First attempt at SN inference test
BIN
tests/sn_corner.png
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@ -7,12 +7,17 @@ import astropy.units as apu
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import jax.numpy as jnp
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import jax
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import corner
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import matplotlib.pyplot as plt
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import borg_velocity.poisson_process as poisson_process
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import borg_velocity.projection as projection
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import borg_velocity.utils as utils
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import numpyro
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import numpyro.distributions as dist
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from jax import lax, random
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from tfr_inference import get_fields, generateMBData
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# Output stream management
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@ -464,7 +469,218 @@ def test_likelihood_scan(prior, alpha, a_tripp, b_tripp, M_SN, sigma_SN, sigma_v
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return
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def run_mcmc(num_warmup, num_samples, prior, initial, dens, vel, cpar, L, xmin, interp_order, bias_epsilon,
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czCMB, m_obs, stretch_obs, c_obs, sigma_m, sigma_stretch, sigma_c, MB_pos,):
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"""
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Run MCMC over the model parameters
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Args:
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- num_warmup (int): Number of warmup steps to take in the MCMC
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- num_samples (int): Number of samples to take in the MCMC
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- prior
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- initial
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- dens (np.ndarray): Over-density field (shape = (N, N, N))
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- vel (np.ndarray): Velocity field (km/s) (shape = (3, N, N, N))
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- cpar (borg.cosmo.CosmologicalParameters): Cosmological parameters to use
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- L (float): Comoving box size (Mpc/h)
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- xmin (float): Coordinate of corner of the box (Mpc/h)
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- interp_order (int): Order of interpolation from grid points to the line of sight
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- bias_epsilon (float): Small number to add to 1 + delta to prevent 0^#
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- cz_obs (np.ndarray): Observed redshifts (km/s) of the tracers (shape = (Nt,))
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- m_obs (np.ndarray): Observed apparent magnitudes of the tracers (shape = (Nt,))
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- sigma_m (float): Uncertainty on the apparent magnitude measurements
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- MB_pos (np.ndarray): Comoving coordinates of integration points to use in likelihood (Mpc/h).
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The shape is (3, Nt, Nsig)
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Returns:
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- mcmc (numpyro.infer.MCMC): MCMC object which has been run
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"""
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Nt = stretch_obs.shape[0]
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omega_m = cpar.omega_m
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h = cpar.h
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sigma_bulk = utils.get_sigma_bulk(L, cpar)
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def sn_model():
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alpha = numpyro.sample("alpha", dist.Uniform(*prior['alpha']))
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a_tripp = numpyro.sample("a_tripp", dist.Uniform(*prior['a_tripp']))
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b_tripp = numpyro.sample("b_tripp", dist.Uniform(*prior['b_tripp']))
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M_SN = numpyro.sample("M_SN", dist.Uniform(*prior['M_SN']))
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sigma_SN = numpyro.sample("sigma_SN", dist.HalfCauchy(1.0))
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sigma_v = numpyro.sample("sigma_v", dist.Uniform(*prior['sigma_v']))
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hyper_mean_m = numpyro.sample("hyper_mean_m", dist.Uniform(*prior['hyper_mean_m']))
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hyper_sigma_m = numpyro.sample("hyper_sigma_m", dist.HalfCauchy(1.0)) # Equivalent to 1/sigma prior
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hyper_mean_stretch = numpyro.sample("hyper_mean_stretch", dist.Uniform(*prior['hyper_mean_stretch']))
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hyper_sigma_stretch = numpyro.sample("hyper_sigma_stretch", dist.HalfCauchy(1.0)) # Equivalent to 1/sigma prior
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hyper_mean_c = numpyro.sample("hyper_mean_c", dist.Uniform(*prior['hyper_mean_c']))
