The radial acceleration relation persists at intermediate redshifts but with a characteristic acceleration scale that increases linearly with redshift.
Marginalised Normal Regression: Unbiased curve fitting in the presence of x-errors
3 Pith papers cite this work, alongside 10 external citations. Polarity classification is still indexing.
abstract
The history of the seemingly simple problem of straight line fitting in the presence of both $x$ and $y$ errors has been fraught with misadventure, with statistically ad hoc and poorly tested methods abounding in the literature. The problem stems from the emergence of latent variables describing the "true" values of the independent variables, the priors on which have a significant impact on the regression result. By analytic calculation of maximum a posteriori values and biases, and comprehensive numerical mock tests, we assess the quality of possible priors. In the presence of intrinsic scatter, the only prior that we find to give reliably unbiased results in general is a mixture of one or more Gaussians with means and variances determined as part of the inference. We find that a single Gaussian is typically sufficient and dub this model Marginalised Normal Regression (MNR). We illustrate the necessity for MNR by comparing it to alternative methods on an important linear relation in cosmology, and extend it to nonlinear regression and an arbitrary covariance matrix linking $x$ and $y$. We publicly release a Python/Jax implementation of MNR and its Gaussian mixture model extension that is coupled to Hamiltonian Monte Carlo for efficient sampling, which we call ROXY (Regression and Optimisation with X and Y errors).
representative citing papers
Resolved stellar mass maps from 10-band SED fitting in 19 MIGHTEE-HI galaxies give a radial acceleration relation with intrinsic scatter 0.045 dex, a higher acceleration scale than SPARC, and tentative 2.4-sigma redshift evolution.
A survey claiming to be the first comprehensive review of uncertainty quantification in symbolic regression, organized into three research directions and noting the area remains underexplored.
citing papers explorer
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MUSE-DARK III: The evolution of the radial acceleration relation at intermediate redshifts
The radial acceleration relation persists at intermediate redshifts but with a characteristic acceleration scale that increases linearly with redshift.
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MIGHTEE-HI: The radial acceleration relation with resolved stellar mass measurements
Resolved stellar mass maps from 10-band SED fitting in 19 MIGHTEE-HI galaxies give a radial acceleration relation with intrinsic scatter 0.045 dex, a higher acceleration scale than SPARC, and tentative 2.4-sigma redshift evolution.
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Are you sure? A Comprehensive and Comprehensible Survey of Uncertainty Quantification in Symbolic Regression
A survey claiming to be the first comprehensive review of uncertainty quantification in symbolic regression, organized into three research directions and noting the area remains underexplored.