REDUCING THE DIMENSIONALITY OF DATA: LOCALLY LINEAR EMBEDDING OF SLOAN GALAXY SPECTRA
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[1] G. Vaucouleurs. Classification and Morphology of External Galaxies , 1959 .
[2] A. Naim,et al. Neural computation as a tool for galaxy classification: methods and examples , 1995, astro-ph/9508012.
[3] B. Skiff,et al. VizieR Online Data Catalog , 2009 .
[4] M. Skrutskie,et al. The Two Micron All Sky Survey (2MASS) , 2006 .
[5] I. Jolliffe. Principal Component Analysis , 2002 .
[6] University of Toronto,et al. A New Approach to Galaxy Morphology. I. Analysis of the Sloan Digital Sky Survey Early Data Release , 2003, astro-ph/0301239.
[7] Harinder P. Singh,et al. Stellar spectral classification using principal component analysis and artificial neural networks , 1998 .
[8] Sabine Van Huffel,et al. Total least squares problem - computational aspects and analysis , 1991, Frontiers in applied mathematics.
[9] A. Szalay,et al. Reliable eigenspectra for new generation surveys , 2008, 0809.0881.
[10] William H. Press,et al. Spectral Classification and Luminosity Function of Galaxies in the Las Campanas Redshift Survey , 1997, astro-ph/9711227.
[11] Trevor Hastie,et al. The Elements of Statistical Learning , 2001 .
[12] Alexei V. Filippenko,et al. A Search for “Dwarf'' Seyfert Nuclei. III. Spectroscopic Parameters and Properties of the Host Galaxies , 1997, astro-ph/9704107.
[13] Christian Reichardt,et al. Recovering physical parameters from galaxy spectra using MOPED , 2001, astro-ph/0101074.
[14] Global regularities in integrated galaxy spectra , 1996, astro-ph/9612161.
[15] R. Nichol,et al. Distributions of Galaxy Spectral Types in the Sloan Digital Sky Survey , 2004, astro-ph/0407061.
[16] Puragra Guhathakurta,et al. The DEEP2 Galaxy Redshift Survey: Spectral Classification of Galaxies at z ∼ 1 , 2003, astro-ph/0305587.
[17] D. Donoho,et al. Hessian eigenmaps: Locally linear embedding techniques for high-dimensional data , 2003, Proceedings of the National Academy of Sciences of the United States of America.
[18] D. Osterbrock,et al. OPTICAL SPECTRA OF IRAS "WARM" GALAXIES. , 1985 .
[19] S. Bergh. A new classification system for galaxies. , 1976 .
[20] O. Lahav,et al. Massive lossless data compression and multiple parameter estimation from galaxy spectra , 1999, astro-ph/9911102.
[21] Frederic H. Chaffee,et al. An objective classification scheme for QSO spectra , 1992 .
[22] Lloyd N. Trefethen,et al. Large-Scale Computation of Pseudospectra Using ARPACK and Eigs , 2001, SIAM J. Sci. Comput..
[23] Robert Jedicke,et al. Pan-STARRS: A Large Synoptic Survey Telescope Array , 2002, SPIE Astronomical Telescopes + Instrumentation.
[24] J. Baldwin,et al. ERRATUM - CLASSIFICATION PARAMETERS FOR THE EMISSION-LINE SPECTRA OF EXTRAGALACTIC OBJECTS , 1981 .
[25] D. Madgwick,et al. Spectroscopic Detection of Type Ia Supernovae in the Sloan Digital Sky Survey , 2003, astro-ph/0310887.
[26] Dit-Yan Yeung,et al. Robust locally linear embedding , 2006, Pattern Recognit..
[27] Francisco Valdes,et al. The Morphologies of Distant Galaxies. I. an Automated Classification System , 1994 .
[28] E. al.,et al. The Sloan Digital Sky Survey: Technical summary , 2000, astro-ph/0006396.
[29] Galaxy spectral parametrization in the 2dF Galaxy Redshift Survey as a diagnostic of star formation history , 2002, astro-ph/0210471.
[30] P. Holland,et al. Robust regression using iteratively reweighted least-squares , 1977 .
[31] K. Abazajian,et al. THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY , 2008, 0812.0649.
[32] Robert L. Kurucz,et al. A calibration of Geneva photometry for B to G stars in terms of Teff, log g and $[M/H]$ , 1997 .
[33] Multivariate analysis of elliptical galaxies , 1984 .
[34] O. Lahav,et al. Principal component analysis of synthetic galaxy spectra , 1998, astro-ph/9805130.
[35] O. Lahav,et al. An artificial neural network approach to the classification of galaxy spectra , 1996, astro-ph/9608073.
[36] A. Szalay,et al. Spectral Classification of Quasars in the Sloan Digital Sky Survey: Eigenspectra, Redshift, and Luminosity Effects , 2004, astro-ph/0408578.
[37] S T Roweis,et al. Nonlinear dimensionality reduction by locally linear embedding. , 2000, Science.
[38] A. Szalay,et al. Spectral classification of galaxies: An Orthogonal approach , 1994, astro-ph/9411044.
[39] L. Kewley,et al. Theoretical Modeling of Starburst Galaxies , 2001, astro-ph/0106324.
[40] Ted von Hippel,et al. Automated classification of stellar spectra - II. Two-dimensional classification with neural networks and principal components analysis , 1998, astro-ph/9803050.
[41] M. Fukugita,et al. The Sloan Digital Sky Survey Photometric System , 1996 .
[42] V. Narayanan,et al. Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample , 2002, astro-ph/0206225.
[43] STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE , 1998, astro-ph/9807187.
[44] T. Boroson,et al. The Emission-Line Properties of Low-Redshift Quasi-stellar Objects , 1992 .
[45] et al,et al. The Sloan Digital Sky Survey Photometric Camera , 1998, astro-ph/9809085.
[46] K. Taylor,et al. The 2dF Galaxy Redshift Survey: spectral types and luminosity functions , 1999, astro-ph/9903456.
[47] A. Pasquali,et al. A Principal Component Analysis approach to the Star Formation History of elliptical galaxies in Compact Groups , 2005, astro-ph/0511753.
[48] Hans-Peter Kriegel,et al. Fast nearest neighbor search in high-dimensional space , 1998, Proceedings 14th International Conference on Data Engineering.
[49] G. Bruzual,et al. Stellar population synthesis at the resolution of 2003 , 2003, astro-ph/0309134.
[50] Ann B. Lee,et al. EXPLOITING LOW-DIMENSIONAL STRUCTURE IN ASTRONOMICAL SPECTRA , 2008, 0807.2900.
[51] C. Pritchet. The Stellar Content of Local Group Galaxies: IAU Symposium 192 , 1998 .
[52] Amos Storkey,et al. Advances in Neural Information Processing Systems 20 , 2007 .