The dependence of clustering on galaxy properties
暂无分享,去创建一个
[1] J. Brinkmann,et al. New York University Value-Added Galaxy Catalog: A Galaxy Catalog Based on New Public Surveys , 2005 .
[2] J. Brinkmann,et al. NYU-VAGC: a galaxy catalog based on new public surveys , 2004, astro-ph/0410166.
[3] J. Frieman,et al. The Luminosity and Color Dependence of the Galaxy Correlation Function , 2004, astro-ph/0408569.
[4] D. Eisenstein,et al. Interpreting the Relationship between Galaxy Luminosity, Color, and Environment , 2004, astro-ph/0406633.
[5] Y. Jing,et al. The Pairwise Velocity Dispersion of Galaxies: Luminosity Dependence and a New Test of Galaxy Formation Models , 2004, astro-ph/0406077.
[6] R. Nichol,et al. The Three-Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky Survey , 2003, astro-ph/0310725.
[7] Walter A. Siegmund,et al. The Second Data Release of the Sloan Digital Sky Survey , 2004 .
[8] J. Brinkmann,et al. The environmental dependence of the relations between stellar mass, structure, star formation and nuclear activity in galaxies , 2004, astro-ph/0402030.
[9] Chisato Yamauchi,et al. The morphology–density relation in the Sloan Digital Sky Survey , 2003, astro-ph/0312043.
[10] J. Brinkmann,et al. The physical properties of star-forming galaxies in the low-redshift universe , 2003, astro-ph/0311060.
[11] R. Nichol,et al. The 3D power spectrum of galaxies from the SDSS , 2003, astro-ph/0310725.
[12] J. Brinkmann,et al. Relationship between Environment and the Broadband Optical Properties of Galaxies in the Sloan Digital Sky Survey , 2003, astro-ph/0310453.
[13] R. Nichol,et al. Quantifying the Bimodal Color-Magnitude Distribution of Galaxies , 2003, astro-ph/0309710.
[14] G. Bruzual,et al. Stellar population synthesis at the resolution of 2003 , 2003, astro-ph/0309134.
[15] R. Nichol,et al. The Environment of Active Galactic Nuclei in the Sloan Digital Sky Survey , 2003, astro-ph/0307124.
[16] A. Szalay,et al. Angular Clustering with Photometric Redshifts in the Sloan Digital Sky Survey: Bimodality in the Clustering Properties of Galaxies , 2003, astro-ph/0305603.
[17] F. M. Maley,et al. An Efficient Targeting Strategy for Multiobject Spectrograph Surveys: the Sloan Digital Sky Survey “Tiling” Algorithm , 2001, astro-ph/0105535.
[18] R. Ellis,et al. The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type , 2003, astro-ph/0303668.
[19] R. Nichol,et al. On Departures from a Power Law in the Galaxy Correlation Function , 2003, astro-ph/0301280.
[20] R. Ellis,et al. The 2dF Galaxy Redshift Survey: correlation functions, peculiar velocities and the matter density of the Universe , 2002, astro-ph/0212375.
[21] D. York,et al. The Overdensities of Galaxy Environments as a Function of Luminosity and Color , 2002, astro-ph/0212085.
[22] Ž. Ivezić,et al. Astrometric Calibration of the Sloan Digital Sky Survey , 2002, astro-ph/0211375.
[23] R. Nichol,et al. The Galaxy Luminosity Function and Luminosity Density at Redshift z = 0.1 , 2002, astro-ph/0210215.
[24] H. Mo,et al. Constraining galaxy formation and cosmology with the conditional luminosity function of galaxies , 2002, astro-ph/0207019.
[25] R. Sheth,et al. Halo Models of Large Scale Structure , 2002, astro-ph/0206508.
[26] Alexander S. Szalay,et al. Galaxy Clustering in Early Sloan Digital Sky Survey Redshift Data , 2002 .
[27] Mamoru Doi,et al. Estimating Fixed-Frame Galaxy Magnitudes in the Sloan Digital Sky Survey , 2002, astro-ph/0205243.
[28] R. Nichol,et al. The dependence of star formation history and internal structure on stellar mass for 105 low‐redshift galaxies , 2002, astro-ph/0205070.
[29] R. Nichol,et al. Stellar masses and star formation histories for 105 galaxies from the Sloan Digital Sky Survey , 2002, astro-ph/0204055.
[30] Alan Uomoto,et al. The [CLC][ITAL]u[/ITAL][/CLC][arcmin]′[CLC][ITAL]g[/ITAL][/CLC][arcmin]′[CLC][ITAL]r[/ITAL][/CLC][arcmin]′[CLC][ITAL]i[/ITAL][/CLC][arcmin]′[CLC][ITAL]z[/ITAL][/CLC][arcmin]′ Standard-Star System , 2002 .
[31] R. Ellis,et al. The 2dF Galaxy Redshift Survey: the dependence of galaxy clustering on luminosity and spectral type , 2001, astro-ph/0112043.
[32] Max Tegmark,et al. The power spectrum of galaxies in the 2dF 100k redshift survey , 2001, Monthly Notices of the Royal Astronomical Society.
[33] D. Weinberg,et al. The Halo Occupation Distribution: Toward an Empirical Determination of the Relation between Galaxies and Mass , 2001, astro-ph/0109001.
[34] V. Narayanan,et al. Color Separation of Galaxy Types in the Sloan Digital Sky Survey Imaging Data , 2001, astro-ph/0107201.
[35] J. Gunn,et al. A Photometricity and Extinction Monitor at the Apache Point Observatory , 2001, astro-ph/0106511.
[36] et al,et al. Galaxy Clustering in Early SDSS Redshift Data , 2001, astro-ph/0106476.
[37] F. M. Maley,et al. An Efficient Algorithm for Positioning Tiles in the Sloan Digital Sky Survey , 2001, astro-ph/0105535.
[38] D. Madgwick,et al. The 2dF Galaxy Redshift Survey: luminosity dependence of galaxy clustering , 2001, astro-ph/0105500.
[39] Max Tegmark,et al. The real-space power spectrum of the PSCz survey from 0.01 to 300 h Mpc−1 , 2000, astro-ph/0008392.
[40] Walter A. Siegmund,et al. The Sloan Digital Sky Survey: Technical Summary , 2000, astro-ph/0006396.
[41] J. Peacock,et al. Halo occupation numbers and galaxy bias , 2000, astro-ph/0005010.
[42] U. Seljak. Analytic model for galaxy and dark matter clustering , 2000, astro-ph/0001493.
[43] C. Baugh,et al. The dependence of velocity and clustering statistics on galaxy properties , 1999, astro-ph/9910488.
[44] Hia,et al. Differential Galaxy Evolution in Cluster and Field Galaxies at z ≈ 0.3 , 1999, astro-ph/9906470.
[45] Denmark,et al. The nature of galaxy bias and clustering , 1999, astro-ph/9903343.
[46] Walter A. Siegmund,et al. The Sloan Digital Sky Survey Photometric Camera , 1998, astro-ph/9809085.
[47] D. Schlegel,et al. Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .
[48] G. Kauffmann,et al. Clustering of galaxies in a hierarchical universe - I. Methods and results at z=0 , 1998, astro-ph/9805283.
[49] A. Szalay,et al. Can Baryonic Features Produce the Observed 100 [CLC][ITAL]h[/ITAL][/CLC][TSUP]−1[/TSUP] M[CLC]pc[/CLC] Clustering? , 1998 .
[50] J. Holtzman,et al. Cold dark matter variant cosmological models — I. Simulations and preliminary comparisons , 1997, astro-ph/9712142.
[51] D. Schlegel,et al. Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds , 1997, astro-ph/9710327.
[52] H. M. P. Couchman,et al. Evolution of Structure in Cold Dark Matter Universes , 1997, astro-ph/9709010.
[53] D. Ottaviani,et al. Hγ and Hδ Absorption Features in Stars and Stellar Populations , 1997 .
[54] Y. Jing,et al. Spatial Correlation Function and Pairwise Velocity Dispersion of Galaxies: Cold Dark Matter Models versus the Las Campanas Survey , 1997, astro-ph/9707106.
[55] M. Fukugita,et al. The Sloan Digital Sky Survey Photometric System , 1996 .
[56] G. Kauffmann,et al. Galaxy formation and large scale bias , 1995, astro-ph/9512009.
[57] A. Hamilton. Toward Better Ways to Measure the Galaxy Correlation Function , 1993 .
[58] Y. Jing,et al. On the error estimates of correlation functions , 1992 .
[59] A. Kashlinsky,et al. Large-scale structure in the Universe , 1991, Nature.
[60] J. Barrow,et al. A bootstrap resampling analysis of galaxy clustering , 1984 .
[61] P. Peebles,et al. The Large-Scale Structure of the Universe , 1980 .
[62] A. Dressler. Galaxy morphology in rich clusters: Implications for the formation and evolution of galaxies , 1980 .
[63] P. Schechter. An analytic expression for the luminosity function for galaxies , 1976 .
[64] Marc Davis,et al. Galaxy Correlations as a Function of Morphological Type , 1975 .
[65] Jr. Oemler Augustus. The Systematic Properties of Clusters of Galaxies. Photometry of 15 Clusters , 1974 .
[66] John E. Davis,et al. Sloan Digital Sky Survey: Early Data Release , 2002 .