Exoplanet imaging data challenge: benchmarking the various image processing methods for exoplanet detection
- Creators
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Cantalloube, F.
- Gomez-Gonzalez, C.
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Absil, O.
- Cantero, C.
- Bacher, R.
- Bonse, J. M.
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Bottom, M.
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Dahlqvist, C.-H.
- Desgrange, C.
- Flasseur, O.
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Fuhrmann, T.
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Henning, Th.
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Jensen-Clem, R.
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Kenworthy, M.
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Mawet, D.
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Mesa, D.
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Meshkat, T.
- Mouillet, D.
- Müller, A.
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Nasedkin, E.
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Pairet, B.
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Piérard, S.
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Ruffio, J.-B.
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Samland, M.
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Stone, J.
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Van Droogenbroeck, M.
Abstract
The Exoplanet Imaging Data Challenge is a community-wide effort meant to offer a platform for a fair and common comparison of image processing methods designed for exoplanet direct detection. For this purpose, it gathers on a dedicated repository (Zenodo), data from several high-contrast ground-based instruments worldwide in which we injected synthetic planetary signals. The data challenge is hosted on the CodaLab competition platform, where participants can upload their results. The specifications of the data challenge are published on our website https://exoplanet-imaging-challenge.github.io/. The first phase, launched on the 1st of September 2019 and closed on the 1st of October 2020, consisted in detecting point sources in two types of common data-set in the field of high-contrast imaging: data taken in pupil-tracking mode at one wavelength (subchallenge 1, also referred to as ADI) and multispectral data taken in pupil-tracking mode (subchallenge 2, also referred to as ADI+mSDI). In this paper, we describe the approach, organisational lessons-learnt and current limitations of the data challenge, as well as preliminary results of the participants' submissions for this first phase. In the future, we plan to provide permanent access to the standard library of data sets and metrics, in order to guide the validation and support the publications of innovative image processing algorithms dedicated to high-contrast imaging of planetary systems.
Additional Information
© 2020 Society of Photo-Optical Instrumentation Engineers (SPIE). The EIDC collaboration would like to thank the GPIES collaboration and the SHINE collaboration, for providing us the pre-reduced data from Gemini/GPI and VLT/SPHERE respectively. This research has benefited from the SpeX Prism Spectral Libraries, maintained by Adam Burgasser at http://pono.ucsd.edu/~adam/browndwarfs/spexprism. This work was supported by the Fonds de la Recherche Scientifique-FNRS under Grant n F.4504.18 and by the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (grant agreement n 819155). T.H. acknowledges support from the European Research Council under the Horizon 2020 Framework Program via the ERC Advanced Grant Origins 832428.Attached Files
Published - 114485A.pdf
Published - SPIE-AS20-ec33ebe5-faa3-ea11-8143-005056be4d05.pdf
Accepted Version - 2101.05080.pdf
Files
Additional details
- Eprint ID
- 107384
- Resolver ID
- CaltechAUTHORS:20210108-143245499
- Fonds de la Recherche Scientifique (FNRS)
- F.4504.18
- European Research Council (ERC)
- 819155
- European Research Council (ERC)
- 832428
- Created
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2021-01-09Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field
- Caltech groups
- Astronomy Department
- Series Name
- Proceedings of SPIE
- Series Volume or Issue Number
- 11448