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Switch to Jeffrey prior (#153)
* Switch to Jeffrey * Add Jeffrey priors * Bring things back
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1 changed files with 12 additions and 1 deletions
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@ -607,10 +607,15 @@ class PV_LogLikelihood(BaseFlowValidationModel):
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Vmono = field_calibration_params["Vmono"]
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Vmono = field_calibration_params["Vmono"]
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Vext_rad = project_Vext(Vext[0], Vext[1], Vext[2], self.RA, self.dec)
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Vext_rad = project_Vext(Vext[0], Vext[1], Vext[2], self.RA, self.dec)
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e_mu = distmod_params["e_mu"]
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# Jeffrey's prior on sigma_v and the intrinsic scatter, they are above
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# "sampled" from uniform distributions.
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ll0 -= jnp.log(sigma_v) + jnp.log(e_mu)
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# ------------------------------------------------------------
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# ------------------------------------------------------------
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# 1. Sample true observables and obtain the distance estimate
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# 1. Sample true observables and obtain the distance estimate
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# ------------------------------------------------------------
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# ------------------------------------------------------------
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e_mu = distmod_params["e_mu"]
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if self.kind == "SN":
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if self.kind == "SN":
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mag_cal = distmod_params["mag_cal"]
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mag_cal = distmod_params["mag_cal"]
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alpha_cal = distmod_params["alpha_cal"]
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alpha_cal = distmod_params["alpha_cal"]
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@ -624,6 +629,9 @@ class PV_LogLikelihood(BaseFlowValidationModel):
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c_mean, c_std = sample_gaussian_hyperprior(
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c_mean, c_std = sample_gaussian_hyperprior(
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"c", self.name, self.c_min, self.c_max)
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"c", self.name, self.c_min, self.c_max)
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# Jeffrey's prior on the the MNR hyperprior widths.
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ll0 -= jnp.log(mag_std) + jnp.log(x1_std) + jnp.log(c_std)
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# NOTE: that the true variables are currently uncorrelated.
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# NOTE: that the true variables are currently uncorrelated.
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with plate(f"true_SN_{self.name}", self.ndata):
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with plate(f"true_SN_{self.name}", self.ndata):
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mag_true = sample(
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mag_true = sample(
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@ -675,6 +683,9 @@ class PV_LogLikelihood(BaseFlowValidationModel):
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corr_mag_eta = sample(
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corr_mag_eta = sample(
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f"corr_mag_eta_{self.name}", Uniform(-1, 1))
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f"corr_mag_eta_{self.name}", Uniform(-1, 1))
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# Jeffrey's prior on the the MNR hyperprior widths.
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ll0 -= jnp.log(mag_std) + jnp.log(eta_std)
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loc = jnp.array([mag_mean, eta_mean])
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loc = jnp.array([mag_mean, eta_mean])
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cov = jnp.array(
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cov = jnp.array(
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[[mag_std**2, corr_mag_eta * mag_std * eta_std],
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[[mag_std**2, corr_mag_eta * mag_std * eta_std],
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