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The Subaru Coronagraphic Extreme Adaptive Optics Imager: First Results and On-Sky Performance

Instrumentation and Methods for Astrophysics 2013-07-17 v1 Earth and Planetary Astrophysics

Abstract

We present new on-sky results for the Subaru Coronagraphic Extreme Adaptive Optics imager (SCExAO) verifying and quantifying the contrast gain enabled by key components: the closed-loop coronagraphic low-order wavefront sensor (CLOWFS) and focal plane wavefront control ("speckle nulling"). SCExAO will soon be coupled with a high-order, Pyramid wavefront sensor which will yield > 90% Strehl ratio and enable 10^6--10^7 contrast at small angular separations allowing us to image gas giant planets at solar system scales. Upcoming instruments like VAMPIRES, FIRST, and CHARIS will expand SCExAO's science capabilities.

Keywords

Cite

@article{arxiv.1307.4093,
  title  = {The Subaru Coronagraphic Extreme Adaptive Optics Imager: First Results and On-Sky Performance},
  author = {Thayne Currie and Olivier Guyon and Frantz Martinache and Christophe Clergeon and Michael McElwain and Christian Thalmann and Nemanja Jovanovic and Garima Singh and Tomoyuki Kudo},
  journal= {arXiv preprint arXiv:1307.4093},
  year   = {2013}
}

Comments

IAU 299/Victoria conference proceedings