English

The VORTEX coronagraphic test bench

Instrumentation and Methods for Astrophysics 2016-05-03 v1

Abstract

In this paper, we present the infrared coronagraphic test bench of the University of Li\`ege named VODCA (Vortex Optical Demonstrator for Coronagraphic Applications). The goal of the bench is to assess the performances of the Annular Groove Phase Masks (AGPMs) at near- to mid-infrared wavelengths. The AGPM is a subwavelength grating vortex coronagraph of charge two (SGVC2) made out of diamond. The bench is designed to be completely achromatic and will be composed of a super continuum laser source emitting in the near to mid-infrared, several parabolas, diaphragms and an infrared camera. This way, we will be able to test the different AGPMs in the M, L, K and H bands. Eventually, the bench will also allow the computation of the incident wavefront aberrations on the coronagraph. A reflective Lyot stop will send most of the stellar light to a second camera to perform low-order wavefront sensing. This second system coupled with a deformable mirror will allow the correction of the wavefront aberrations. We also aim to test other pre- and/or post-coronagraphic concepts such as optimal apodization.

Cite

@article{arxiv.1604.08334,
  title  = {The VORTEX coronagraphic test bench},
  author = {Aissa Jolivet and Pierre Piron and Elsa Huby and Olivier Absil and Christian Delacroix and Dimitri Mawet and Jean Surdej and Serge Habraken},
  journal= {arXiv preprint arXiv:1604.08334},
  year   = {2016}
}
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