A Bayesian Convolutional Neural Network for Robust Galaxy Ellipticity
Regression
- URL: http://arxiv.org/abs/2104.09970v1
- Date: Tue, 20 Apr 2021 14:01:57 GMT
- Title: A Bayesian Convolutional Neural Network for Robust Galaxy Ellipticity
Regression
- Abstract summary: We propose a Convolutional Neural Network to reliably estimate the ellipticity of galaxies.
We show that a convolutional network can be trained to correctly estimate well aleatoric uncertainty, calibrated -- the uncertainty due to the presence of noise in the images -- it is unable to generate a trustworthy ellipticity distribution.
- Score: 5.129856875153228
- License: http://creativecommons.org/publicdomain/zero/1.0/
- Abstract: Cosmic shear estimation is an essential scientific goal for large galaxy
surveys. It refers to the coherent distortion of distant galaxy images due to
weak gravitational lensing along the line of sight. It can be used as a tracer
of the matter distribution in the Universe. The unbiased estimation of the
local value of the cosmic shear can be obtained via Bayesian analysis which
relies on robust estimation of the galaxies ellipticity (shape) posterior
distribution. This is not a simple problem as, among other things, the images
may be corrupted with strong background noise. For current and coming surveys,
another central issue in galaxy shape determination is the treatment of
statistically dominant overlapping (blended) objects. We propose a Bayesian
Convolutional Neural Network based on Monte-Carlo Dropout to reliably estimate
the ellipticity of galaxies and the corresponding measurement uncertainties. We
show that while a convolutional network can be trained to correctly estimate
well calibrated aleatoric uncertainty, -- the uncertainty due to the presence
of noise in the images -- it is unable to generate a trustworthy ellipticity
distribution when exposed to previously unseen data (i.e. here, blended
scenes). By introducing a Bayesian Neural Network, we show how to reliably
estimate the posterior predictive distribution of ellipticities along with
robust estimation of epistemic uncertainties. Experiments also show that
epistemic uncertainty can detect inconsistent predictions due to unknown
blended scenes.
Related papers
- Neural Posterior Estimation for Tomographic Weak Lensing Mass Mapping [4.453455555213445]
We train a deep neural network to map a multiband image to a variational distribution over the underlying tomographic shear and convergence fields.<n>When evaluated on synthetic images from the LSST-DESC DC2 Simulated Sky Survey, NPE produces well-calibrated variational distributions for shear and convergence.
arXiv Detail & Related papers (2026-09-07T18:00:10Z) - Neural Posterior Estimation for Inferring Weak Lensing Shear [3.3301932549351907]
We train a deep neural network to map a simulated multiband image to a variational distribution over the underlying shear field.<n>Once trained, the network accounts for all features present in the simulated images, including potential sources of bias.<n>Results demonstrate that NPE can be a viable shear estimation method in settings where all anticipated features and artifacts can be simulated.
arXiv Detail & Related papers (2026-07-10T18:01:20Z) - Impact of PSF misestimation and galaxy population bias on precision
shear measurement using a CNN [0.0]
We investigate the application of convolutional neural networks (CNNs) to precision shear estimation.
We simulate a population of noisy disk and elliptical galaxies and adopt a PSF that is representative of a Euclid-like survey.
We quantify the accuracy achieved by the CNN assuming a linear relationship between the estimated and true shears.
arXiv Detail & Related papers (2024-02-04T18:06:39Z) - Calibrating Neural Simulation-Based Inference with Differentiable
Coverage Probability [50.44439018155837]
We propose to include a calibration term directly into the training objective of the neural model.
By introducing a relaxation of the classical formulation of calibration error we enable end-to-end backpropagation.
It is directly applicable to existing computational pipelines allowing reliable black-box posterior inference.
arXiv Detail & Related papers (2023-10-20T10:20:45Z) - Posterior samples of source galaxies in strong gravitational lenses with
score-based priors [107.52670032376555]
We use a score-based model to encode the prior for the inference of undistorted images of background galaxies.
