... cm

Appendix A is only available in electronic form at http://www.edpsciences.org/. To download Appendix B, please see [astro-ph/0507282] or contact the author.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

...

Table 2 is also available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/445/243

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

... components

PSRs B0450+55, B1540-06, B0525+21, B1839-04, B2020+28, the outer components of B0329+54 and possibly PSR B0052+51. Also PSR B1237+25 is a known example.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

... catalogued

http://www.atnf.csiro.au/research/pulsar/psrcat/

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

... package

http://pulsar.princeton.edu/tempo/

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

... pulses

  For a few observations with a low number of pulses shorter transforms were used.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

... pulsar

 This pulsar is not in our source list, because the required observation length is too long. Therefore this pulsar is not included in the statistics.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

... short

Our observation was too short to contain the required minimum of one thousand pulses. Because we have detected drifting, we did not reobserve this pulsar.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

... pulsar

This pulsar is not in our source list, because the flux is not in the catalog. Therefore this pulsar is not included in the statistics.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

... diagram

Except PSR B1744-24A, which has a negative $\dot P$.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.