Galaxy Zoo: the dependence of morphology and colour on environment by Bamford, S, Nichol, R, Baldry, I, Land, K, Lintott, C, Schawinski, K, Slosar, A, Szalay, A, Thomas, D, Torki, M, Andreescu, D, Edmondson, E, Miller, C, Murray, P, Raddick, M, Vandenberg, J

“…We analyse the relationships between galaxy morphology, colour, environment and stellar mass using data for over 100,000 objects from Galaxy Zoo, the largest sample of visually classified morphologies yet compiled. …”

Galaxy Zoo: the dependence of morphology and colour on environment by Bamford, S, Nichol, R, Baldry, I, Land, K, Lintott, C, Schawinski, K, Slosar, A, Szalay, A, Thomas, D, Torki, M, Andreescu, D, Edmondson, E, Miller, C, Murray, P, Raddick, M, Vandenberg, J

“…We analyse the relationships between galaxy morphology, colour, environment and stellar mass using data for over 10 5 objects from Galaxy Zoo, the largest sample of visually classified morphologies yet compiled. …”

Galaxy Zoo: Chiral correlation function of galaxy spins by Slosar, A, Land, K, Bamford, S, Lintott, C, Andreescu, D, Murray, P, Nichol, R, Raddick, M, Schawinski, K, Szalay, A, Thomas, D, Vandenberg, J

“…Galaxy Zoo is the first study of nearby galaxies that contains reliable information about the spiral sense of rotation of galaxy arms for a sizeable number of galaxies. …”

Galaxy Zoo : 'Hanny's Voorwerp', a quasar light echo? by Lintott, C, Schawinski, K, Keel, W, Arkel, H, Bennert, N, Edmondson, E, Thomas, D, Smith, D, Herbert, P, Jarvis, M, Virani, S, Andreescu, D, Bamford, S, Land, K, Murray, P, Nichol, R, Raddick, J, Slosar, A, Szalay, A, Vandenberg, J

“…We report the discovery of an unusual object near the spiral galaxy IC 2497, discovered by visual inspection of the Sloan Digital Sky Survey (SDSS) as part of the Galaxy Zoo project. The object, known as Hanny's Voorwerp, is bright in the SDSS g band due to unusually strong OIII 4959-5007 emission lines. …”

Galaxy Zoo: A sample of blue early-type galaxies at low redshift by Schawinski, K, Lintott, C, Thomas, D, Sarzi, M, Andreescu, D, Bamford, S, Kaviraj, S, Khochfar, S, Land, K, Murray, P, Nichol, R, Raddick, M, Slosar, A, Szalay, A, VandenBerg, J, Yi, S

“…They are identified by their visual morphology as provided by Galaxy Zoo for SDSS DR6 and their u-r colour. We select a volume-limited sample in the redshift range 0.02 < z < 0.05, corresponding to luminosities of approximately L* and above, and with u-r colours significantly bluer than the red sequence. …”

Galaxy Zoo 1 : Data Release of Morphological Classifications for nearly 900,000 galaxies by Lintott, C, Schawinski, K, Bamford, S, Slosar, A, Land, K, Thomas, D, Edmondson, E, Masters, K, Nichol, R, Raddick, J, Szalay, A, Andreescu, D, Murray, P, Vandenberg, J

“…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. …”

Galaxy Zoo: A correlation between coherence of galaxy spin chirality and star formation efficiency by Jimenez, R, Slosar, A, Verde, L, Bamford, S, Lintott, C, Schawinski, K, Nichol, R, Andreescu, D, Land, K, Murray, P, Raddick, M, Szalay, A, Thomas, D, Vandenberg, J

“…This is obtained by cross-correlating star formation histories, derived with MOPED, and spin direction (chirality), as determined by the Galaxy Zoo project, for a sample of SDSS galaxies. Our findings suggest that spiral galaxies which formed the majority of their stars early (z > 2) tend to display coherent rotation over scales of ~10 Mpc/h. …”

Galaxy Zoo: The large-scale spin statistics of spiral galaxies in the Sloan Digital Sky Survey by Land, K, Slosar, A, Lintott, C, Andreescu, D, Bamford, S, Murray, P, Nichol, R, Raddick, M, Schawinski, K, Szalay, A, Thomas, D, Vandenberg, J

“…We have a sample of $\sim 37,000$ spiral galaxies from the Sloan Digital Sky Survey, with their line of sight spin direction confidently classified by members of the public through the online project Galaxy Zoo. After establishing and correcting for a certain level of bias in our handedness results we find the winding sense of the galaxies to be consistent with statistical isotropy. …”

Galaxy Zoo: morphologies derived from visual inspection of galaxies from the Sloan Digital Sky Survey by Lintott, C, Schawinski, K, Slosar, A, Land, K, Bamford, S, Thomas, D, Raddick, M, Nichol, R, Szalay, A, Andreescu, D, Murray, P, Vandenberg, J

“…This paper introduces a project, Galaxy Zoo, which provides visual morphological classifications for nearly one million galaxies, extracted from the Sloan Digital Sky Survey (SDSS). …”

Galaxy Zoo : Morphologies derived from visual inspection of galaxies from the Sloan Digital Sky Survey by Lintott, C, Schawinski, K, Slosar, A, Land, K, Bamford, S, Thomas, D, Raddick, M, Nichol, R, Szalay, A, Andreescu, D, Murray, P, Berg, J

“…This paper introduces a project, Galaxy Zoo, which provides visual morphological classifications for nearly one million galaxies, extracted from the Sloan Digital Sky Survey (SDSS). …”