activity
20162026
most citedNo evidence for extensions to the standard cosmological model

169 citations · 353 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2026

KiDS+VIKING-450 cosmology with Bayesian hierarchical model redshift distributions

George T. Kyriacou, Arrykrishna Mootoovaloo, Alan F. Heavens +3

Tomographic redshift distributions from photometric data are crucial ingredients in cosmic shear analysis, since they are required for the theoretical calculation of the signal bas…

astro-ph.CO2024★ 1 cited

: Normalising Flows for Joint Cosmological Analysis

Arrykrishna Mootoovaloo, Carlos García-García, David Alonso +1

Given the growth in the variety and precision of astronomical datasets of interest for cosmology, the best cosmological constraints are invariably obtained by combining data from d…

astro-ph.IM2024★ 1 cited

Assessment of Gradient-Based Samplers in Standard Cosmological Likelihoods

Arrykrishna Mootoovaloo, Jaime Ruiz-Zapatero, Carlos García-García +1

We assess the usefulness of gradient-based samplers, such as the No-U-Turn Sampler (NUTS), by comparison with traditional Metropolis-Hastings algorithms, in tomographic $3 \times 2…

astro-ph.IM2023

Extreme data compression for Bayesian model comparison

Alan F. Heavens, Arrykrishna Mootoovaloo, Roberto Trotta +1

We develop extreme data compression for use in Bayesian model comparison via the MOPED algorithm, as well as more general score compression. We find that Bayes factors from data co…

astro-ph.CO2023★ 17 cited

Analytical marginalisation over photometric redshift uncertainties in cosmic shear analyses

Jaime Ruiz-Zapatero, Boryana Hadzhiyska, David Alonso +3

As the statistical power of imaging surveys grows, it is crucial to account for all systematic uncertainties. This is normally done by constructing a model of these uncertainties a…

astro-ph.CO2021★ 35 cited

Kernel-Based Emulator for the 3D Matter Power Spectrum from CLASS

Arrykrishna Mootoovaloo, Andrew H. Jaffe, Alan F. Heavens +1

The 3D matter power spectrum, is a fundamental quantity in the analysis of cosmological data such as large-scale structure, 21cm observations, and weak lensing. Existing…

astro-ph.CO2020★ 27 cited

Parameter Inference for Weak Lensing using Gaussian Processes and MOPED

Arrykrishna Mootoovaloo, Alan F. Heavens, Andrew H. Jaffe +1

In this paper, we propose a Gaussian Process (GP) emulator for the calculation of a) tomographic weak lensing band-power spectra, and b) coefficients of summary data massively comp…

astro-ph.IM2020★ 38 cited

Imbalance Learning for Variable Star Classification

Zafiirah Hosenie, Robert Lyon, Benjamin Stappers +2

The accurate automated classification of variable stars into their respective sub-types is difficult. Machine learning based solutions often fall foul of the imbalanced learning pr…

astro-ph.IM2019★ 35 cited

Comparing Multi-class, Binary and Hierarchical Machine Learning Classification schemes for variable stars

Zafiirah Hosenie, Robert Lyon, Benjamin Stappers +1

Upcoming synoptic surveys are set to generate an unprecedented amount of data. This requires an automatic framework that can quickly and efficiently provide classification labels f…

stat.CO2017★ 29 cited

Marginal Likelihoods from Monte Carlo Markov Chains

Alan Heavens, Yabebal Fantaye, Arrykrishna Mootoovaloo +4

In this paper, we present a method for computing the marginal likelihood, also known as the model likelihood or Bayesian evidence, from Markov Chain Monte Carlo (MCMC), or other sa…

astro-ph.CO2017★ 169 cited

No evidence for extensions to the standard cosmological model

Alan Heavens, Yabebal Fantaye, Elena Sellentin +4

We compute the Bayesian Evidence for models considered in the main analysis of Planck cosmic microwave background data. By utilising carefully-defined nearest-neighbour distances i…

astro-ph.IM2016★ 1 cited

Bayes Factors via Savage-Dickey Supermodels

A. Mootoovaloo, Bruce A. Bassett, M. Kunz

We outline a new method to compute the Bayes Factor for model selection which bypasses the Bayesian Evidence. Our method combines multiple models into a single, nested, Supermodel…