activity
20102026
most citedConsistency of the Adaptive Multiple Importance Sampling

23 citations · 118 across the 21 of their papers we have counts for

collaborators

23 papers

astro-ph.CO2026★ 1 cited

Owl-z: a Bayesian tool to select z \geq 7 quasars

Meriam Ezziati, Roser Pello, Jean-Gabriel Cuby +9

This paper presents Owl-z, a Bayesian code aiming at identifying z \geq 7 quasars in wide field optical and near-infrared surveys. By construction,the code can also be used to sele…

stat.ME2025

Reconciling Binary Replicates: Beyond the Average

Manuela Royer-Carenzi, Hadrien Lorenzo, Pierre Pudlo

Binary observations are often repeated to improve data quality, creating technical replicates. Several scoring methods are commonly used to infer the actual individual state and ob…

math.AP2024

A continuous approach of modeling tumorigenesis and axons regulation for the pancreatic cancer

Marie-Jose Chaaya, Sophie Chauvet, Florence Hubert +3

The pancreatic innervation undergoes dynamic remodeling during the development of pancreatic ductal adenocarcinoma (PDAC). Denervation experiments have shown that different types o…

cs.SD2023★ 1 cited

Detection and classification of vocal productions in large scale audio recordings

Guillem Bonafos, Pierre Pudlo, Jean-Marc Freyermuth +4

We propose an automatic data processing pipeline to extract vocal productions from large-scale natural audio recordings and classify these vocal productions. The pipeline is based…

stat.CO2022

Tempered, Anti-trunctated, Multiple Importance Sampling

Grégoire Aufort, Pierre Pudlo, Denis Burgarella

Importance sampling is a Monte Carlo method that introduces a proposal distribution to sample the space according to the target distribution. Yet calibration of the proposal distri…

astro-ph.GA2020★ 23 cited

Constraining the recent star formation history of galaxies : an Approximate Bayesian Computation approach

G. Aufort, L. Ciesla, P. Pudlo +1

[Abridged] Although galaxies are found to follow a tight relation between their star formation rate and stellar mass, they are expected to exhibit complex star formation histories…