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Proceedings Article

Planet detection down to a few λ/D: an RSDI/TLOCI approach to PSF subtraction

[+] Author Affiliations
Benjamin L. Gerard

Univ. of Victoria (Canada)

Christian Marois

National Research Council of Canada (Canada)

Proc. SPIE 9909, Adaptive Optics Systems V, 990958 (July 27, 2016); doi:10.1117/12.2231905
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From Conference Volume 9909

  • Adaptive Optics Systems V
  • Enrico Marchetti; Laird M. Close; Jean-Pierre Véran
  • Edinburgh, United Kingdom | June 26, 2016

abstract

Most current high contrast imaging point spread function (PSF) subtraction algorithms use some form of a least-squares noise minimization to find exoplanets that are, before post-processing, often hidden below the instrumental speckle noise. In the current standard PSF subtraction algorithms, a set of reference images is derived from the target image sequence to subtract each target image, using Angular and/or Simultaneous Spectral Differential Imaging (ADI, SSDI, respectively). However, to avoid excessive exoplanet self-subtraction, ADI and SSDI (in the absence of a strong spectral feature) severely limit the available number of reference images at small separations. This limits the performance of the least-squares algorithm, resulting in lower sensitivity to exoplanets at small angular separations. Possible solutions are to use additional reference images by acquiring longer sequences, use SSDI if the exoplanet is expected to show strong spectral features, or use images acquired on other targets. The latter option, known as Reference Star Differential Imaging (RSDI), which relies on the use of reference images that are highly correlated to the target image, has been ineffective in previous ground-based high contrast imaging surveys. The now >200 target reference library from the Gemini Planet Imager Exoplanet Survey (GPIES) allows for a detailed RSDI analysis to possibly improve contrast performance near the focal plane mask, at ∼2-7λ/D separations. We present the results of work to optimize PSF subtraction with the GPIES reference library using a least-squares algorithm designed to minimize speckle noise and maximize planet throughput, thus maximizing the planet signal to noise ratio (SNR). Using December 2014 51 Eri GPI data in the inner 100 mas to 300 mas annulus, we find no apparent improvement in SNR when using RSDI and/or our optimization scheme. This result, while still being investigated, seems to show that current algorithms on ADI+SSDI data sets are optimized, and that limited gains can be achieved by using a PSF archive. © (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Citation

Benjamin L. Gerard and Christian Marois
" Planet detection down to a few λ/D: an RSDI/TLOCI approach to PSF subtraction ", Proc. SPIE 9909, Adaptive Optics Systems V, 990958 (July 27, 2016); doi:10.1117/12.2231905; http://dx.doi.org/10.1117/12.2231905


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