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setup for fitting artis models
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from dalek import assemble_tardis_model | |
from dalek.base.model import SimpleTARDISUncertaintyModel, NormRedSpectrum, LogLikelihood | |
from dalek.base.base import BaseLikelihoodModel | |
from dalek.base.transform import uniform_transform | |
from astropy import units as u, constants as const | |
import os | |
base_dir = '/home/hpc/pr94se/di73qom/projects/tardis/dalek/test_artis_run/artis_fit' | |
artis_filename = os.path.join(base_dir, 'aaflux_057.dat') | |
log_fname = os.path.join(base_dir, 'dalek_log.txt') | |
spec_dir = os.path.join(base_dir, 'spectral_store') | |
class ArtisDELogLikelihood(BaseLikelihoodModel): | |
def transform(self, si, s, ca, fe, co, ni, mg, ti, cr, c, lum, v_inner): | |
v_inner = uniform_transform(v_inner, 7000, 15000) | |
lum = uniform_transform(lum, 4e42, 3e43) | |
s = uniform_transform(s, 0, 0.5) | |
fe = uniform_transform(fe, 0, 0.2) | |
co = uniform_transform(co, 0, 0.2) | |
ni = uniform_transform(ni, 0, 0.2) | |
c = uniform_transform(c, 0, 0.1) | |
mg = uniform_transform(mg, 0, 0.1) | |
ca = uniform_transform(ca, 0, 0.1) | |
ti = uniform_transform(ti, 0, 0.02) | |
cr = uniform_transform(cr, 0, 0.02) | |
o = 1 - np.sum([si, s, ca, fe, co, ni, mg, ti, cr, c]) | |
return o, si, s, ca, fe, co, ni, mg, ti, cr, c, lum, v_inner | |
def calculate_priors(self, o, si, s, ca, fe, co, ni, mg, ti, cr, c, lum, v_inner): | |
priors = 0 | |
if o <= 0.: | |
priors += np.inf | |
if s > si: | |
priors += np.inf | |
return priors | |
parameters = ['model.abundances.o', | |
'model.abundances.si', | |
'model.abundances.s', | |
'model.abundances.ca', | |
'model.abundances.fe', | |
'model.abundances.co', | |
'model.abundances.ni', | |
'model.abundances.mg', | |
'model.abundances.ti', | |
'model.abundances.cr', | |
'model.abundances.c', | |
'supernova.luminosity_requested', | |
'model.structure.velocity.item0'] | |
artisw, artisf = loadtxt(artis_filename, unpack=1) | |
artisw = artisw[198:] | |
artisf = artisf[198:] | |
artisf *= ((1 * u.Mpc)**2).to(u.cm**2).value * 4 * np.pi | |
artisu = artisf * 0.01 | |
tardis_model = assemble_tardis_model('tardis_artis_fits.yml', parameters) | |
full_model = (tardis_model | SimpleTARDISUncertaintyModel(artisw) | |
| NormRedSpectrum() | LogLikelihood(artisw, artisf, artisu, wavelength_end=9000.)) | |
deartis = ArtisDELogLikelihood(full_model, log_fname, spec_dir=spec_dir) |
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