 ;reionization optical depth | ||
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[halo_model_parameters] | ||
A = 3.13 | ||
eta = 0.603 |
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[runtime] | ||
sampler = test | ||
root = ${PWD} | ||
resume = T | ||
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[test] | ||
save_dir=output/act_dr6_lens | ||
fatal_errors=T | ||
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[nautilus] | ||
n_live = 1500 | ||
verbose = T | ||
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[emcee] | ||
walkers = 64 | ||
samples = 1000 | ||
nsteps = 5 | ||
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[pipeline] | ||
; these names refer to sections later in the file: | ||
modules = consistency camb act_dr6_lens | ||
values = examples/act-dr6-lens-values.ini | ||
priors = examples/act-dr6-lens-priors.ini | ||
quiet=F | ||
debug=F | ||
timing=F | ||
extra_output=cosmological_parameters/sigma_8 cosmological_parameters/omega_m | ||
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[act_dr6_lens] | ||
file = ./likelihood/act-dr6-lens/act_dr6_lenslike_interface.py | ||
like_corrections = T | ||
variant = actplanck_baseline | ||
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[output] | ||
filename = output/act-dr6-lens.txt | ||
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; The consistency module translates between our chosen parameterization | ||
; and any other that modules in the pipeline may want (e.g. camb) | ||
[consistency] | ||
file = ./utility/consistency/consistency_interface.py | ||
cosmomc_theta = T | ||
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[camb] | ||
file = boltzmann/camb/camb_interface.py | ||
mode = cmb | ||
lmax = 4000 ;max ell to use for cmb calculation | ||
lens_margin = 1250 | ||
lens_potential_accuracy = 4 | ||
feedback=0 ;amount of output to print | ||
AccuracyBoost=1.0 ;CAMB accuracy boost parameter | ||
lSampleBoost = 1.0 | ||
lAccuracyBoost = 1.0 | ||
do_tensors = T ;include tensor modes | ||
do_lensing = T ;lensing is required w/ Planck data | ||
NonLinear = lens | ||
theta_H0_range = "20 100" | ||
halofit_version = takahashi |
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data/ |
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BSD 2-Clause License | ||
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Copyright (c) 2023, Members of the Atacama Cosmology Telescope Collaboration | ||
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Redistribution and use in source and binary forms, with or without | ||
modification, are permitted provided that the following conditions are met: | ||
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1. Redistributions of source code must retain the above copyright notice, this | ||
list of conditions and the following disclaimer. | ||
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2. Redistributions in binary form must reproduce the above copyright notice, | ||
this list of conditions and the following disclaimer in the documentation | ||
and/or other materials provided with the distribution. | ||
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THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS" | ||
AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE | ||
IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE | ||
DISCLAIMED. IN NO EVENT SHALL THE COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE | ||
FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL | ||
DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR | ||
SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER | ||
CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, | ||
OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE | ||
OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. |
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