With the advent of future big-data surveys, automated tools for unsupervised discovery are becoming ever more necessary. In this talk I will show how deep generative models can be used to learn a representation of expected data defined by the training set and then look for deviations from the learned representation by looking for the best reconstruction of a given object. We perform several experiments: 1. We first show that we are able to detect ~90% of interacting galaxies if we train our network only with a sample of isolated galaxies. 2. We then explore how the presented approach can be used to compare images of observed and simulated galaxies by identifying real objects not well rendered in the simulations. 3. We, finally, blindly loo...
International audienceEstablishing accurate morphological measurements of galaxies in a reasonable a...
Observations of astrophysical objects such as galaxies are limited by various sources of random and ...
Accepted for publication in MNRAS. Comments welcomeInternational audienceABSTRACT Hydrodynamical sim...
International audienceWith the advent of future big-data surveys, automated tools for unsupervised d...
We examine the capability of generative models to produce realistic galaxy images. We show that mixi...
14 pages, submitted to MNRAS. Comments most welcomeInternational audienceABSTRACT Image simulations ...
We examine the capability of generative models to produce realistic galaxy images. We show that mixi...
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Deep generative models including generative adversarial networks (GANs) are powerful unsupervised to...
This thesis explores four projects applying supervised deep learning to help answer astrophysical qu...
Astronomers have typically set out to solve supervised machine learning problems by creating their o...
We present the data used in "DeepAdversaries: Examining the Robustness of Deep Learning Models for G...
International audienceBlending of galaxies has a major contribution in the systematic error budget o...
Accurately reproducing the morphology of galaxies in our Universe is a crucial test for hydrodynamic...
Machine learning techniques are found to be increasingly useful in analyzing data from large galaxy ...
International audienceEstablishing accurate morphological measurements of galaxies in a reasonable a...
Observations of astrophysical objects such as galaxies are limited by various sources of random and ...
Accepted for publication in MNRAS. Comments welcomeInternational audienceABSTRACT Hydrodynamical sim...
International audienceWith the advent of future big-data surveys, automated tools for unsupervised d...
We examine the capability of generative models to produce realistic galaxy images. We show that mixi...
14 pages, submitted to MNRAS. Comments most welcomeInternational audienceABSTRACT Image simulations ...
We examine the capability of generative models to produce realistic galaxy images. We show that mixi...
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Deep generative models including generative adversarial networks (GANs) are powerful unsupervised to...
This thesis explores four projects applying supervised deep learning to help answer astrophysical qu...
Astronomers have typically set out to solve supervised machine learning problems by creating their o...
We present the data used in "DeepAdversaries: Examining the Robustness of Deep Learning Models for G...
International audienceBlending of galaxies has a major contribution in the systematic error budget o...
Accurately reproducing the morphology of galaxies in our Universe is a crucial test for hydrodynamic...
Machine learning techniques are found to be increasingly useful in analyzing data from large galaxy ...
International audienceEstablishing accurate morphological measurements of galaxies in a reasonable a...
Observations of astrophysical objects such as galaxies are limited by various sources of random and ...
Accepted for publication in MNRAS. Comments welcomeInternational audienceABSTRACT Hydrodynamical sim...