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Matt Hoffman

5 accepted papers

2020

Improving the Gating Mechanism of Recurrent Neural Networks

ICML 2020poster

Gating mechanisms are widely used in neural network models, where they allow gradients to backpropagate easily through depth or time. However, their saturation property introduces problems of its own. For example, in recurrent models these gates need to have outputs near 1 to propagate information o…

Cited by 108SourcePDFScholar
2020

Making Efficient Use of Demonstrations to Solve Hard Exploration Problems

ICLR 2020poster

This paper introduces R2D3, an agent that makes efficient use of demonstrations to solve hard exploration problems in partially observable environments with highly variable initial conditions. We also introduce a suite of eight tasks that combine these three properties, and show that R2D3 can solve…

Cited by 107SourceScholar
2019

Audio Texture Synthesis with Random Neural Networks: Improving Diversity and Quality

ICASSP 2019accepted

Texture synthesis techniques based on matching the Gram matrix of feature activations in neural networks have achieved spectacular success in the image domain. In this paper we extend these techniques to the audio domain. We demonstrate that synthesizing diverse audio textures is challenging, and ar…

Cited by 0SourceScholar
2015

A trust-region method for stochastic variational inference with applications to streaming data

ICML 2015poster

Stochastic variational inference allows for fast posterior inference in complex Bayesian models. However, the algorithm is prone to local optima which can make the quality of the posterior approximation sensitive to the choice of hyperparameters and initialization. We address this problem by replaci…

Cited by 41SourcePDFScholar
2015

Celeste: Variational inference for a generative model of astronomical images

ICML 2015poster

We present a new, fully generative model of optical telescope image sets, along with a variational procedure for inference. Each pixel intensity is treated as a Poisson random variable, with a rate parameter dependent on latent properties of stars and galaxies. Key latent properties are themselves r…

Cited by 46SourcePDFScholar