Successes and challenges of the APP Coronagraph
Abstract
The Apodizing Phase Plate (APP) coronagraph has been used to image the exoplanet β Pictoris b and the protoplanet candidate around HD 100546, and is currently in use in surveys with NaCo at the VLT. Its success is due to its tolerance to tip-tilt pointing errors in current AO systems, which degrade the performance of nearly all other coronagraphs. Currently the sensitivity of the APP is limited by non-common path errors in the science camera systems and by its chromatic behaviour. We present the achromatized Vector APP coronagraph and address how we will measure and minimise non-common path errors with Focal Plane Wavefront Sensing algorithms.
- Publication:
-
Exploring the Formation and Evolution of Planetary Systems
- Pub Date:
- January 2014
- DOI:
- 10.1017/S1743921313007771
- Bibcode:
- 2014IAUS..299...40K
- Keywords:
-
- instrumentation: high angular resolution;
- stars: planetary systems;
- stars: individual (β Pic;
- HD 100546)