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hyper_sigma_c = numpyro.sample("hyper_sigma_c", dist.HalfCauchy(1.0)) # Equivalent to 1/sigma prior
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# Sample correlation matrix using LKJ prior
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L_corr = numpyro.sample("L_corr", dist.LKJCholesky(3, concentration=1.0)) # Cholesky factor of correlation matrix
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corr_matrix = L_corr @ L_corr.T # Convert to full correlation matrix
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# Construct full covariance matrix: Σ = D * Corr * D
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hyper_mean = jnp.array([hyper_mean_m, hyper_mean_stretch, hyper_mean_c])
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hyper_sigma = jnp.array([hyper_sigma_m, hyper_sigma_stretch, hyper_sigma_c])
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hyper_cov = jnp.diag(hyper_sigma) @ corr_matrix @ jnp.diag(hyper_sigma)
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# Sample m_true and eta_true
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x = numpyro.sample("true_vars", dist.MultivariateNormal(hyper_mean, hyper_cov), sample_shape=(Nt,))
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m_true = numpyro.deterministic("m_true", x[:, 0])
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stretch_true = numpyro.deterministic("stretch_true", x[:, 1])
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c_true = numpyro.deterministic("c_true", x[:, 2])
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# Sample bulk velocity
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vbulk_x = numpyro.sample("vbulk_x", dist.Normal(0, sigma_bulk / jnp.sqrt(3)))
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vbulk_y = numpyro.sample("vbulk_y", dist.Normal(0, sigma_bulk / jnp.sqrt(3)))
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vbulk_z = numpyro.sample("vbulk_z", dist.Normal(0, sigma_bulk / jnp.sqrt(3)))
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# Evaluate the likelihood
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numpyro.sample("obs", SNLikelihood(alpha, a_tripp, b_tripp, M_SN, sigma_SN, sigma_v, m_true, stretch_true, c_true, vbulk_x, vbulk_y, vbulk_z), obs=jnp.array([m_obs, stretch_obs, c_obs]))
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class SNLikelihood(dist.Distribution):
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support = dist.constraints.real
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def __init__(self, alpha, a_tripp, b_tripp, M_SN, sigma_SN, sigma_v, m_true, stretch_true, c_true, vbulk_x, vbulk_y, vbulk_z):
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self.alpha, self.a_tripp, self.b_tripp, self.M_SN, self.sigma_SN, self.sigma_v, self.m_true, self.stretch_true, self.c_true, self.vbulk_x, self.vbulk_y, self.vbulk_z = dist.util.promote_shapes(alpha, a_tripp, b_tripp, M_SN, sigma_SN, sigma_v, m_true, stretch_true, c_true, vbulk_x, vbulk_y, vbulk_z)
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batch_shape = lax.broadcast_shapes(
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jnp.shape(alpha),
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jnp.shape(a_tripp),
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jnp.shape(b_tripp),
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jnp.shape(M_SN),
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jnp.shape(sigma_SN),
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jnp.shape(sigma_v),
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jnp.shape(m_true),
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jnp.shape(stretch_true),
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jnp.shape(c_true),
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jnp.shape(vbulk_x),
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jnp.shape(vbulk_y),
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jnp.shape(vbulk_z),
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)
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super(SNLikelihood, self).__init__(batch_shape = batch_shape)
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def sample(self, key, sample_shape=()):
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raise NotImplementedError
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def log_prob(self, value):
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vbulk = jnp.array([self.vbulk_x, self.vbulk_y, self.vbulk_z])
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loglike = likelihood(self.alpha, self.a_tripp, self.b_tripp, self.M_SN, self.sigma_SN, self.sigma_v,
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self.m_true, self.stretch_true, self.c_true, vbulk,
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dens, vel, omega_m, h, L, xmin, interp_order, bias_epsilon,
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czCMB, m_obs, stretch_obs, c_obs, sigma_m, sigma_stretch, sigma_c, MB_pos)
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return loglike
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rng_key = random.PRNGKey(6)
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rng_key, rng_key_ = random.split(rng_key)
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values = initial
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values['true_vars'] = jnp.array([m_obs, stretch_obs, c_obs]).T
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values['L_corr'] = jnp.identity(3)
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values['vbulk_x'] = 0.
