activity
19942002
most citedAccurate fitting formula for the two-point correlation function of the dark matter halos

230 citations · 557 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph2002

Slow relative motion of IRAS galaxies at small separations: implications for galaxy formation models

Y. P. Jing, G. Boerner, Yasushi Suto

We report on the measurement of the two-point correlation function and the pairwise peculiar velocity of galaxies in the IRAS PSCz survey. The real space two-point correlation func…

astro-ph2001★ 63 cited

Spatial correlation functions and the pairwise peculiar velocity dispersion of galaxies in the PSCz survey: implications for the galaxy biasing in cold dark matter models

Y. P. Jing, G. Boerner, Yasushi Suto

We report on the measurement of the two-point correlation function, and the pairwise peculiar velocity of galaxies in the IRAS PSCz survey. We compute these statistics first in red…

astro-ph2000

Dark Matter Halos Simulated with Million Particles

Y. P. Jing, Yasushi Suto

We report a series of high-resolution N-body simulations designed to examine the internal physical properties of dark matter halos. A total of fifteen halos, each represented by $\…

astro-ph1999★ 18 cited

Two-point correlation functions of X-ray selected clusters of galaxies: theoretical predictions for flux-limited surveys

Yasushi Suto, Kazuhiro Yamamoto, Tetsu Kitayama +1

We have developed a model to describe two-point correlation functions of clusters of galaxies in X-ray flux-limited surveys. Our model properly takes account of nonlinear gravitati…

astro-ph1999★ 36 cited

Deciphering cosmological information from redshift surveys of high-z objects - the cosmological light-cone effect and redshift-space distortion -

Yasushi Suto, Hiromitsu Magira, Y. P. Jing +2

The three-dimensional distribution of astronomical objects observed in redshift space significantly differs from the true distribution since the distance to each object cannot be d…

astro-ph1999★ 61 cited

Accurate determination of the Lagrangian bias for the dark matter halos

Y. P. Jing

We use a new method, the cross power spectrum between the linear density field and the halo number density field, to measure the Lagrangian bias for dark matter halos. The method h…