A new high-contrast imaging subtraction algorithm (TLOCI) is presented to maximize a planet signal-to-noise ratio. The technique uses an input spectrum and template PSFs to optimize the reference image coefficient determination to minimize the flux contamination via self-subtraction (thus maximizing its throughput wavelength per wavelength) of any planet that have a similar spectrum to the template spectrum in the image, while trying, at the same time, to maximize the speckle noise subtraction. The optimization is performed by a correlation matrix conditioning. Using laboratory Gemini Planet Imager data, the new algorithm is shown to be superior to the simple/double difference, polynomial fit and original LOCI algorithm. Copyright © 2013, International Astronomical Union.
CITATION STYLE
Marois, C., Correia, C., Véran, J. P., & Currie, T. (2013). TLOCI: A fully loaded speckle killing machine. In Proceedings of the International Astronomical Union (Vol. 8, pp. 48–49). Cambridge University Press. https://doi.org/10.1017/S1743921313007813
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