Comparison of density estimation methods for astronomical datasets
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Michael H. F. Wilkinson | Jos B. T. M. Roerdink | Scott Trager | Bilkis Jamal Ferdosi | H. Buddelmeijer | J. Roerdink | S. Trager | H. Buddelmeijer | M. Wilkinson | B. J. Ferdosi
[1] The Bimodal Galaxy Color Distribution: Dependence on Luminosity and Environment , 2004, astro-ph/0406266.
[2] V. A. Epanechnikov. Non-Parametric Estimation of a Multivariate Probability Density , 1969 .
[3] V. Springel,et al. Phase‐space structures – II. Hierarchical Structure Finder , 2008, 0812.0288.
[4] J. Peacock,et al. Simulations of the formation, evolution and clustering of galaxies and quasars , 2005, Nature.
[5] C. Loader. Bandwidth selection: classical or plug-in? , 1999 .
[6] G. Lucia,et al. The hierarchical formation of the brightest cluster galaxies , 2006, astro-ph/0606519.
[7] E. Parzen. On Estimation of a Probability Density Function and Mode , 1962 .
[8] Enn Saar,et al. Statistics of the Galaxy Distribution , 2001 .
[9] B. Jones,et al. A lognormal model for the cosmological mass distribution. , 1991 .
[10] S. Driver,et al. The Millennium Galaxy Catalogue : morphological classification and bimodality in the colour-concentration plane , 2006, astro-ph/0602240.
[11] B. Silverman. Density estimation for statistics and data analysis , 1986 .
[12] A. Dressler. Galaxy morphology in rich clusters: Implications for the formation and evolution of galaxies , 1980 .
[13] M H Wilkinson,et al. DATAPLOT: a graphical display package for bacterial morphometry and fluorimetry data. , 1995, Computer methods and programs in biomedicine.
[14] Galaxy colour, morphology and environment in the Sloan Digital Sky Survey , 2006, astro-ph/0610171.
[15] M. Raddick,et al. The Fifth Data Release of the Sloan Digital Sky Survey , 2007, 0707.3380.
[16] I. Csiszár. Why least squares and maximum entropy? An axiomatic approach to inference for linear inverse problems , 1991 .
[17] D. Fabricant,et al. The color-magnitude relation in CL 1358+62 at z=0.33: Evidence for significant evolution in the S0 population , 1998, astro-ph/9801190.
[18] V. Narayanan,et al. Color Separation of Galaxy Types in the Sloan Digital Sky Survey Imaging Data , 2001, astro-ph/0107201.
[19] Donald Ervin Knuth,et al. The Art of Computer Programming, Volume II: Seminumerical Algorithms , 1970 .
[20] J. Monaghan,et al. Smoothed particle hydrodynamics: Theory and application to non-spherical stars , 1977 .
[21] P. Schechter. An analytic expression for the luminosity function for galaxies , 1976 .
[22] Stéphane Colombi,et al. The fully connected N-dimensional skeleton: probing the evolution of the cosmic web , 2008, ArXiv.
[23] K. Abazajian,et al. THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY , 2008, 0812.0649.
[24] S. Roweis,et al. K-Corrections and Filter Transformations in the Ultraviolet, Optical, and Near-Infrared , 2006, astro-ph/0606170.
[25] E. Hubble,et al. No. 427. The velocity-distance relation among extra-galactic nebulae. , 1931 .
[26] Amina Helmi,et al. Mapping the substructure in the Galactic halo with the next generation of astrometric satellites , 2000, astro-ph/0007166.
[27] R. van de Weygaert,et al. Density estimators in particle hydrodynamics DTFE versus regular SPH , 2003, astro-ph/0303071.
[28] Xinfa Deng,et al. THE DEPENDENCE OF LUMINOSITY AND g − r COLOR ON THE ENVIRONMENT FOR THE SAME MORPHOLOGICAL TYPES , 2009 .
[29] S. Bamford,et al. Galaxy bimodality versus stellar mass and environment , 2006, astro-ph/0607648.
[30] D. Steinberg,et al. Technometrics , 2008 .
[31] Baltimore.,et al. Multiscale phenomenology of the cosmic web , 2010, 1007.0742.
[32] James Stephen Marron,et al. Comparison of data-driven bandwith selectors , 1988 .
[33] R. Weygaert,et al. Delaunay Tessellation Field Estimator analysis of the PSCz local Universe: density field and cosmic flow , 2007 .
[34] Zeljko Ivezic,et al. The Environment of Galaxies at Low Redshift , 2008, 0801.0312.
[35] L. Lucy. A numerical approach to the testing of the fission hypothesis. , 1977 .
[36] F. Kitaura,et al. Bayesian power-spectrum inference for large-scale structure data , 2009, 0911.2493.
[37] L. Breiman,et al. Variable Kernel Estimates of Multivariate Densities , 1977 .
[38] C. D. Kemp,et al. Density Estimation for Statistics and Data Analysis , 1987 .
[39] J. Copas,et al. Interpreting Kullback-Leibler divergence with the Neyman-Pearson lemma , 2006 .
[40] Donald Ervin Knuth,et al. The Art of Computer Programming , 1968 .
[41] F. Braglia,et al. Flaming, bright galaxies along the filaments of A 2744 , 2007, 0705.0273.
[42] E. al.,et al. The Sloan Digital Sky Survey: Technical summary , 2000, astro-ph/0006396.
[43] J. E. Felten. Study of the luminosity function for field galaxies , 1977 .