Integrating single pulses from PSR 1133+16 in intensity bins.

This is a temporary page, just to show results of integrating single pulses from PSR 1133+16 in intensity bins.

The observations were made before the upgrade of the telescope.

Data set S (1990 single pulses). Limits of the intensity bins have been selected in such a way, that each profile is made of approximately the same number of single pulses.
Note a change of width of the profile with intensity.:

Data set N (3705 pulses, better S/N ratio). In this case equal intensity bins were used, as a result profiles are made of different number of single pulses: