Abstract
Morphology is a powerful indicator of a galaxy’s dynamical and merger history. It is strongly correlated with many physical parameters, including mass, star formation history and the distribution of mass. The Galaxy Zoo project collected simple morphological classifications of nearly 900 000 galaxies drawn from the Sloan Digital Sky Survey, contributed by hundreds of thousands of volunteers. This large number of classifications allows us to exclude classifier error, and measure the influence of subtle biases inherent in morphological classification. This paper presents the data collected by the project, alongside measures of classification accuracy and bias
| Original language | English |
|---|---|
| Pages (from-to) | 166-178 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 410 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 1 Jan 2011 |
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