. Presented are measurements from the Las Campanas Redshift Survey (LCRS) of the galaxy-galaxy autocorrelation function in redshiftspace, ? gg (s). For separations 2:0h \Gamma1 Mpc ! s ! 16:4h \Gamma1...
. Presented are measurements from the Las Campanas Redshift Survey (LCRS) of the galaxy-galaxy autocorrelation function in redshiftspace, ? gg (s). For separations 2:0h \Gamma1 Mpc ! s ! 16:4h \Gamma1...
The rate of mass accumulation due to galaxy merging depends on the mass, density, and velocity distribution of galaxies in the near neighborhood of a host galaxy. The fractional luminosity in kinemati...
. Presented are measurements from the Las Campanas Redshift Survey (LCRS) of the galaxy-galaxy autocorrelation function in redshiftspace, ? gg (s). For separations 2:0h \Gamma1 Mpc ! s ! 16:4h \Gamma1...
We present a new statistic---the redshift dispersion--- which may prove useful for comparing next generation redshift surveys (e.g., the Sloan Digital Sky Survey) and cosmological simulations. Our sta...
We have carried out a survey to search for hidden blazars in a sample of z2 radio-loud quasars. The idea is based on our prediction that we should be able to see large CIV line variability not associa...
We have carried out a survey to search for hidden blazars in a sample of z2 radio-loud quasars. The idea is based on our prediction that we should be able to see large CIV line variability not associa...
We have carried out a survey to search for hidden blazars in a sample of z2 radio-loud quasars. The idea is based on our prediction that we should be able to see large CIV line variability not associa...