Laboratory validation of the dual-zone phase mask coronagraph in broadband light at the high-contrast imaging THD-testbed
arXiv:1605.08523 · doi:10.1051/0004-6361/201628587
Abstract
Specific high contrast imaging instruments are mandatory to characterize circumstellar disks and exoplanets around nearby stars. Coronagraphs are commonly used in these facilities to reject the diffracted light of an observed star and enable the direct imaging and spectroscopy of its circumstellar environment. One important property of the coronagraph is to be able to work in broadband light. Among several proposed coronagraphs, the dual-zone phase mask coronagraph is a promising solution for starlight rejection in broadband light. In this paper, we perform the first validation of this concept in laboratory. First, we recall the principle of the dual-zone phase mask coronagraph. Then, we describe the high-contrast imaging THD testbed, the manufacturing of the components and the quality-control procedures. Finally, we study the sensitivity of our coronagraph to low-order aberrations (inner working angle and defocus) and estimate its contrast performance. Our experimental broadband light results are compared with numerical simulations to check agreement with the performance predictions. With the manufactured prototype and using a dark hole technique based on the self-coherent camera, we obtain contrast levels down to between 5 and 17 in monochromatic light (640 nm). We also reach contrast levels of between 7 and 17 in broadband ( nm, nm and %), which demonstrates the excellent chromatic performance of the dual-zone phase mask coronagraph. The performance reached by the dual-zone phase mask coronagraph is promising for future high-contrast imaging instruments that aim at detecting and spectrally characterizing old or light gaseous planets.
9 pages, 16 figures
References in corpus (4)
- Wavefront error correction and Earth-like planet detection by Self-Coherent Camera in space
- Apodized pupil Lyot coronagraphs for arbitrary apertures. V. Hybrid Shaped Pupil designs for imaging Earth-like planets with future space observatories
- Focal plane wavefront sensor achromatization : The multireference self-coherent camera
- Apodization in high-contrast long-slit spectroscopy. II. Concept validation and first on-sky results with VLT/SPHERE
Cited by in corpus (5)
- Atmospheric characterization of Proxima b by coupling the Sphere high-contrast imager to the Espresso spectrograph
- Imaging exoplanets with coronagraphic instruments
- Active minimization of non-common path aberrations in long-exposure imaging of exoplanetary systems
- Apodized Pupil Lyot Coronagraphs with arbitrary aperture telescopes: novel designs using hybrid focal plane masks
- Extended Linearity in the High-Order Wavefront Sensor for the Roman Coronagraph