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Exoplanet direct imaging data challenge
Presentation given at the Paris-Saclay Center for Data Science (INRIA Saclay) on the topic of data challenges for astronomical high-contrast imaging and direct detection of exoplanets.
Carlos Alberto Gomez Gonzalez
April 11, 2018
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30 slides
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Exoplanet direct imaging data challenge Carlos Alberto Gomez Gonzalez Paris-Saclay
Center for Data Science, 11/04/2018 -
Grenoble Alpes Data Institue ▪ WP1: Data Science for Earth,
Space and Environmental Sciences ▪ WP2: Data Science for Life Sciences ▪ WP3: Massive and Rich Data for Humanities ▪ WP4: Data Science, Social Media and Social Sciences ▪ WP5: Data Governance, Data Protection and Privacy WP0: Coordination MSTIC - Mathematics, Information and Communication Sciences and Technologies CBS - Chemistry, Biology, Health PAGE - Particle physics, Astrophysics, Geosciences, Environment and ecology SHS - Humanities and Social Sciences PSS - Social Sciences USMB – Univ Savoie Mont Blanc 19 Labs involved that cover 5 research domains IDEX Cross disciplinary Program • 1.7 million euros • From 2017 to 2020 -
Grenoble Alpes Data Institue • Data Challenge: • epigenetic &
High-dimension Mediation Data Challenge, • audio-visual diarization, • cancer research, • home-made framework (codalab / jupyter)? • Data Science in the Alpes (March 20) • R in Grenoble group. • PySciDataGre group. • Data club. • Data Carpentry. -
What do I do • Interdisciplinary research. • Exoplanetary science
and astrophysics with CS & ML. • Integrating cutting-edge ML developments. • Ensuring the use of robust statistical approaches and well-suited metrics. • Open-source development. • Data challenges. -
Mostly, we rely on indirect methods for detecting exoplanets …
it’s very hard to “see” them -
Milli et al. 2016 Konopacky et al. 2013 Bowler 2016
Marois et al. 2010 HR8799, L’ band 20 AU 0.5” b c d e Power of direct imaging -
Basic calibration and “cosmetics” • Dark/bias subtraction • Flat fielding
• Sky or thermal background subtraction • Bad pixel correction Raw astronomical images Detection on final residual image Image recentering Bad frames removal PSF modeling • Median • Pairwise, ANDROMEDA • LOCI • PCA, NMF • LLSG Image combination Model PSF subtraction De-rotation (ADI) or rescaling (mSDI) Characterization of detected companions Sequence of calibrated images -
calib. im ages planet Angular differential imaging - bright synthetic
planet Speckle noise ANIMATION -
HR8799 bcde (Marois et al. 2008-2010) On of the lucky
cases! Final images after post-processing (several epochs) post- proc. ANIMATION -
• Available on Pypi • https://github.com/vortex-exoplanet/VIP • Documentation (Sphynx): http://vip.readthedocs.io/
• Jupyter tutorial • Python 2/3 compatibility • Continuous integration (Travis CI) and automated testing (Pytest) Gomez Gonzalez et al. 2017 Vortex Image Processing library -
Marois et al. 2007 Gomez Gonzalez et al. 2016 Lafrenière
et al. 2007 A lgo- ZO O Marois et al. 2007 Soummer et al. 2012 Amara & Quanz 2012 Absil et al. 2013 Gomez Gonzalez et al. 2017 Gomez Gonzalez et al. 2016 Gomez Gonzalez et al. 2016 Marois et al. 2014 Marois et al. 2014 Hagelberg et al. 2015 Mugnier et al. 2009 Cantalloube et al. 2015 -
“Today, software is to scientific research what Galileo’s telescope was
to astronomy: a tool, combining science and engineering. It lies outside the central field of principal competence among the researchers that rely on it. … it builds upon scientific progress and shapes our scientific vision.” Pradal et al. 2015 -
Image sequence Detection Final residual image ? ? ? ?
? ? ? Speckles (?) Real planet Synth. planet -
“Essentially, all models are wrong, but some are useful.” George
Box “…if the model is going to be wrong anyway, why not see if you can get the computer to ‘quickly’ learn a model from the data, rather than have a human laboriously derive a model from a lot of thought.” Peter Norvig -
PC 1 PC 2 Unsupervised Supervised Regression Classification Dimensionality reduction
Clustering ML in a nutshell Density estimation and reinforcement learning -
The goal is to learn a mapping from the input
samples to the labels: given a labeled dataset : Supervised learning Goodfellow et al. 2016 -
Model PSF subtraction combined residuals Supervised detection (SODINN) noisy and
unlabelled images data transformation + adequate (ML) model higher sensitivity -
• Small committee takes care of most of the planing.
• Main organizer takes care of logistics/ leaderboard. • Main organizer writes a review-type paper. • Community effort. • Using a robust framework for data challenges creation. • Hands-on sessions. • Workshop for analyzing results and learning from different approaches. Old school Open science Data challenges -
• Low detection rate so far - observational bias or
reality? • Several instruments/surveys with large databases. • New instruments coming online in the next years. • ~13 years of image processing techniques. • Discovering new techniques! Exoplanet DI challenge Motivation -
• Benchmark datasets — Metrics — Sub-challenges. • Finding the
right platform (RAMP?). • Avoid excluding “old” code/pipelines: IDL, MATLAB, etc. Exoplanet DI challenge Planning: • benchmark datasets • sub-challenges • metrics Kick-off one-day session (RAMP?) Submission of results • Final leaderboard • Comparison of results/ approaches Workshop: image processing for exoplanet DI -
• Possible sub-challenges. • Each observing technique: different data format/dimensionality,
variability to exploit. • Detection & characterization. • Focus on exoplanets (excluding disks?). Exoplanet DI challenge ADI (NACO, SPHERE/ IRDIS, NIRC2, LMIRcam, etc) ADI + mSDI (SPHERE/IFS, GPI, etc) RDI, other techniques?