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Table B.4.
Fit results for pulsars where the spectrum was modelled by a PL with two breaks.
| PSR | Frequency | # of | Ref. | Ref. | Spectral | Lower | Uncertainty | Spectral | Higher | Uncertainty | Spectral | Fitted |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| span | points, | freq., | flux, | index, | break | range for | index | break | range for | index, | flux | |
| (MHz) | Np | ν0 | S0 | αlo | freq., |  |
αmid | freq., |  |
αhi | scatter, | |
| (MHz) | (mJy) |  |
(MHz) |  |
(MHz) |  |
||||||
| (MHz) | (MHz) | |||||||||||
| B0450+55 | 25–14 600 | 24 | 600 | 30.0 | −0.5 ± 1.4 | 94 | 45–243 | −1.3 ± 0.5 | 1914 | 708–4676 | −1.8 ± 0.7 | 0.31 |
| B0823+26 | 20–32 000 | 86 | 800 | 39.0 | −2.0 ± 0.8 | 54 | 45–65 | −1.25 ± 0.08 | 2808 | 1199–4182 | −2.2 ± 0.3 | 0.08 |
| B1237+25 | 20–24 620 | 82 | 700 | 48.0 | −2.6 ± 1.4 | 55 | 36–69 | −0.9 ± 0.2 | 843 | 709–917 | −2.2 ± 0.1 | 0.13 |
| B1811+40 | 59–2600 | 12 | 400 | 10.0 | −0.9 ± 0.6 | 260 | 130–413 | −1.4 ± 0.6 | 956 | 711–1060 | −2.8 ± 0.6 | 0.06 |
| B2217+47 | 35–4900 | 39 | 400 | 110.0 | −1.0 ± 0.4 | 241 | 147–357 | −2.7 ± 0.6 | 1257 | 711–1574 | −1.8 ± 0.8 | 0.20 |
| B2303+30 | 49–4850 | 19 | 500 | 14.0 | −0.5 ± 0.4 | 337 | 236–418 | −2.7 ± 0.6 | 928 | 726–1057 | −1.2 ± 0.4 | 0.06 |
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