We present an implicit likelihood approach to quantifying cosmological information over discrete catalogue data, assembled as graphs. To do so, we explore cosmological inference using mock dark matter halo catalogues. We employ Information Maximising Neural Networks (IMNNs) to quantify Fisher information extraction as a function of graph representation. We a) demonstrate the high sensitivity of modular graph structure to the underlying cosmology in the noise-free limit, b) show that networks automatically combine mass and clustering information through comparisons to traditional statistics, c) demonstrate that graph neural networks can still extract information when catalogues are subject to noisy survey cuts, and d) illustrate how nonlinea...
Understanding the halo-galaxy connection is fundamental in order to improve our knowledge on the nat...
The new generation of galaxy surveys will provide unprecedented data allowing us to test gravity at ...
The standard approach to inference from cosmic large-scale structure data employs summary statistics...
We train deep learning models on thousands of galaxy catalogues from the state-of-the-art hydrodynam...
We present a novel approach for estimating cosmological parameters, $\Omega_m$, $\sigma_8$, $w_0$, a...
International audienceCompressing large data sets to a manageable number of summaries that are infor...
The future astronomical imaging surveys are set to provide precise constraints on cosmological param...
The standard model of cosmology describes the complex large scale structure of the Universe through ...
Cosmological studies of large-scale structure have relied on two-point statistics, not fully exploit...
In this thesis work we exploited two alternative ML-based techniques to put constraints on the matte...
[Abridged] Galaxy clusters are the most massive gravitationally-bound systems in the universe and ar...
Recent application of the Bayesian algorithm \textsc{borg} to the Sloan Digital Sky Survey (SDSS) ma...
We present a set of maps classifying regions of the sky according to their information gain potentia...
We present \textsc{C}lassification of \textsc{C}luster \textsc{Ga}laxy \textsc{Me}mbers (\textsc{C$^...
The future 21 cm intensity mapping observations constitute a promising way to trace the matter distr...
Understanding the halo-galaxy connection is fundamental in order to improve our knowledge on the nat...
The new generation of galaxy surveys will provide unprecedented data allowing us to test gravity at ...
The standard approach to inference from cosmic large-scale structure data employs summary statistics...
We train deep learning models on thousands of galaxy catalogues from the state-of-the-art hydrodynam...
We present a novel approach for estimating cosmological parameters, $\Omega_m$, $\sigma_8$, $w_0$, a...
International audienceCompressing large data sets to a manageable number of summaries that are infor...
The future astronomical imaging surveys are set to provide precise constraints on cosmological param...
The standard model of cosmology describes the complex large scale structure of the Universe through ...
Cosmological studies of large-scale structure have relied on two-point statistics, not fully exploit...
In this thesis work we exploited two alternative ML-based techniques to put constraints on the matte...
[Abridged] Galaxy clusters are the most massive gravitationally-bound systems in the universe and ar...
Recent application of the Bayesian algorithm \textsc{borg} to the Sloan Digital Sky Survey (SDSS) ma...
We present a set of maps classifying regions of the sky according to their information gain potentia...
We present \textsc{C}lassification of \textsc{C}luster \textsc{Ga}laxy \textsc{Me}mbers (\textsc{C$^...
The future 21 cm intensity mapping observations constitute a promising way to trace the matter distr...
Understanding the halo-galaxy connection is fundamental in order to improve our knowledge on the nat...
The new generation of galaxy surveys will provide unprecedented data allowing us to test gravity at ...
The standard approach to inference from cosmic large-scale structure data employs summary statistics...