COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring. |
University of Cambridge > Talks.cam > Astro Data Science Discussion Group > Neural ratio estimation: the future of supernova cosmology?
Neural ratio estimation: the future of supernova cosmology?Add to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact David Yallup. Simulation-based inference (SBI) has the potential to revolutionise how we do supernova cosmology and let us incorporate arbitrarily complex effects within a Bayesian model. I will present recent work which sought to validate neural ratio estimation (NRE) by comparing NRE -derived posteriors on supernova properties to those obtained with a likelihood-based MCMC approach for the same data, and then discuss how NRE and SBI in general provide a pathway towards a model extending all the way from type Ia supernova light curves to cosmological parameters as part of a single analysis. This talk is part of the Astro Data Science Discussion Group series. This talk is included in these lists:
Note that ex-directory lists are not shown. |
Other listsJean Monnet - Marie Curie Seminar Series Film Screenings and Talks CaMediaOther talksOperator Algebras A continuous random operator associated with the H^{2|2} model Layering in strongly stratified geophysical and astrophysical turbulence (with Chini, Garaud, Caulfield, Cope) Quantum Groups Hierarchical star cluster assembly boosts intermediate-mass black hole formation |