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Deep Vacuum Cleaner

Deep Vacuum Cleaner

Deconvolving radio astronomy images using a convolution network.

Gijs Molenaar

August 02, 2018
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  1. Deep Learning, why? • Deep learning seems to perform well

    on image to image tasks • Using convolution network for learning inverse of convolution • Can learn any function given enough nodes in hidden layer • Recursive networks are Turing complete • Interesting to get experience with
  2. generative adversarial U- shape auto encoder network • Actually 2

    networks • Generator • Discriminator (used during training)
  3. In short • Works on Linux, OS X (Containers) •

    Implicit parallelisation • Support for various schedulers (Slurm, Mesos) • Open Standard
  4. Training data • Deep learning usually needs a lot of

    data • Point sources only • 256x256 fits • 2000 Meerkat16 datasets • We can flip and rotate those! Boom, more data. • Randomised: sky position, synthesis time, channel width, fluxes
  5. What (doesn’t) works • All bright sources found • PSF

    independent • Fluxes are wrong • Network is good at generating images that ‘look like’ what we want
  6. Experiment PSF • Add PSF to network as channel •

    Network converges faster • Probably only helps in center of image
  7. Time performance • Deconvolving deep2 image • 1089 tiles •

    30 seconds total • 10 seconds ‘warming up’ • 20 ms per tile • Exported model is about 100 megabytes
  8. Future work • Better train data • Try different architecture

    • Infrastructure is there • Collaborate with Deep Learning experts • Recurrent Inference Machines for Solving Inverse function ill- posed problems • https://arxiv.org/abs/ 1706.04008
  9. Fin