We show how the balance between the likelihood and the prior meet our expectations in an experiment with out-of-distribution data.
arXiv Detail & Related papers (2022-11-07T19:00:42Z) - Inferring Structural Parameters of Low-Surface-Brightness-Galaxies with
Uncertainty Quantification using Bayesian Neural Networks [70.80563014913676]
We show that a Bayesian Neural Network (BNN) can be used for the inference, with uncertainty, of such parameters from simulated low-surface-brightness galaxy images.
Compared to traditional profile-fitting methods, we show that the uncertainties obtained using BNNs are comparable in magnitude, well-calibrated, and the point estimates of the parameters are closer to the true values.
arXiv Detail & Related papers (2022-07-07T17:55:26Z) - Deep Bayesian inference for seismic imaging with tasks [0.6445605125467573]
We propose to use techniques from Bayesian inference and deep neural networks to translate uncertainty in seismic imaging to uncertainty in tasks performed on the image.
A systematic approach is proposed to translate uncertainty due to noise in the data to confidence intervals of automatically tracked horizons in the image.
arXiv Detail & Related papers (2021-10-10T15:25:44Z) - Estimating and Exploiting the Aleatoric Uncertainty in Surface Normal
Estimation [25.003116148843525]
Surface normal estimation from a single image is an important task in 3D scene understanding.
In this paper, we address two limitations shared by the existing methods: the inability to estimate the aleatoric uncertainty and lack of detail in the prediction.
We present a novel decoder framework where pixel-wise perceptrons are trained on a subset of pixels sampled based on the estimated uncertainty.
arXiv Detail & Related papers (2021-09-20T23:30:04Z) - Improving Uncertainty Calibration via Prior Augmented Data [56.88185136509654]
Neural networks have proven successful at learning from complex data distributions by acting as universal function approximators.
They are often overconfident in their predictions, which leads to inaccurate and miscalibrated probabilistic predictions.
We propose a solution by seeking out regions of feature space where the model is unjustifiably overconfident, and conditionally raising the entropy of those predictions towards that of the prior distribution of the labels.
arXiv Detail & Related papers (2021-02-22T07:02:37Z) - The Hidden Uncertainty in a Neural Networks Activations [105.4223982696279]
The distribution of a neural network's latent representations has been successfully used to detect out-of-distribution (OOD) data.
This work investigates whether this distribution correlates with a model's epistemic uncertainty, thus indicating its ability to generalise to novel inputs.
arXiv Detail & Related papers (2020-12-05T17:30:35Z) - Learnable Uncertainty under Laplace Approximations [65.24701908364383]
We develop a formalism to explicitly "train" the uncertainty in a decoupled way to the prediction itself.
We show that such units can be trained via an uncertainty-aware objective, improving standard Laplace approximations' performance.
arXiv Detail & Related papers (2020-10-06T13:43:33Z) - Uncertainty quantification in imaging and automatic horizon tracking: a
Bayesian deep-prior based approach [0.5156484100374059]
Uncertainty quantification (UQ) deals with a probabilistic description of the solution nonuniqueness and data noise sensitivity.
In this paper, we focus on how UQ trickles down to horizon tracking for the determination of stratigraphic models.
arXiv Detail & Related papers (2020-04-01T04:26:33Z) - A deep-learning based Bayesian approach to seismic imaging and
uncertainty quantification [0.4588028371034407]
Uncertainty is essential when dealing with ill-conditioned inverse problems.
It is often not possible to formulate a prior distribution that precisely encodes our prior knowledge about the unknown.
We propose to use the functional form of a randomly convolutional neural network as an implicit structured prior.
arXiv Detail & Related papers (2020-01-13T23:46:18Z)
This list is automatically generated from the titles and abstracts of the papers in this site.
This site does not guarantee the quality of this site (including all information) and is not responsible for any consequences.