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Inclination-Dependent Luminosity Function of Spiral Galaxies in the Sloan Digital Sky Survey: Implication for Dust Extinction
Zhengyi Shao, Quanbao Xiao, Shiyin Shen +3
Using a samples of 61506 spiral galaxies selected from the SDSS DR2, we examine the luminosity function (LF) of spiral galaxies with different inclination angles. We find that the…
Understanding the Results of Galaxy-Galaxy Lensing using Galaxy-Mass Correlation in Numerical Simulations
XiaoHu Yang, H. J. Mo, Guinevere Kauffmann +1
McKay et al. (2002) have recently used measurements of weak galaxy-galaxy lensing in the Sloan Digital Sky Survey to estimate the cross correlation between galaxies and the project…
Analytical Approximations to Galaxy Clustering
H. J. Mo
We discuss some recent progress in constructing analytic approximations to the galaxy clustering. We show that successful models can be constructed for the clustering of both dark…
Constraints on the Cosmic Structure Formation Models from Early Formation of Giant Galaxies
H. J. Mo, M. Fukugita
A recent observation of Steidel et al. indicates that a substantial fraction of giant galaxies were formed at an epoch as early as redshift . We show that this early forma…
High-Order Correlations of Peaks and Halos: a Step toward Understanding Galaxy Biasing
H. J. Mo, Y. P. Jing, S. D. M. White
We develop an analytic model for the hierarchical correlation amplitudes S_j(R)= \bxi_j(R)/\bxi_2^{j-1}(R) of density peaks and dark matter halos in the quasi-linear regime. The st…
An analytic model for the spatial clustering of dark matter haloes
H. J. Mo, S. D. M. White
We develop a simple analytic model for the gravitational clustering of dark matter haloes to understand how their spatial distribution is biased relative to that of the mass. The s…