Machine learning cosmological structure formation
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Michelle Lochner | Andrew Pontzen | Luisa Lucie-Smith | H. Peiris | M. Lochner | A. Pontzen | Luisa Lucie-Smith | Hiranya V Peiris
[1] R. Sheth,et al. Peaks theory and the excursion set approach , 2012, 1206.3506.
[2] Alan L. Yuille,et al. Performance comparison of machine learning algorithms and number of independent components used in fMRI decoding of belief vs. disbelief , 2011, NeuroImage.
[3] C. A. Oxborrow,et al. Planck2015 results , 2015, Astronomy & Astrophysics.
[4] J. Hilden. The Area under the ROC Curve and Its Competitors , 1991, Medical decision making : an international journal of the Society for Medical Decision Making.
[5] H. M. P. Couchman,et al. The mass function of dark matter haloes , 2000, astro-ph/0005260.
[6] G. Lake,et al. Evolution of the mass function of dark matter haloes , 2003, astro-ph/0301270.
[7] G. Chapman,et al. [Medical decision making]. , 1976, Lakartidningen.
[8] Robert J. Brunner,et al. Machine Learning and Cosmological Simulations I: Semi-Analytical Models , 2015, 1510.06402.
[9] O. Lahav,et al. PHOTOMETRIC SUPERNOVA CLASSIFICATION WITH MACHINE LEARNING , 2016, 1603.00882.
[10] Marc Toussaint,et al. Probabilistic inference for solving discrete and continuous state Markov Decision Processes , 2006, ICML.
[11] A. Farahi,et al. Excursion set theory for correlated random walks , 2013, 1303.0337.
[12] Rich Caruana,et al. Predicting good probabilities with supervised learning , 2005, ICML.
[13] A. Knebe,et al. Ahf: AMIGA'S HALO FINDER , 2009, 0904.3662.
[14] Ravi K. Sheth Giuseppe Tormen. Large scale bias and the peak background split , 1999 .
[15] A. Ludlow,et al. The formation of cold dark matter haloes – II. Collapse time and tides , 2014, 1405.7367.
[16] A. Szalay,et al. The statistics of peaks of Gaussian random fields , 1986 .
[17] R. Sheth,et al. Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes , 1999, astro-ph/9907024.
[18] Leo Breiman,et al. Random Forests , 2001, Machine Learning.
[19] V. Springel,et al. GADGET: a code for collisionless and gasdynamical cosmological simulations , 2000, astro-ph/0003162.
[20] J. Bond,et al. The Peak-Patch Picture of Cosmic Catalogs. I. Algorithms , 1996 .
[21] D. M. Green,et al. Signal detection theory and psychophysics , 1966 .
[22] William H. Press,et al. Formation of Galaxies and Clusters of Galaxies by Self-Similar Gravitational Condensation , 1974 .
[23] Ian H. Witten,et al. Data mining: practical machine learning tools and techniques, 3rd Edition , 1999 .
[24] Tom Fawcett,et al. An introduction to ROC analysis , 2006, Pattern Recognit. Lett..
[25] Canada.,et al. Data Mining and Machine Learning in Astronomy , 2009, 0906.2173.
[26] Rich Caruana,et al. An empirical comparison of supervised learning algorithms , 2006, ICML.
[27] Risa H. Wechsler,et al. Modeling the Impact of Baryons on Subhalo Populations with Machine Learning , 2017, The Astrophysical Journal.
[28] Bruce A. Bassett,et al. Painting galaxies into dark matter haloes using machine learning , 2017, 1712.03255.
[29] M. Halpern,et al. FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: LIKELIHOODS AND PARAMETERS FROM THE WMAP DATA , 2008, 0803.0586.
[30] Gaël Varoquaux,et al. Scikit-learn: Machine Learning in Python , 2011, J. Mach. Learn. Res..
[31] Michael S. Warren,et al. Toward a Halo Mass Function for Precision Cosmology: The Limits of Universality , 2008, 0803.2706.
[32] M. Maggiore,et al. THE HALO MASS FUNCTION FROM EXCURSION SET THEORY. I. GAUSSIAN FLUCTUATIONS WITH NON-MARKOVIAN DEPENDENCE ON THE SMOOTHING SCALE , 2009, 0903.1249.
[33] Mark Vogelsberger,et al. Numerical simulations of the dark universe: State of the art and the next decade , 2012, 1209.5745.
[34] Stuart P. D. Gill,et al. The evolution of substructure - I. A new identification method , 2004, astro-ph/0404258.
[35] V. Springel. The Cosmological simulation code GADGET-2 , 2005, astro-ph/0505010.
[36] J. R. Bond,et al. Excursion set mass functions for hierarchical Gaussian fluctuations , 1991 .