Integrating single pulses from PSR 1541+09 in intensity bins.

This is a temporary page, just to show results of integrating single pulses from PSR 1541+09 in non-equal intensity bins. Limits of those intensity bins have been selected in such a way, that each profile is made of approximately the same number of single pulses.
Note that the first component becomes quite strong in the last intensity bin, containing the strongest pulses.

The observations were made before the upgrade of the telescope.