Fields for 2dF redshift survey are shown as the small black circles.
2dF galaxy slices taken from APM survey, The decrease in galaxy density at the outer edges is due, of course, to the magnitude limit of the APM survey.
2dF Quasar survey. Although there is clearly a change with epoch (redshift) at any given redshift, the distribution is homogeneous
Figures taken from the 2dF website.