Table 2.
Description of the observational set-up for the data used in this paper.
| Telescope | Backend | fc | BW | Nchan | Nbin |
|---|---|---|---|---|---|
| (MHz) | (MHz) | ||||
| EFF | PSRIX | 1347.5 | 200 | 128 | 1024 |
| JBO | ROACH | 1532 | 400 | 400/1600 | 2048 |
| NRT | NUPPI | 1484 | 512 | 128 | 2048 |
| WSRT | PuMa-II | 1380 | 160 | 512 | 1024 |
Notes. We list the telescope identifier (see text), the name of the data recording device (referred to as backend), the centre frequency fc of the observations, the observing bandwidth BW (not considering RFI or band-edge removal), the number of frequency channels Nchan, and the maximum number of phase bins across the profile Nbin. For some pulsars, JBO and WSRT only had 256 phase bins, as specified in the text.
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