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Applications of belief propagation in low-level vision

Applications of belief propagation in low-level vision. Bill Freeman Massachusetts Institute of Technology Jan. 12, 2010. Joint work with: Egon Pasztor, Jonathan Yedidia, Yair Weiss, Thouis Jones, Edward Adelson, Marshall Tappen. y 1. x 1. y 2. x 2. y 3. x 3.

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Applications of belief propagation in low-level vision

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  1. Applications of belief propagation in low-level vision Bill Freeman Massachusetts Institute of Technology Jan. 12, 2010 Joint work with: Egon Pasztor, Jonathan Yedidia, Yair Weiss, Thouis Jones, Edward Adelson, Marshall Tappen.

  2. y1 x1 y2 x2 y3 x3 Derivation of belief propagation

  3. y1 y3 y2 x1 x3 x2 The posterior factorizes

  4. y1 y3 y2 x1 x3 x2 Propagation rules

  5. y1 y3 y2 x1 x3 x2 Propagation rules

  6. y1 y3 y2 x1 x3 x2 Propagation rules

  7. Belief propagation messages A message: can be thought of as a set of weights on each of your possible states To send a message: Multiply together all the incoming messages, except from the node you’re sending to, then multiply by the compatibility matrix and marginalize over the sender’s states. = i j j i

  8. Belief propagation: the nosey neighbor rule “Given everything that I’ve heard, here’s what I think is going on inside your house” (Given my incoming messages, affecting my state probabilities, and knowing how my states affect your states, here’s how I think you should modify the probabilities of your states)

  9. Beliefs To find a node’s beliefs: Multiply together all the messages coming in to that node. j (Show this for the toy example.)

  10. Optimal solution in a chain or tree:Belief Propagation • “Do the right thing” Bayesian algorithm. • For Gaussian random variables over time: Kalman filter. • For hidden Markov models: forward/backward algorithm (and MAP variant is Viterbi).

  11. Markov Random Fields • Allows rich probabilistic models for images. • But built in a local, modular way. Learn local relationships, get global effects out.

  12. MRF nodes as pixels Winkler, 1995, p. 32

  13. MRF nodes as patches image patches scene patches image F(xi, yi) Y(xi, xj) scene

  14. Network joint probability 1 Õ Õ = Y F P ( x , y ) ( x , x ) ( x , y ) i j i i Z , i j i scene Scene-scene compatibility function Image-scene compatibility function image neighboring scene nodes local observations

  15. In order to use MRFs: • Given observations y, and the parameters of the MRF, how infer the hidden variables, x? • How learn the parameters of the MRF?

  16. Inference in Markov Random Fields Gibbs sampling, simulated annealing Iterated conditional modes (ICM) Belief propagation Application examples: super-resolution motion analysis shading/reflectance separation Graph cuts Variational methods

  17. Inference in Markov Random Fields Gibbs sampling, simulated annealing Iterated conditional modes (ICM) Belief propagation Application examples: super-resolution motion analysis shading/reflectance separation Graph cuts Variational methods

  18. y1 x1 y2 x2 y3 x3 Derivation of belief propagation

  19. y1 y3 y2 x1 x3 x2 Y ( x , x ) 1 3 No factorization with loops!

  20. Applications of belief propagation in low-level vision Bill Freeman Massachusetts Institute of Technology Jan. 12, 2010 Joint work with: Egon Pasztor, Jonathan Yedidia, Yair Weiss, Thouis Jones, Edward Adelson, Marshall Tappen.

  21. Belief, and message updates j = i j i

  22. Optimal solution in a chain or tree:Belief Propagation • “Do the right thing” Bayesian algorithm. • For Gaussian random variables over time: Kalman filter. • For hidden Markov models: forward/backward algorithm (and MAP variant is Viterbi).

  23. Justification for running belief propagation in networks with loops Kschischang and Frey, 1998; McEliece et al., 1998 • Experimental results: • Error-correcting codes • Vision applications • Theoretical results: • For Gaussian processes, means are correct. • Large neighborhood local maximum for MAP. • Equivalent to Bethe approx. in statistical physics. • Tree-weighted reparameterization Freeman and Pasztor, 1999; Frey, 2000 Weiss and Freeman, 1999 Weiss and Freeman, 2000 Yedidia, Freeman, and Weiss, 2000 Wainwright, Willsky, Jaakkola, 2001

  24. Results from Bethe free energy analysis • Fixed point of belief propagation equations iff. Bethe approximation stationary point. • Belief propagation always has a fixed point. • Connection with variational methods for inference: both minimize approximations to Free Energy, • variational: usually use primal variables. • belief propagation: fixed pt. equs. for dual variables. • Kikuchi approximations lead to more accurate belief propagation algorithms. • Other Bethe free energy minimization algorithms—Yuille, Welling, etc.

