Now back in Technicolor!

The science team and I want to thank to everyone who’s helped participate in the last month of classifications for the single-band Sloan Digital Sky Survey images in Galaxy Zoo, which were finished last night! The data will help us answer one of our key science questions (how does morphology change as a function of observed wavelength?), helping explore the role played by dust, stellar populations of different ages, and active regions of star formation. Researchers, particularly those at the University of Portsmouth, are eager to start looking at your classifications immediately.

Not saturated enough to be Technicolor, strictly speaking.

“Look, Toto – Galaxy Zoo’s back in color!” (Image courtesy MGM/Ryan McCormick)

In the meantime, we’re returning to images that are likely more familiar to many volunteers: the SDSS gri color images from Data Release 8. These galaxies still need more data, especially for the disk/featured galaxies and detailed structures. However, we should have two new sets of data ready for classification very soon alongside the SDSS, including a brand-new telescope and something a little different than before.

Please let us know on Talk if you have any questions, particularly if you have feedback about the single-band images or the science we’re working on. Thanks again!!

About Kyle Willett

Kyle Willett is a postdoc and astronomer at the University of Minnesota. He works as a member of the Galaxy Zoo team, and gets to study galaxy morphology and evolution, AGN, blazars, megamasers, citizen science engagement, and many other cool things.

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