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The Geneva Reduction and Analysis Pipeline for High-contrast Imaging of planetary Companions

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arxiv 1510.04331 v2 pith:I3PTCGQM submitted 2015-10-14 astro-ph.IM astro-ph.EP

The Geneva Reduction and Analysis Pipeline for High-contrast Imaging of planetary Companions

classification astro-ph.IM astro-ph.EP
keywords pipelinecompanionsconventionaldatafourierreductiontransformsgeometric
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We present GRAPHIC, a new angular differential imaging (ADI) reduction pipeline where all geometric image operations are based on Fourier transforms. To achieve this goal the entire pipeline is parallelised making it possible to reduce large amounts of observation data without the need to bin the data. The specific rotation and shift algorithms based on Fourier transforms are described and performance comparison with conventional interpolation algorithm are given. Tests using fake companions injected in real science frames demonstrate the significant gain obtained by using geometric operations based on Fourier transforms compared to conventional interpolation. This also translates in a better point spread function and speckle subtraction with respect to conventional reduction pipelines, achieving detection limits comparable to current best performing pipelines. Flux conservation of the companions is also demonstrated. This pipeline is currently able to reduce science data produced by VLT/NACO, Gemini/NICI, VLT/SPHERE, and Subaru/SCExAO.

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