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[1] George Cybenko,et al. Approximation by superpositions of a sigmoidal function , 1992, Math. Control. Signals Syst..
[2] A. Szalay,et al. Galaxy Luminosity Functions to z~1 from DEEP2 and COMBO-17: Implications for Red Galaxy Formation , 2005, astro-ph/0506044.
[3] E. Suchman,et al. The American soldier: Adjustment during army life. (Studies in social psychology in World War II), Vol. 1 , 1949 .
[4] Geoffrey E. Hinton,et al. Deep Learning , 2015, Nature.
[5] C. Lintott,et al. Galaxy Zoo 1: data release of morphological classifications for nearly 900 000 galaxies , 2010, 1007.3265.
[6] Ronald J. Buta,et al. The Catalog of Southern Ringed Galaxies , 1994 .
[7] E. Bell,et al. The Optical and Near-Infrared Properties of Galaxies. I. Luminosity and Stellar Mass Functions , 2003, astro-ph/0302543.
[8] G. Neugebauer,et al. Ultraluminous infrared galaxies and the origin of quasars , 1988 .
[9] H. D. Brunk,et al. Statistical inference under order restrictions : the theory and application of isotonic regression , 1973 .
[10] C. Lintott,et al. Galaxy Zoo: morphologies derived from visual inspection of galaxies from the Sloan Digital Sky Survey , 2008, 0804.4483.
[11] L. Hernquist,et al. Gasdynamics and starbursts in major mergers , 1995, astro-ph/9512099.
[12] Carnegie-Mellon,et al. A Unified, Merger-driven Model of the Origin of Starbursts, Quasars, the Cosmic X-Ray Background, Supermassive Black Holes, and Galaxy Spheroids , 2005, astro-ph/0506398.
[13] François Chollet,et al. Xception: Deep Learning with Depthwise Separable Convolutions , 2016, 2017 IEEE Conference on Computer Vision and Pattern Recognition (CVPR).
[14] E. Treister,et al. MAJOR GALAXY MERGERS ONLY TRIGGER THE MOST LUMINOUS ACTIVE GALACTIC NUCLEI , 2012, 1209.5393.
[15] Christopher J. Conselice,et al. The Relationship between Stellar Light Distributions of Galaxies and Their Formation Histories , 2003 .
[16] Stuart Lynn,et al. The Galaxy Zoo survey for giant AGN-ionized clouds: past and present black hole accretion events , 2011, 1110.6921.
[17] Richard S. Ellis,et al. Analysis of a complete galaxy redshift survey – II. The field-galaxy luminosity function , 1988 .
[18] A. S. Szalay,et al. Galaxy Zoo: the fraction of merging galaxies in the SDSS and their morphologies , 2009, 0903.4937.
[19] F. Attneave,et al. The Organization of Behavior: A Neuropsychological Theory , 1949 .
[20] Geoffrey E. Hinton,et al. ImageNet classification with deep convolutional neural networks , 2012, Commun. ACM.
[21] Yoshua Bengio,et al. Gradient-based learning applied to document recognition , 1998, Proc. IEEE.
[22] T. D. Matteo,et al. Modelling feedback from stars and black holes in galaxy mergers , 2004, astro-ph/0411108.
[23] Ben Hoyle,et al. Measuring photometric redshifts using galaxy images and Deep Neural Networks , 2015, Astron. Comput..
[24] Tom Fawcett,et al. An introduction to ROC analysis , 2006, Pattern Recognit. Lett..
[25] Antonio Torralba,et al. Comparison of deep neural networks to spatio-temporal cortical dynamics of human visual object recognition reveals hierarchical correspondence , 2016, Scientific Reports.
[26] Sander Dieleman,et al. Rotation-invariant convolutional neural networks for galaxy morphology prediction , 2015, ArXiv.
[27] Puragra Guhathakurta,et al. The DEEP2 Galaxy Redshift Survey: Evolution of Close Galaxy Pairs and Major-Merger Rates up to z ~ 1.2 , 2004, astro-ph/0411104.
[28] A. Toomre,et al. Galactic Bridges and Tails , 1972 .
[29] M. Geller,et al. Minor Galaxy Interactions: Star Formation Rates and Galaxy Properties , 2007, astro-ph/0703729.