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values['vbulk_y'] = 0.
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values['vbulk_z'] = 0.
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myprint('Preparing MCMC kernel')
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kernel = numpyro.infer.NUTS(sn_model,
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init_strategy=numpyro.infer.initialization.init_to_value(values=initial)
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)
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mcmc = numpyro.infer.MCMC(kernel, num_warmup=num_warmup, num_samples=num_samples)
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myprint('Running MCMC')
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mcmc.run(rng_key_)
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mcmc.print_summary()
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return mcmc
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def process_mcmc_run(mcmc, param_labels, truths, true_vars):
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"""
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Make summary plots from the MCMC and save these to file
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Args:
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- mcmc (numpyro.infer.MCMC): MCMC object which has been run
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- param_labels (list[str]): Names of the parameters to plot
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- truths (list[float]): True values of the parameters to plot. If unknown, then entry is None
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- true_vars (dict): True values of the observables to compare against inferred ones
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"""
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# Convert samples into a single array
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samples = mcmc.get_samples()
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samps = jnp.empty((len(samples[param_labels[0]]), len(param_labels)))
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for i, p in enumerate(param_labels):
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if p.startswith('hyper_corr'):
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L_corr = samples['L_corr']
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corr_matrix = jnp.matmul(L_corr, jnp.transpose(L_corr, (0, 2, 1)))
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if p == 'hyper_corr_mx':
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samps = samps.at[:,i].set(corr_matrix[:,0,1])
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elif p == 'hyper_corr_mc':
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samps = samps.at[:,i].set(corr_matrix[:,0,2])
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elif p == 'hyper_corr_xc':
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samps = samps.at[:,i].set(corr_matrix[:,1,2])
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else:
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raise NotImplementedError
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else:
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samps = samps.at[:,i].set(samples[p])
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# Trace plot of non-redshift quantities
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fig1, axs1 = plt.subplots(samps.shape[1], 1, figsize=(6,3*samps.shape[1]), sharex=True)
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axs1 = np.atleast_1d(axs1)
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for i in range(samps.shape[1]):
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axs1[i].plot(samps[:,i])
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axs1[i].set_ylabel(param_labels[i])
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if truths[i] is not None:
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axs1[i].axhline(truths[i], color='k')
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axs1[-1].set_xlabel('Step Number')
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fig1.tight_layout()
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fig1.savefig('sn_trace.png')
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# Corner plot
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fig2, axs2 = plt.subplots(samps.shape[1], samps.shape[1], figsize=(20,20))
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corner.corner(
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np.array(samps),
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labels=param_labels,
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fig=fig2,
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truths=truths
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)
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fig2.savefig('sn_corner.png')
