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Modeling with the Crowd: Optimizing the Human-Machine Partnership with Zooniverse

Status Report From: arXiv.org e-Print archive
Posted: Wednesday, March 20, 2019

Hugh Dickinson, Lucy Fortson, Claudia Scarlata, Melanie Beck, Mike Walmsley

(Submitted on 19 Mar 2019)

LSST and Euclid must address the daunting challenge of analyzing the unprecedented volumes of imaging and spectroscopic data that these next-generation instruments will generate. A promising approach to overcoming this challenge involves rapid, automatic image processing using appropriately trained Deep Learning (DL) algorithms. However, reliable application of DL requires large, accurately labeled samples of training data. Galaxy Zoo Express (GZX) is a recent experiment that simulated using Bayesian inference to dynamically aggregate binary responses provided by citizen scientists via the Zooniverse crowd-sourcing platform in real time. The GZX approach enables collaboration between human and machine classifiers and provides rapidly generated, reliably labeled datasets, thereby enabling online training of accurate machine classifiers. We present selected results from GZX and show how the Bayesian aggregation engine it uses can be extended to efficiently provide object-localization and bounding-box annotations of two-dimensional data with quantified reliability. DL algorithms that are trained using these annotations will facilitate numerous panchromatic data modeling tasks including morphological classification and substructure detection in direct imaging, as well as decontamination and emission line identification for slitless spectroscopy. Effectively combining the speed of modern computational analyses with the human capacity to extrapolate from few examples will be critical if the potential of forthcoming large-scale surveys is to be realized.

Comments: 5 pages, 1 figure. To appear in Proceedings of the International Astronomical Union

Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM); Astrophysics of Galaxies (astro-ph.GA)

Cite as: arXiv:1903.07776 [astro-ph.IM] (or arXiv:1903.07776v1 [astro-ph.IM] for this version)

Submission history

From: Hugh Dickinson  

[v1] Tue, 19 Mar 2019 00:14:07 UTC (94 KB)

https://arxiv.org/abs/1903.07776

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