Papers › CANDELS Visual Classifications: Scheme, Data Release, and First Results
CANDELS Visual Classifications: Scheme, Data Release, and First Results
Jeyhan S. Kartaltepe, Mark Mozena, Dale Kocevski, Daniel H. McIntosh, Jennifer Lotz, Eric F. Bell, Sandra Faber, Henry Ferguson, David Koo, Robert Bassett, Maksym Bernyk, Kirsten Blancato, Frederic Bournaud, Paolo Cassata, Marco Castellano, Edmond Cheung, Christopher J. Conselice, Darren Croton, Tomas Dahlen, Duilia F. de Mello, Laura DeGroot, Jennifer Donley, Javiera Guedes, Norman Grogin, Nimish Hathi, Matt Hilton, Brett Hollon, Hanae Inami, Susan Kassin, Anton Koekemoer, Caterina Lani, Nick Liu, Ray A. Lucas, Marie Martig, Elizabeth McGrath, Conor McPartland, Bahram Mobasher, Alice Morlock, Simon Mutch, Erin O'Leary, Mike Peth, Janine Pforr, Annalisa Pillepich, Gregory B. Poole, Zachary Rizer, David Rosario, Emmaris Soto, Amber Straughn, Olivia Telford, Ben Sunnquist, Benjamin Weiner, Stijn Wuyts
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We have undertaken an ambitious program to visually classify all galaxies in the five CANDELS fields down to H<24.5 involving the dedicated efforts of 65 individual classifiers. Once completed, we expect to have detailed morphological classifications for over 50,000 galaxies up to z<4 over all the fields. Here, we present our detailed visual classification scheme, which was designed to cover a wide range of CANDELS science goals. This scheme includes the basic Hubble sequence types, but also includes a detailed look at mergers and interactions, the clumpiness of galaxies, k-corrections, and a variety of other structural properties. In this paper, we focus on the first field to be completed -- GOODS-S. The wide area coverage spanning the full field includes 7634 galaxies that have been classified by at least three different people. In the deep area of the field, 2534 galaxies have been classified by at least five different people at three different depths. With this paper, we release to the public all of the visual classifications in GOODS-S along with the GUI that we developed to classify galaxies. We find that the level of agreement among classifiers is good and depends on both the galaxy magnitude and the galaxy type, with disks showing the highest level of agreement and irregulars the lowest. A comparison of our classifications with the Sersic index and rest-frame colors shows a clear separation between disk and spheroid populations. Finally, we explore morphological k-corrections between the V-band and H-band observations and find that a small fraction (84 galaxies in total) are classified as being very different between these two bands. These galaxies typically have very clumpy and extended morphology or are very faint in the V-band.
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