activity
20242026
collaborators

6 papers

astro-ph.CO2026

A Simulation Based Inference Approach to Modelling of Type Ia Supernova Populations

B. Popovic, M. Grayling, M. O'Callaghan +12

Type Ia Supernovae (SNe Ia) are prominent cosmological probes, utilising a standardisation process to reduce their observed scatter to mag. A growing number of models se…

astro-ph.CO2026

FlowSN: Neural Simulation-Based Inference under Realistic Selection Effects applied to Supernova Cosmology

Benjamin M. Boyd, Kaisey S. Mandel, Matthew Grayling +10

We present FlowSN, a statistical framework using simulation-based inference (SBI) with normalising flows to account for selection effects in observational astronomy. Failure to acc…

astro-ph.CO2026

On the origin of the environmental step: A BayeSN view of the ZTF SN Ia DR2

Madeleine Ginolin, Matthew Grayling, Kaisey S. Mandel +5

Astrophysical variabilities of Type Ia supernovae (SNe Ia), such as their link with their birth environment, are now one of the leading sources of systematic uncertainties on the m…

stat.ML2025

Misspecification-robust amortised simulation-based inference using variational methods

Matthew O'Callaghan, Kaisey S. Mandel, Gerry Gilmore

Recent advances in neural density estimation have enabled powerful simulation-based inference (SBI) methods that can flexibly approximate Bayesian inference for intractable stochas…

astro-ph.GA2025

Data-driven dust inference at mid-to-high Galactic latitudes using probabilistic machine learning

Matthew O'Callaghan, Kaisey S. Mandel, Gerry Gilmore

We present a method for accurately and precisely inferring photometric dust extinction towards stars at mid-to-high Galactic latitudes using probabilistic machine learning to model…

astro-ph.GA2024

Quantifying Interstellar Extinction at High Galactic Latitudes

Matthew O'Callaghan, Gerry Gilmore, Kaisey S. Mandel

A detailed map of the distribution of dust at high Galactic latitudes is essential for future cosmic microwave background (CMB) polarization experiments because the dust, while dif…