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Twelve years of Galaxy Zoo

Published online by Cambridge University Press:  14 May 2020

Karen L. Masters Open the ORCID record for Karen L. Masters [Opens in a new window]  and
Galaxy Zoo Team
Karen L. Masters
Affiliation:
Haverford College, Department of Physics and Astronomy, 370 Lancaster Avenue, Haverford, PA19041, USA email: klmasters@haverford.edu
Galaxy Zoo Team
Affiliation:
Haverford College, Department of Physics and Astronomy, 370 Lancaster Avenue, Haverford, PA19041, USA email: klmasters@haverford.edu
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Abstract

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The Galaxy Zoo project has provided quantitative visual morphologies for over a million galaxies, and has been part of a reinvigoration of interest in the morphologies of galaxies and what they reveal about galaxy evolution. Morphological information collected by GZ has shown itself to be a powerful tool for studying galaxy evolution, and GZ continues to collect classifications - currently serving imaging from DECaLS in its main site, and running a variety of related projects hosted by the Zooniverse; the citizen science platform which came out of the early success of GZ. I highlight some of the results from the last twelve years, with a particular emphasis on linking morphology and dynamics, look forward to future projects in the GZ family, and provide a quick start guide for how you can easily make use of citizen science techniques to analysis your own large and complex data sets.

Keywords

galaxies:fundamental parametersgalaxies:kinematics and dynamicsgalaxies: evolutiongalaxies:statisticscatalogs
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S353: Galactic Dynamics in the Era of Large Surveys , June 2019 , pp. 205 - 212
Copyright
© International Astronomical Union 2020

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