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Pre-seminar What is ML? Geneva University , Jan, 2020 What is Machine learning? What is Dimensionality reduction? What is Clustering Analysis? What am I doing with ML? What is Machine learning? Classification vs. regression


  1. Pre-seminar What is ML? Geneva University , Jan, 2020

  2. ● What is Machine learning? ● What is Dimensionality reduction? ● What is Clustering Analysis? ● What am I doing with ML?

  3. What is Machine learning?

  4. Classification vs. regression

  5. Supervised vs Unsupervised

  6. What is Dimensionality reduction?

  7. What is Clustering Analysis?

  8. What am I doing with ML?

  9. RFI mitigation

  10. Inpaintjng CMB

  11. Inpaintjng CMB

  12. Inpaintjng CMB

  13. Medical physics

  14. Mining cosmic datasets +some cool DS stufg Alireza Vafaei Sadr IPM, Tehran Geneva University , Jan, 2020

  15. Outline  Cosmology and BIG data  A Quick Review of Applicatjons  Anomaly detectjon  DRAMA  Future directjons

  16. Cosmology/Astrophysics E. Siegel, with images derived from ESA/Planck and the DoE/NASA/ NSF interagency task force on CMB research. From his book, Beyond The Galaxy.

  17. Cosmology and Big data

  18. It is getting hotter! Number of physics submitted manuscripts that include “machine learning” in their abstracts.

  19. A quick review on what people have done

  20. Classifjcatjon htup://cdn.spacetelescope.org/archives/images/screen/heic9902o.jpg

  21. Galaxy zoo challenge htups://www.galaxyzoo.org/

  22. Detectjon

  23. Data cleansing

  24. Simulatjon

  25. htups://towardsdatascience.com/do-gans-really-model-the-true-data-distributjon-or-are-they-just-cleverly-fooling-us-d08df69f25eb

  26. htups://arxiv.org/pdf/1905.08233v1.pdf

  27. Anomaly detectjon The light from quasar pairs reach Earth, although some were absorbed by the gas in the cosmic web, Springel et al. (2005) (cosmic web) / J. Neidel, MPIA

  28. 10

  29. Norris, R. P. (2017). Discovering the unexpected in astronomical survey data. Publications of the Astronomical Society of Australia , 34 .

  30. Current projects in SKA (MeerKAT) DS team:  Source detection (Mightee, SKAch-I)  Anomaly detection WTF, PLAsTiCC  RFI simulatjon/mitjgatjon  Extended source simulation  Observation strategy

  31. A. Vafaei Sadr, B. Bassetu, M. Kunz ISCMI-2019

  32. No Free Lunch Theorems  Any two optjmizatjon algorithms are equivalent when their performance is averaged across all possible problems  No anomaly detectjon algorithm works for all anomalies  No anomaly algorithm is “best” on average.  Difgerent algorithms work for difgerent anomalies  So lets consider families of anomaly algorithms

  33. Dimensionality Reductjon Anomaly Meta Algorithm htups://github.com/vafaei-ar/drama

  34. Dimensionality reductjon

  35. Clustering

  36. As an example: MNIST

  37. DRAMA (Dimensionality Reductjon Anomaly Meta-Algorithm):

  38. Dimensionality Reduction T echnique • Autoencoder • Variational autoencoder • principal component analysis • independent component analysis • non negative matrix factorization Also newly added: • Convolutjonal (V)AE (1D) • Convolutjonal (V)AE (2D) • Convolutjonal UMAP

  39. Clustering

  40. Clustering

  41. Distance metrics

  42. Comparison with LOF and i-forest: Simulated Real

  43. Benchmark metrics:

  44. AE, VAE, PCA, ICA, NMF, …? L1, L2, L4, Chebyshev, Canbera, …? Semi-supervised or actjve learning DRAMA vs. LOF vs. iforest

  45. Local anomaly in low dimension n f =100

  46. New class anomaly in low dimension n f =100

  47. Local anomaly in high dimension n f =3000

  48. New class anomaly in high dimension n f =3000

  49. Averaged on real data

  50. Widefield ouTlier Finder (WTF) Includes 337 boring objects and 17 interesting AUC: 87 MCC: 26 RWS: 31 interesting boring

  51. Future directjons • 2D convolutjons • PLAsTiCC (Kaggle competjtjons) • Deep learning based clustering • Graphical user interface • Actjve learning mode • Detect and classify • ...

  52. Thanks for your attention. You can fjnd DRAMA here htups://github.com/vafaei-ar/drama

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