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# True vs predicted
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for var in ['stretch', 'c', 'm']:
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vname = var + '_true'
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if vname in samples.keys():
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xtrue = true_vars[var]
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xpred_median = np.median(samples[vname], axis=0)
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xpred_plus = np.percentile(samples[vname], 84, axis=0) - xpred_median
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xpred_minus = xpred_median - np.percentile(samples[vname], 16, axis=0)
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fig3, axs3 = plt.subplots(2, 1, figsize=(10,8), sharex=True)
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plot_kwargs = {'fmt':'.', 'markersize':3, 'zorder':10,
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'capsize':1, 'elinewidth':1, 'alpha':1}
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axs3[0].errorbar(xtrue, xpred_median, yerr=[xpred_minus, xpred_plus], **plot_kwargs)
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axs3[1].errorbar(xtrue, xpred_median - xtrue, yerr=[xpred_minus, xpred_plus], **plot_kwargs)
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axs3[1].set_xlabel('True')
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axs3[0].set_ylabel('Predicted')
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axs3[1].set_ylabel('Predicted - True')
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xlim = axs3[0].get_xlim()
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ylim = axs3[0].get_ylim()
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axs3[0].plot(xlim, xlim, color='k', zorder=0)
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axs3[0].set_xlim(xlim)
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axs3[0].set_ylim(ylim)
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axs3[1].axhline(0, color='k', zorder=0)
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fig3.suptitle(var)
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fig3.align_labels()
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fig3.tight_layout()
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fig3.savefig(f'sn_true_predicted_{var}.png')
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return
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def main():
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@ -493,15 +709,8 @@ def main():
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M_SN = - 18.558
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sigma_SN = 0.082
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prior = {
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'alpha': [0.5, 4.5],
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'a_tripp': [0.01, 0.2],
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'b_tripp': [2.5, 4.5],
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'M_SN': [-19.5, -17.5],
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'hyper_mean_stretch': [hyper_stretch_mu - hyper_stretch_sigma, hyper_stretch_mu + hyper_stretch_sigma],
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'hyper_mean_c':[hyper_c_mu - hyper_c_sigma, hyper_c_mu + hyper_c_sigma],
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'sigma_v': [10, 3000],
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}
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num_warmup = 1000
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num_samples = 2000
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# Make mock
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np.random.seed(123)
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@ -513,6 +722,30 @@ def main():
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sigma_v, interp_order=interp_order, bias_epsilon=bias_epsilon)
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MB_pos = generateMBData(RA, Dec, czCMB, L, N, R_lim, Nsig, Nint_points, sigma_v, frac_sigma_r)
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initial = {
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'a_tripp': a_tripp,
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'b_tripp': b_tripp,
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'M_SN': M_SN,
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'sigma_SN': sigma_SN,
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'sigma_v': sigma_v,
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'hyper_mean_stretch': hyper_stretch_mu,
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'hyper_sigma_stretch': hyper_stretch_sigma,
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'hyper_mean_c': hyper_c_mu,
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'hyper_sigma_c': hyper_c_sigma,
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'hyper_mean_m': np.median(m_obs),
