def test_make_interpolation(self):
""" Test Keplerian circular orbit model. """
# Instantiate emissivity object in setup mode.
emissivity_setup = Emissivity(setup_mode=True)
emissivity_setup.rt_results_db = 'test_jar/mock_rt_results.db'
emissivity_setup.rt_results_table = 'mock_data'
# Setup spectral line and wind velocity profile.
emissivity_setup.set_spectral_line(line=3)
emissivity_setup.set_wind_velocity_profile(
wind_velocity_solution='beta_1',
initial_velocity=20,
stellar_radius=50,
sonic_radius=60)
# Build interpolation object.
Mdot = 5e-4
Vinf = 500
Time = np.linspace(0, 1000, 10)
emissivity_setup.build_static_interpolation_object(Mdot, Vinf, Time)
def test_convolutional_model_rt_interp_kernel_eccentric(self):
""" Test ck-motion w/ RT interp kernel for eccentric orbit. """
# Arbitrary eccentric orbit.
emissivity = Emissivity(setup_mode=False, pickle_dir='test_jar')
windy_star.configure_params(
period=2022.7, eccentricity=0.9, rv_semi_amplitude=100,
argument_of_periastron=270, rv_offset=0,
m_dot_a=5e-4, wind_velocity_a=500)
windy_star.configure_epochs(epochs=np.linspace(0, 2, 1000))
windy_star.configure_kernel(kernel_mode='RTInterp',
kernel_line=3, interp_dims='Grid',
emissivity_interpolators=emissivity)
res_df = windy_star.convolutional_model_centroid_velocity
from ckm.core.motion import windy_star
from ckm.radiative.emissivity import Emissivity
from ckm.core.utils import unpickle_observations
# Setup
OBSERVATIONS = ['emission_line_fits_1.p', 'emission_line_fits_2.p']
# Load observations.
obs = unpickle_observations(OBSERVATIONS_PATH,
OBSERVATIONS,
time_of_periastron=2555555,
period=1000,
n_periods=2)
# Load interpolation objects.
emissivity = Emissivity(setup_mode=False, pickle_dir='interp_jar/rt_code_v1')
# Configure params and epochs and kernel.
windy_star.configure_params(period=1000,
eccentricity=0.7,
rv_semi_amplitude=60,
argument_of_periastron=250,
rv_offset=-20)
windy_star.configure_epochs(epochs=np.linspace(0, 2, 1000))
windy_star.configure_kernel(kernel_mode='RTInterp',
kernel_line=4,
interp_dims='Point',
emissivity_interpolators=emissivity)
# Calculate centroid velocity of convolved/time averaged Keplerian orbit
res_df = windy_star.convolutional_model_centroid_velocity
print('Convergence stats: mean tau={} <? threshold N/50={}'.format(
convergence['mean_tau'], convergence['threshold']))
# Optimized parameter results taken to be 50th percentile.
# Errors, 16th - 84th percentiles.
param_labels = [
'TimeOfPeriastron', 'Eccentricity', 'RVSemiAmplitude',
'ArgumentOfPeriastron'
]
percentiles = calc_mcmc_chain_percentiles(sample_chain, param_labels)
print(percentiles['16th_percentile'], '\n')
print(percentiles['Median'], '\n')
print(percentiles['84th_percentile'])
# Load interpolation objects.
emissivity = Emissivity(setup_mode=False, pickle_dir=INTERP_PICKLE)
# Iterate observed spectral lines.
fig = plt.figure(figsize=(20, 10))
line_index = 1
for line, data in observations.items():
print('Line {}.'.format(line_index))
ax = fig.add_subplot(2, math.ceil(len(observations) / 2), line_index)
markers, caps, bars = ax.errorbar(data['Phase'],
data['Velocity'] +
systemic[line_index - 1],
yerr=None,
color='#000000',
fmt='o',
markersize='1',
# Grid parameterisations: must be evenly spaced and correspond
# to available param space output from radiative transfer. N.B
# limiting times provides a kernel size which ensures complete
# overlap in the convolution's valid mode for a given
# number/fraction of signal/periods.
Mdot = 1e-5
Vinf = 1300
Time = np.linspace(0, 10, 100)
# Iterate spectral lines.
spectral_lines = [1, 2]
for line in spectral_lines:
# Instantiate emissivity object in setup mode.
# N.B see line_label for verbose transition name.
emissivity_setup = Emissivity(setup_mode=True)
emissivity_setup.rt_results_db = RT_DB_PATH
emissivity_setup.rt_results_table = RT_TABLE
# Setup spectral line and wind velocity profile.
emissivity_setup.set_spectral_line(line)
emissivity_setup.set_wind_velocity_profile(
wind_velocity_solution=WIND_VELOCITY_SOL,
initial_velocity=INITIAL_VELOCITY,
stellar_radius=STELLAR_RADIUS,
sonic_radius=SONIC_RADIUS)
# Build interpolation object.
emissivity_setup.build_static_interpolation_object(Mdot, Vinf, Time)
# Write interpolation object to disk.