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

Published online by Cambridge University Press:  06 January 2014

Janis Hagelberg ,
Damien Ségransan ,
Stéphane Udry  and
François Wildi
Janis Hagelberg
Affiliation:
Observatoire de Genève, University of Geneva, 51 Chemin des Maillettes, 1290, Versoix, Switzerland email: janis.hagelberg@unige.ch
Damien Ségransan
Affiliation:
Observatoire de Genève, University of Geneva, 51 Chemin des Maillettes, 1290, Versoix, Switzerland email: janis.hagelberg@unige.ch
Stéphane Udry
Affiliation:
Observatoire de Genève, University of Geneva, 51 Chemin des Maillettes, 1290, Versoix, Switzerland email: janis.hagelberg@unige.ch
François Wildi
Affiliation:
Observatoire de Genève, University of Geneva, 51 Chemin des Maillettes, 1290, Versoix, Switzerland email: janis.hagelberg@unige.ch
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Abstract

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We present a new analysis and reduction pipeline for the detection of planetary companions using Angular Differential Imaging. The pipeline uses Fourier transforms for image shifting and rotation in order to achieve very low signal loss. Furthermore it is parallelised in order to run on computer clusters of up to 1024 cores. The pipeline was developed in Geneva for the ongoing direct imaging campaign for stars with radial velocity drifts in the HARPS and CORALIE radial-velocity planet-search surveys. In addition to that, a disk mode has been implemented in the context of observations of the protoplanetary disk around HD142527.

Keywords

instrumentation: adaptive opticstechniques: high angular resolutiontechniques: image processingmethods: data analysisplanetary systemsstars: low-massbrown dwarfs
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S299: Exploring the Formation and Evolution of Planetary Systems , June 2013 , pp. 38 - 39
Copyright
Copyright © International Astronomical Union 2013 

References

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