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Article Contents
1 Introduction
2 Wave propagation
3 Intensity variance and other fourth moments of the wavefield
4 Lensing by a power law mass spectrum
5 The contribution from stars and other discrete objects
6 Power spectrum of intensity fluctuations from stellar lensing
7 Signatures of lensing and magnitude estimates
8 Conclusions
References
Online Material
Appendix A: The structure function for a power law spectrum
Appendix B: Characteristics of lensing by a power law mass spectrum
Appendix C: Calculation of the temporal intensity fluctuation spectrum for lensing by stars

List of figures

Copyright ESO 2007
Published by EDP Sciences