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Galaxy Zoo DECaLS: Detailed visual morphology measurements from volunteers and deep learning for 314,000 galaxies

Journal Article · · Monthly Notices of the Royal Astronomical Society
 [1];  [1];  [1];  [2];  [3];  [4];  [5];  [6];  [4];  [1];  [7];  [8];  [7];  [9];  [1];  [1];  [1];  [1]
  1. Univ. of Oxford (United Kingdom)
  2. European Space Agency, Noordwijk (Netherlands)
  3. Univ. of Portsmouth (United Kingdom)
  4. Univ. of Minnesota, Minneapolis, MN (United States)
  5. Univ. of Nottingham (United Kingdom)
  6. Princeton Univ., NJ (United States)
  7. Univ. of Alabama, Tuscaloosa, AL (United States)
  8. Haverford College, PA (United States)
  9. Lancaster Univ. (United Kingdom)
We present Galaxy Zoo DECaLS: detailed visual morphological classifications for Dark Energy Camera Legacy Survey images of galaxies within the SDSS DR8 footprint. Deeper DECaLS images (r = 23.6 versus r = 22.2 from SDSS) reveal spiral arms, weak bars, and tidal features not previously visible in SDSS imaging. To best exploit the greater depth of DECaLS images, volunteers select from a new set of answers designed to improve our sensitivity to mergers and bars. Galaxy Zoo volunteers provide 7.5 million individual classifications over 314 000 galaxies. 140 000 galaxies receive at least 30 classifications, sufficient to accurately measure detailed morphology like bars, and the remainder receive approximately 5. All classifications are used to train an ensemble of Bayesian convolutional neural networks (a state-of-the-art deep learning method) to predict posteriors for the detailed morphology of all 314 000 galaxies. We use active learning to focus our volunteer effort on the galaxies which, if labelled, would be most informative for training our ensemble. When measured against confident volunteer classifications, the trained networks are approximately 99 per cent accurate on every question. Morphology is a fundamental feature of every galaxy; our human and machine classifications are an accurate and detailed resource for understanding how galaxies evolve.
Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
Sponsoring Organization:
USDOE
Contributing Organization:
Galaxy Zoo; Sloan Digital Sky Survey (SDSS)
Grant/Contract Number:
AC02-05CH11231
OSTI ID:
1982517
Journal Information:
Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 3 Vol. 509; ISSN 0035-8711
Publisher:
Oxford University PressCopyright Statement
Country of Publication:
United States
Language:
English

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