Paris workshop on Bayesian Deep Learning for Cosmology and Time Domain Astrophysics 3rd ed.

Session

Static sky cosmology

21 mai 2025, 14:00

Buffon Amphitheater (Université Paris Cité)

12. Using AI to probe the invisible universe: machine learning methods for weak gravitational lensing

Samuel Farrens (CosmoStat, CEA Paris-Saclay)

21/05/2025 14:00

Talk

Keynote talk + discussion session

27. Outliers and Hidden Relations in Galaxy Spectroscopy and Photometry

Peter Melchior (Princeton University)

21/05/2025 15:30

Talk

I will present the neural network architect "spender", which is specifically designed for galaxy spectra at variable redshifts. Trained in 500k SDSS or DESI spectra, it is capable of automatically detecting highly meaningful outliers as well as making predictions of the physical state of the galaxies, thus serving as a summary for simulation-based inference approaches. Recently, my group has...

29. Pixel level Bayesian analysis of PSFs and Strong Gravitational Lenses

Connor Stone (Université de Montréal)

21/05/2025 15:50

Talk

Score Based Diffusion models have emerged as a powerful tool for high dimensional Bayesian analysis. Here we present work done at the Université de Montréal to analyze strong gravitational lenses. As a first step, we sample robust posteriors over high resolution point spread function models to represent the image distortions in the Hubble Space Telescope. We then perform source reconstruction...

6. Learning to Deblend Galaxies from Blended Observations with Diffusion Models

Benjamin Remy (Princeton University)

21/05/2025 16:10

Cosmology

Talk

Galaxy surveys such as LSST require robust deblending methods to separate overlapping sources in crowded fields, a challenging inverse problem due to PSF convolution, noise, and source mixing. In this talk, I present a Bayesian framework that leverages diffusion models to learn a prior on galaxy light profiles directly from blended observations. Building on a recent expectation-maximization...

8. Probabilistic inference of galaxy properties using multi-modal variational autoencoders

Kirill Grishin (Universite de Paris)

23/05/2025 09:05

ML Tools

Talk

Variational autoencoders (VAEs) are powerful tools for inferring object properties, particularly well-suited for processing imaging data due to their architectural design. In this work, we use multi-modal VAEs to generate probability distributions for various galaxy properties using multi-band photometric observations. The VAE is trained on synthetic photometric and spectral datasets to infer...

9. Interpretable Machine Learning for Constraining Self-Interacting Dark Matter in Galaxy Clusters

Ethan Tregidga (EPFL)

23/05/2025 09:25

Cosmology

Talk

Cold dark matter, the standard cosmological model, faces several challenges on small scales that self-interacting dark matter may help resolve. Traditional methods to constrain the nature of dark matter often rely on summary statistics, which discard much of the available information, or require complex and computationally expensive lensing models. Machine learning (ML) has gained traction in...

10. Hybrid Analytical-Deep Solver for reconstructing maps in Cosmology

Leonora Kardum

23/05/2025 09:45

Cosmology

Talk

The revolutionary methods of Machine Learning (ML) support most data science analyses today in many ways. An often neglected question remains on the interpretability of used models, and clarity on how the information inside our data is used. This work presents a physics-guided method combined with the architecture of Deep Learning, to provide both the reliability and explainability of...

11. A Comprehensive Analysis of Beyond \(\Lambda\)CDM with Cosmological Data

Dr Shambel Akalu (Centre for Space Research, North-West University)

23/05/2025 10:05

Cosmology

Talk

In this talk the discrepancies include the long-standing difference in the Hubble constant ( H_0 ), as well as variations between Planck data and weak lensing measurements regarding the matter-energy density ( \Omega_m ) and the amplitude ( \sigma_8 ) (or the redshift space distortion ( f \sigma_8 )) of cosmic structures will be explored. These inconsistencies suggest the possibility...

18. Concluding Talk - Bayesian Analysis of Multi-Channel Astronomical Data: From Time Domain to Static Sciences

Biswajit Biswas (APC)

23/05/2025 10:55

Talk

keynote talk + discussion