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'hyper_sigma_m': (np.percentile(m_obs, 84) - np.percentile(m_obs, 16)) / 2,
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}
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prior = {
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'alpha': [0.5, 4.5],
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'a_tripp': [0.01, 0.2],
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'b_tripp': [2.5, 4.5],
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'M_SN': [-19.5, -17.5],
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'hyper_mean_stretch': [hyper_stretch_mu - hyper_stretch_sigma, hyper_stretch_mu + hyper_stretch_sigma],
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'hyper_mean_c':[hyper_c_mu - hyper_c_sigma, hyper_c_mu + hyper_c_sigma],
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'hyper_mean_m':[initial['hyper_mean_m'] - initial['hyper_sigma_m'], initial['hyper_mean_m'] + initial['hyper_sigma_m']],
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'sigma_v': [10, 3000],
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}
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# Test likelihood
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loglike = likelihood(alpha, a_tripp, b_tripp, M_SN, sigma_SN, sigma_v, m_true, stretch_true, c_true, vbulk,
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dens, vel, cpar.omega_m, cpar.h, L, xmin, interp_order, bias_epsilon,
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@ -525,9 +758,32 @@ def main():
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czCMB, m_obs, stretch_obs, c_obs, sigma_m, sigma_stretch, sigma_c, MB_pos)
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# Run a MCMC
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mcmc = run_mcmc(num_warmup, num_samples, prior, initial, dens, vel, cpar, L, xmin, interp_order, bias_epsilon,
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czCMB, m_obs, stretch_obs, c_obs, sigma_m, sigma_stretch, sigma_c, MB_pos,)
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param_labels = ['alpha', 'a_tripp', 'b_tripp', 'M_SN', 'sigma_SN', 'sigma_v',
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'hyper_mean_m', 'hyper_sigma_m', 'hyper_mean_stretch', 'hyper_sigma_stretch',
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'hyper_mean_c', 'hyper_sigma_c', 'hyper_corr_mx', 'hyper_corr_mc', 'hyper_corr_xc',
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'vbulk_x', 'vbulk_y', 'vbulk_z']
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truths = [alpha, a_tripp, b_tripp, M_SN, sigma_SN, sigma_v,
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None, None, hyper_stretch_mu, hyper_stretch_sigma,
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hyper_c_mu, hyper_c_sigma, None, None, None,
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vbulk[0], vbulk[1], vbulk[2]]
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true_vars = {'m':m_true, 'stretch':stretch_true, 'c': c_true}
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process_mcmc_run(mcmc, param_labels, truths, true_vars)
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return
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if __name__ == "__main__":
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main()
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"""
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TO DO
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- Fix SN inference - poor sampling and Tripp variables not constrained
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- Deal with case where sigma_eta and sigma_m could be floats vs arrays
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- Add in selection cuts for the supernovae
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"""
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BIN
tests/sn_trace.png
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After Width: | Height: | Size: 518 KiB |
BIN
tests/sn_true_predicted_c.png
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After Width: | Height: | Size: 52 KiB |
BIN
tests/sn_true_predicted_m.png
Normal file
After Width: | Height: | Size: 44 KiB |
BIN
tests/sn_true_predicted_stretch.png
Normal file
After Width: | Height: | Size: 47 KiB |
BIN
tests/tfr_corner.png
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After Width: | Height: | Size: 1.2 MiB |
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@ -666,7 +666,7 @@ def test_likelihood_scan(prior, alpha, a_TFR, b_TFR, sigma_TFR, sigma_v, m_true,
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plt.axhline(orig_ll, ls='--', color='k')
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plt.xlabel(name)
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plt.ylabel('Negative log-likelihood')
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plt.savefig(f'likelihood_scan_{name}.png')