  25. References on BP and GBP • J. Pearl, 1985 • classic • Y. Weiss, NIPS 1998 • Inspires application of BP to vision • W. Freeman et al learning low-level vision, IJCV 1999 • Applications in super-resolution, motion, shading/paint discrimination • H. Shum et al, ECCV 2002 • Application to stereo • M. Wainwright, T. Jaakkola, A. Willsky • Reparameterization version • J. Yedidia, AAAI 2000 • The clearest place to read about BP and GBP.

  26. Inference in Markov Random Fields Gibbs sampling, simulated annealing Iterated conditional modes (ICM) Belief propagation Application examples: super-resolution motion analysis shading/reflectance separation Graph cuts Variational methods

  27. image scene Super-resolution • Image: low resolution image • Scene: high resolution image ultimate goal...

  28. Pixel-based images are not resolution independent Pixel replication Cubic spline, sharpened Cubic spline Training-based super-resolution Polygon-based graphics images are resolution independent

  29. 3 approaches to perceptual sharpening amplitude (1) Sharpening; boost existing high frequencies. (2) Use multiple frames to obtain higher sampling rate in a still frame. (3) Estimate high frequencies not present in image, although implicitly defined. spatial frequency amplitude In this talk, we focus on (3), which we’ll call “super-resolution”. spatial frequency

  30. Super-resolution: other approaches • Schultz and Stevenson, 1994 • Pentland and Horowitz, 1993 • fractal image compression (Polvere, 1998; Iterated Systems) • astronomical image processing (eg. Gull and Daniell, 1978; “pixons” http://casswww.ucsd.edu/puetter.html) • Follow-on: Jianchao Yang, John Wright, Thomas S. Huang, Yi Ma: Image super-resolution as sparse representation of raw image patches. CVPR 2008

  31. Training images,~100,000 image/scene patch pairs Images from two Corel database categories: “giraffes” and “urban skyline”.

  32. Do a first interpolation Zoomed low-resolution Low-resolution

  33. Zoomed low-resolution Full frequency original Low-resolution

  34. Representation Zoomed low-freq. Full freq. original

  35. Representation Zoomed low-freq. Full freq. original True high freqs Low-band input (contrast normalized, PCA fitted) (to minimize the complexity of the relationships we have to learn, we remove the lowest frequencies from the input image, and normalize the local contrast level).

  36. Gather ~100,000 patches ... ... high freqs. low freqs. Training data samples (magnified)

  37. Nearest neighbor estimate True high freqs. Input low freqs. Estimated high freqs. ... ... high freqs. low freqs. Training data samples (magnified)

  38. Nearest neighbor estimate Input low freqs. Estimated high freqs. ... ... high freqs. low freqs. Training data samples (magnified)

  39. Example: input image patch, and closest matches from database Input patch Closest image patches from database Corresponding high-resolution patches from database

  40. d Scene-scene compatibility function, Y(xi, xj) Assume overlapped regions, d, of hi-res. patches differ by Gaussian observation noise: Uniqueness constraint, not smoothness.

  41. y Image-scene compatibility function, F(xi, yi) Assume Gaussian noise takes you from observed image patch to synthetic sample: x

  42. Markov network image patches F(xi, yi) scene patches Y(xi, xj)

  43. Belief Propagation After a few iterations of belief propagation, the algorithm selects spatially consistent high resolution interpretations for each low-resolution patch of the input image. Input Iter. 0 Iter. 1 Iter. 3

  44. Cubic spline zoom to 340x204 Max. likelihood zoom to 340x204 Zooming 2 octaves We apply the super-resolution algorithm recursively, zooming up 2 powers of 2, or a factor of 4 in each dimension. 85 x 51 input

  45. Now we examine the effect of the prior assumptions made about images on the high resolution reconstruction. First, cubic spline interpolation. Original 50x58 (cubic spline implies thin plate prior) True 200x232

  46. Original 50x58 (cubic spline implies thin plate prior) True 200x232 Cubic spline

  47. Next, train the Markov network algorithm on a world of random noise images. Original 50x58 Training images True

  48. The algorithm learns that, in such a world, we add random noise when zoom to a higher resolution. Original 50x58 Training images Markov network True

  49. Next, train on a world of vertically oriented rectangles. Original 50x58 Training images True

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