Portrait of Laurence Perreault-Levasseur

Laurence Perreault-Levasseur

Core Academic Member
Assistant Professor, Université de Montréal, Department of Physics
Research Topics
Bayesian Inference
Computer Vision
Deep Learning
Dynamical Systems
Generative Models
Probabilistic Models

Biography

Laurence Perreault-Levasseur is the Canada Research Chair in Computational Cosmology and Artificial Intelligence. She is an assistant professor at Université de Montréal and an associate academic member of Mila – Quebec Artificial Intelligence Institute. Perreault-Levasseur’s research focuses on the development and application of machine learning methods to cosmology.

She is also a Visiting Scholar at the Flatiron Institute in New York City. Prior to that, she was a research fellow at their Center for Computational Astrophysics, and a KIPAC postdoctoral fellow at Stanford University.

For her PhD degree at the University of Cambridge, she worked on applications of open effective field theory methods to the formalism of inflation. She completed her BSc and MSc degrees at McGill University.

Current Students

PhD - Université de Montréal
PhD - McGill University
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PhD - Université de Montréal
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PhD - Université de Montréal
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Postdoctorate - McGill University
Research Intern - Université de Montréal
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PhD - Université de Montréal
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PhD - Université de Montréal
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Research Intern - Université de Montréal
Postdoctorate - Université de Montréal
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PhD - Université de Montréal
PhD - Université de Montréal
Master's Research - Université de Montréal
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PhD - Université de Montréal
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PhD - Université de Montréal
Postdoctorate - McGill University
Master's Research - Université de Montréal
Postdoctorate - Université de Montréal
Principal supervisor :
Postdoctorate - McGill University
Co-supervisor :
Postdoctorate - Université de Montréal
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Publications

Deconvolving X-ray Galaxy Cluster Spectra Using a Recurrent Inference Machine
C. L. Rhea
J. Hlavacek-Larrondo
Ralph P. Kraft
Ákos Bogdán
Recent advances in machine learning algorithms have unlocked new insights in observational astronomy by allowing astronomers to probe new fr… (see more)ontiers. In this article, we present a methodology to disentangle the intrinsic X-ray spectrum of galaxy clusters from the instrumental response function. Employing state-of-the-art modeling software and data mining techniques of the Chandra data archive, we construct a set of 100,000 mock Chandra spectra. We train a recurrent inference machine (RIM) to take in the instrumental response and mock observation and output the intrinsic X-ray spectrum. The RIM can recover the mock intrinsic spectrum below the 1-
Improving Gradient-Guided Nested Sampling for Posterior Inference
We present a performant, general-purpose gradient-guided nested sampling algorithm, …
Assessing the Viability of Generative Modeling in Simulated Astronomical Observations
In this paper, we use methods for assessing the quality of generative models and apply them to a problem from the physical sciences. We turn… (see more) our attention to astrophysics, where cosmological simulations are often used to create mock observations that mimic telescope images. These simulations and their mock observations are often slow and challenging to generate, inspiring some to use generative modeling to enhance the amount of data available to study. In this work, we add realism to simulated images of galaxy clusters and use probability mass estimation to assess their fidelity compared to reality. We find that the simulations are biased compared to real observations and suggest that researchers applying generative modeling to these systems should proceed with caution.
Neural Ratio Estimators Meet Distributional Shift and Mode Misspecification: A Cautionary Tale from Strong Gravitational Lensing
In recent years, there has been increasing interest in the field of astrophysics in applying Neural Ratio Estimators (NREs) to large-scale i… (see more)nference problems where both amortization and marginalization over a large number of nuisance parameters are needed. Here, in order to assess the true potential of this method to produce unbiased inference on real data, we investigate the robustness of NREs to distribution shifts and model misspecification in the specific scientific application of the measurement of dark matter population-level parameters using strong gravitational lensing. We investigate the behaviour of a trained NRE for test data presenting distributional shifts inside the bounds of training, as well as out of distribution, both in the linear and non-linear parameters of this problem. While our results show that NREs perform when tested perfectly in distribution, we find that they exhibit significant biases and drawbacks when confronted with slight deviations from the examples seen in the training distribution. This indicates the necessity for caution when applying NREs to real astrophysical data, where underlying distributions are not perfectly known and models do not perfectly reconstruct the true underlying distributions.
Inpainting Galaxy Counts onto N-Body Simulations over Multiple Cosmologies and Astrophysics
Multi-phase black-hole feedback and a bright [CII] halo in a Lo-BAL quasar at $z\sim6.6$
Manuela Bischetti
Hyunseop 현섭 Choi 최
Fabrizio Fiore
Chiara Feruglio
Stefano Carniani
Valentina D'Odorico
Eduardo Banados
Huanqing Chen
Roberto Decarli
Simona Gallerani
J. Hlavacek-Larrondo
Samuel Lai
Karen M. Leighly
Chiara Mazzucchelli
Roberta Tripodi
Fabian Walter
Feige Wang
Jinyi Yang
Maria Vittoria Zanchettin … (see 1 more)
Yongda Zhu
Caustics: A Python Package for Accelerated Strong Gravitational Lensing Simulations
M. J. Yantovski-Barth
Landung Setiawan
Cordero Core
Charles Wilson
Gabriel Missael Barco
Active learning meets fractal decision boundaries: a cautionary tale from the Sitnikov three-body problem
Mario Pasquato
Alessandro Alberto Trani
Chaotic systems such as the gravitational N-body problem are ubiquitous in astronomy. Machine learning (ML) is increasingly deployed to pred… (see more)ict the evolution of such systems, e.g. with the goal of speeding up simulations. Strategies such as active Learning (AL) are a natural choice to optimize ML training. Here we showcase an AL failure when predicting the stability of the Sitnikov three-body problem, the simplest case of N-body problem displaying chaotic behavior. We link this failure to the fractal nature of our classification problem's decision boundary. This is a potential pitfall in optimizing large sets of N-body simulations via AL in the context of star cluster physics, galactic dynamics, or cosmology.
Bayesian Imaging for Radio Interferometry with Score-Based Priors
No'e Dia
M. J. Yantovski-Barth
Micah Bowles
A. Scaife
U. Montŕeal
Ciela Institute
Flatiron Institute
Learning an Effective Evolution Equation for Particle-Mesh Simulations Across Cosmologies
Unraveling the Mysteries of Galaxy Clusters: Recurrent Inference Deconvolution of X-ray Spectra
C. L. Rhea
J. Hlavacek-Larrondo
Ralph P. Kraft
Ákos Bogdán
The search for the lost attractor
Mario Pasquato
Syphax Haddad
Pierfrancesco Di Cintio
Mircea Petrache
Ugo Niccolò Di Carlo
Alessandro Alberto Trani