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plt.savefig(f'tfr_likelihood_scan_{name}.png')
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fig = plt.gcf()
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plt.clf()
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plt.close(fig)
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@ -685,7 +685,7 @@ def test_likelihood_scan(prior, alpha, a_TFR, b_TFR, sigma_TFR, sigma_v, m_true,
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plt.axhline(orig_ll, ls='--', color='k')
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plt.xlabel('mthresh')
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plt.ylabel('Negative log-likelihood')
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plt.savefig(f'likelihood_scan_mthresh.png')
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plt.savefig(f'tfr_likelihood_scan_mthresh.png')
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fig = plt.gcf()
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plt.clf()
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plt.close(fig)
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|
@ -763,22 +763,20 @@ def run_mcmc(num_warmup, num_samples, prior, initial, dens, vel, cpar, L, xmin,
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vbulk_z = numpyro.sample("vbulk_z", dist.Normal(0, sigma_bulk / jnp.sqrt(3)))
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# Evaluate the likelihood
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numpyro.sample("obs", TFRLikelihood(alpha, a_TFR, b_TFR, sigma_TFR, sigma_v, hyper_mean_eta, hyper_sigma_eta, m_true, eta_true, vbulk_x, vbulk_y, vbulk_z), obs=jnp.array([m_obs, eta_obs]))
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numpyro.sample("obs", TFRLikelihood(alpha, a_TFR, b_TFR, sigma_TFR, sigma_v, m_true, eta_true, vbulk_x, vbulk_y, vbulk_z), obs=jnp.array([m_obs, eta_obs]))
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class TFRLikelihood(dist.Distribution):
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support = dist.constraints.real
|
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def __init__(self, alpha, a_TFR, b_TFR, sigma_TFR, sigma_v, hyper_mean_eta, hyper_sigma_eta, m_true, eta_true, vbulk_x, vbulk_y, vbulk_z):
|
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self.alpha, self.a_TFR, self.b_TFR, self.sigma_TFR, self.sigma_v, self.hyper_mean_eta, self.hyper_sigma_eta, self.m_true, self.eta_true, self.vbulk_x, self.vbulk_y, self.vbulk_z = dist.util.promote_shapes(alpha, a_TFR, b_TFR, sigma_TFR, sigma_v, hyper_mean_eta, hyper_sigma_eta, m_true, eta_true, vbulk_x, vbulk_y, vbulk_z)
|
||||
def __init__(self, alpha, a_TFR, b_TFR, sigma_TFR, sigma_v, m_true, eta_true, vbulk_x, vbulk_y, vbulk_z):
|
||||
self.alpha, self.a_TFR, self.b_TFR, self.sigma_TFR, self.sigma_v, self.m_true, self.eta_true, self.vbulk_x, self.vbulk_y, self.vbulk_z = dist.util.promote_shapes(alpha, a_TFR, b_TFR, sigma_TFR, sigma_v, m_true, eta_true, vbulk_x, vbulk_y, vbulk_z)
|
||||
batch_shape = lax.broadcast_shapes(
|
||||
jnp.shape(alpha),
|
||||
jnp.shape(a_TFR),
|
||||
jnp.shape(b_TFR),
|
||||
jnp.shape(sigma_TFR),
|
||||
jnp.shape(sigma_v),
|
||||
jnp.shape(hyper_mean_eta),
|
||||
jnp.shape(hyper_sigma_eta),
|
||||
jnp.shape(m_true),
|
||||
jnp.shape(eta_true),
|
||||
jnp.shape(vbulk_x),
|
||||
|
@ -851,7 +849,7 @@ def process_mcmc_run(mcmc, param_labels, truths, true_vars):
|
|||
axs1[i].axhline(truths[i], color='k')
|
||||
axs1[-1].set_xlabel('Step Number')
|
||||
fig1.tight_layout()
|
||||
fig1.savefig('trace.png')
|
||||
fig1.savefig('tfr_trace.png')
|
||||
|
||||
# Corner plot
|
||||
fig2, axs2 = plt.subplots(samps.shape[1], samps.shape[1], figsize=(20,20))
|
||||
|
@ -861,7 +859,7 @@ def process_mcmc_run(mcmc, param_labels, truths, true_vars):
|
|||
fig=fig2,
|
||||
truths=truths
|
||||
)
|
||||
fig2.savefig('corner.png')
|
||||
fig2.savefig('tfr_corner.png')
|
||||
|
||||
# True vs predicted
|
||||
for var in ['eta', 'm']:
|
||||
|
@ -889,7 +887,7 @@ def process_mcmc_run(mcmc, param_labels, truths, true_vars):
|
|||
fig3.suptitle(var)
|
||||
fig3.align_labels()
|
||||
fig3.tight_layout()
|
||||
fig3.savefig(f'true_predicted_{var}.png')
|
||||
fig3.savefig(f'tfr_true_predicted_{var}.png')
|
||||
|
||||
return
|
||||
|
||||
|
|
Before Width: | Height: | Size: 17 KiB After Width: | Height: | Size: 17 KiB |
Before Width: | Height: | Size: 18 KiB After Width: | Height: | Size: 18 KiB |
Before Width: | Height: | Size: 18 KiB After Width: | Height: | Size: 18 KiB |
Before Width: | Height: | Size: 18 KiB After Width: | Height: | Size: 18 KiB |
Before Width: | Height: | Size: 18 KiB After Width: | Height: | Size: 18 KiB |
Before Width: | Height: | Size: 18 KiB After Width: | Height: | Size: 18 KiB |
BIN
tests/tfr_trace.png
Normal file
After Width: | Height: | Size: 387 KiB |
BIN
tests/tfr_true_predicted_eta.png
Normal file
After Width: | Height: | Size: 46 KiB |
BIN
tests/tfr_true_predicted_m.png
Normal file
After Width: | Height: | Size: 46 KiB |