Back to the Abstract

	1 Introduction
	2 The MS 2137.3-2353 lens configuration
	3 The dark matter distribution in MS 2137.3-2353
	4 Discussion
	5 Conclusion
	Appendix A: Table of identified dots
	Appendix B: Analytical constraints on generalized-NFW profiles
	Appendix C: Adding haloes of galaxies as substructures
	References

	List of tables
	List of figures