The Dawn of Pulsar Timing Array Gravitational-Wave Astronomy

The Dawn of Pulsar Timing Array Gravitational-Wave Astronomy

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Multimessengers

18 of 37

18 of 37

Multimessengers

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The Dawn of Pulsar Timing Array Gravitational-Wave Astronomy

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  1. 1 Introduction
  2. 2 Pulsars
  3. 3 Pulsar Timing Array
  4. 4 Helens Bounce Curve
  5. 5 Sources
  6. 6 Who are we
  7. 7 A brief aside on terminology
  8. 8 The history of Pulsar limits
  9. 9 Pulsar detection
  10. 10 Common Spectrum Process
  11. 11 Background Issues
  12. 12 Cross Correlations
  13. 13 Road Ahead
  14. 14 Spectral Characterization
  15. 15 Directional Power
  16. 16 Continuous Wave Signals
  17. 17 Bayesian Limits
  18. 18 Multimessengers
  19. 19 Other Sources
  20. 20 Overview
  21. 21 Thanks Steve
  22. 22 Detection prospects for a single stochastic background
  23. 23 When can we expect to meet a robust detection
  24. 24 The source of the gravitational wave background
  25. 25 The spectrum of the background
  26. 26 Analyzing the background
  27. 27 Detecting the second background
  28. 28 Limitations of power law
  29. 29 constraining an isotopy
  30. 30 choosing a basis
  31. 31 Decision threshold
  32. 32 Signal to noise
  33. 33 Signal to noise statistic
  34. 34 Decision threshold evolution
  35. 35 Summary
  36. 36 Questions
  37. 37 Targeted PTA validation

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