The future astronomical imaging surveys are set to provide precise constraints on cosmological parameters, such as dark energy. However, production of synthetic data for these surveys, to test and validate analysis methods, suffers from a very high computational cost. In particular, generating mock galaxy catalogs at sufficiently large volume and high resolution will soon become computationally unreachable. In this paper, we address this problem with a Deep Generative Model to create robust mock galaxy catalogs that may be used to test and develop the analysis pipelines of future weak lensing surveys. We build our model on a custom built Graph Convolutional Networks, by placing each galaxy on a graph node and then connecting the graphs with...
Understanding the nature of dark energy, the mysterious force driving the accelerated expansion of t...
We present an implicit likelihood approach to quantifying cosmological information over discrete cat...
International audienceNext generation telescopes, like Euclid, Rubin/LSST, and Roman, will open new ...
We train deep learning models on thousands of galaxy catalogues from the state-of-the-art hydrodynam...
International audienceABSTRACT In order to prepare for the upcoming wide-field cosmological surveys,...
Deep generative models including generative adversarial networks (GANs) are powerful unsupervised to...
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Upcoming cosmological weak lensing surveys are expected to constrain cosmological parameters with un...
We examine the capability of generative models to produce realistic galaxy images. We show that mixi...
Galaxies play a key role in our endeavor to understand how structure formation proceeds in the Unive...
14 pages, submitted to MNRAS. Comments most welcomeInternational audienceABSTRACT Image simulations ...
Accepted for publication in MNRAS. Comments welcomeInternational audienceABSTRACT Hydrodynamical sim...
We examine the capability of generative models to produce realistic galaxy images. We show that mixi...
Understanding the nature of dark energy, the mysterious force driving the accelerated expansion of t...
We present an implicit likelihood approach to quantifying cosmological information over discrete cat...
International audienceNext generation telescopes, like Euclid, Rubin/LSST, and Roman, will open new ...
We train deep learning models on thousands of galaxy catalogues from the state-of-the-art hydrodynam...
International audienceABSTRACT In order to prepare for the upcoming wide-field cosmological surveys,...
Deep generative models including generative adversarial networks (GANs) are powerful unsupervised to...
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Upcoming cosmological weak lensing surveys are expected to constrain cosmological parameters with un...
We examine the capability of generative models to produce realistic galaxy images. We show that mixi...
Galaxies play a key role in our endeavor to understand how structure formation proceeds in the Unive...
14 pages, submitted to MNRAS. Comments most welcomeInternational audienceABSTRACT Image simulations ...
Accepted for publication in MNRAS. Comments welcomeInternational audienceABSTRACT Hydrodynamical sim...
We examine the capability of generative models to produce realistic galaxy images. We show that mixi...
Understanding the nature of dark energy, the mysterious force driving the accelerated expansion of t...
We present an implicit likelihood approach to quantifying cosmological information over discrete cat...
International audienceNext generation telescopes, like Euclid, Rubin/LSST, and Roman, will open new ...