Back to the Abstract

	1 Introduction
	2 plane coverage
	3 Pupil densification and nulling coronagraphy
	4 Imaging with the phase mask coronagraph applied on a sparse array of telescopes
	5 Planet detection capabilities
	6 Other capabilities
	7 Conclusion
	Appendix A: Performance of the phase mask coronagraph
	Appendix B: Point source detection sensitivity in a snapshot exposure
	References