[30] Sugata Kaviraj,et al. Galaxy Zoo: Major Galaxy Mergers Are Not a Significant Quenching Pathway , 2017, 1708.00866.
[31] Joel R. Primack,et al. The effect of mass ratio on the morphology and time-scales of disc galaxy mergers: Effect of mass ratio on merger morphology , 2009, 0912.1590.
[32] Welch Bl. THE GENERALIZATION OF ‘STUDENT'S’ PROBLEM WHEN SEVERAL DIFFERENT POPULATION VARLANCES ARE INVOLVED , 1947 .
[33] P. Madau,et al. A NEW NONPARAMETRIC APPROACH TO GALAXY MORPHOLOGICAL CLASSIFICATION , 2003, astro-ph/0311352.
[34] Christian Wolf,et al. A new automatic method to identify galaxy mergers – I. Description and application to the Space Telescope A901/902 Galaxy Evolution Survey★ , 2011, 1109.6828.
[35] Alessandro Caccianiga,et al. The merger fraction of active and inactive galaxies in the local Universe through an improved non-parametric classification , 2013, 1303.0036.
[36] Kurt Hornik,et al. Approximation capabilities of multilayer feedforward networks , 1991, Neural Networks.
[37] F. James. Statistical Methods in Experimental Physics , 1973 .
[38] R. Nichol,et al. Quantifying the Bimodal Color-Magnitude Distribution of Galaxies , 2003, astro-ph/0309710.
[39] David Schiminovich,et al. The Star Formation and Extinction Coevolution of UV-Selected Galaxies over 0.05 < z < 1.2 , 2007, 0709.0730.
[40] Oriol Vinyals,et al. Qualitatively characterizing neural network optimization problems , 2014, ICLR.
[41] Kunihiko Fukushima,et al. Neocognitron: A self-organizing neural network model for a mechanism of pattern recognition unaffected by shift in position , 1980, Biological Cybernetics.
[42] O. I. Wong,et al. The green valley is a red herring: Galaxy Zoo reveals two evolutionary pathways towards quenching of star formation in early-and late-type galaxies , 2014, 1402.4814.
[43] Mark Lacy,et al. SHOCKED POSTSTARBUST GALAXY SURVEY. I. CANDIDATE POST-STARBUST GALAXIES WITH EMISSION LINE RATIOS CONSISTENT WITH SHOCKS , 2016, 1601.05085.
[44] Anna K. Weigel,et al. Stellar mass functions: methods, systematics and results for the local Universe , 2016, 1604.00008.
[45] J. P. Jones,et al. An evaluation of the two-dimensional Gabor filter model of simple receptive fields in cat striate cortex. , 1987, Journal of neurophysiology.
[46] P. Natarajan,et al. Major Galaxy Mergers and the Growth of Supermassive Black Holes in Quasars , 2010, Science.
[47] S Marcelja,et al. Mathematical description of the responses of simple cortical cells. , 1980, Journal of the Optical Society of America.
[48] B. Garilli,et al. zCOSMOS – 10k-bright spectroscopic sample - The bimodality in the galaxy stellar mass function: exploring its evolution with redshift , 2009, 0907.5416.
[49] J. Daugman. Uncertainty relation for resolution in space, spatial frequency, and orientation optimized by two-dimensional visual cortical filters. , 1985, Journal of the Optical Society of America. A, Optics and image science.
[50] Daniel H. McIntosh,et al. A First Estimate of the Baryonic Mass Function of Galaxies , 2003, astro-ph/0301616.
[51] Joel R. Primack,et al. Galaxy merger morphologies and time-scales from simulations of equal-mass gas-rich disc mergers , 2008, 0805.1246.
[52] Allan Sandage,et al. The velocity field of bright nearby galaxies. I - The variation of mean absolute magnitude with redshift for galaxies in a magnitude-limited sample , 1979 .
[53] Maarten Schmidt,et al. Space Distribution and Luminosity Functions of Quasi-Stellar Radio Sources , 1968 .
[54] M. Whitlock. Combining probability from independent tests: the weighted Z‐method is superior to Fisher's approach , 2005, Journal of evolutionary biology.
[55] Nilotpal Chakravarti,et al. Isotonic Median Regression: A Linear Programming Approach , 1989, Math. Oper. Res..
[56] Edwin Simpson,et al. Space Warps – I. Crowdsourcing the discovery of gravitational lenses , 2015, 1504.06148.