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Table B.3.
Fit results for pulsars where the spectrum was modelled with a broken PL.
| PSR | Frequency | # of | Ref. | Ref. | Spectral | Break | Uncertainty | Spectral | Fitted |
|---|---|---|---|---|---|---|---|---|---|
| span | points, | freq., | flux, | index, | freq., | range for | index, | flux | |
| (MHz) | Np | ν0 | S0 | αlo | νbr | νbr | αhi | scatter, | |
| (MHz) | (mJy) | (MHz) | (MHz) |  |
|||||
| B0301+19 | 59–4850 | 35 | 500 | 24.0 | −0.5 ± 0.2 | 500 | 354–761 | −1.9 ± 0.3 | 0.11 |
| B0320+39 | 25–4850 | 26 | 300 | 52.0 | −0.9 ± 0.5 | 157 | 133–195 | −2.4 ± 0.2 | 0.10 |
| J0611+30 | 45–430 | 4 | 100 | 70.0 | −1.4 ± 1.5 | 74 | ... | −2.5 ± 0.5 | ... |
| B0809+74 | 12–14 800 | 69 | 400 | 110.0 | −0.8 ± 0.3 | 66 | 58–73 | −1.66 ± 0.06 | 0.14 |
| B0943+10 | 20–1400 | 35 | 200 | 83.0 | −0.2 ± 0.6 | 114 | 87–167 | −2.8 ± 0.7 | 0.31 |
| B1112+50 | 20–4900 | 37 | 300 | 45.0 | −1.1 ± 0.4 | 148 | 133–172 | −2.3 ± 0.2 | 0.36 |
| B1133+16 | 16–32 000 | 130 | 700 | 100.0 | −0.1 ± 0.1 | 232 | 212–257 | −1.93 ± 0.06 | 0.17 |
| J1238+21 | 25–430 | 6 | 100 | 64.0 | −0.8 ± 0.5 | 102 | ... | −2.4 ± 0.4 | ... |
| J1313+0931 | 59–1400 | 4 | 300 | 8.6 | −0.9 ± 1.3 | 149 | ... | −2.6 ± 0.3 | ... |
| B1322+83 | 25–1408 | 12 | 200 | 59.0 | −0.8 ± 0.6 | 214 | 173–306 | −2.5 ± 0.6 | 0.18 |
| B1508+55 | 20–10 750 | 59 | 500 | 52.0 | −2.4 ± 0.4 | 88 | 82–97 | −2.04 ± 0.08 | 0.14 |
| B1530+27 | 25–4850 | 22 | 300 | 17.0 | −1.3 ± 0.5 | 92 | 74–100 | −1.6 ± 0.1 | 0.05 |
| B1541+09 | 39–10 550 | 49 | 600 | 29.0 | −0.7 ± 0.4 | 144 | 133–156 | −2.15 ± 0.09 | 0.09 |
| B1633+24 | 25–1400 | 12 | 200 | 44.0 | −0.6 ± 0.5 | 155 | 131–191 | −2.3 ± 0.3 | 0.06 |
| J1645+1012 | 59–430 | 4 | 200 | 21.0 | −1.5 ± 1.7 | 102 | ... | −2.9 ± 0.5 | ... |
| B1737+13 | 45–4850 | 18 | 500 | 20.0 | −0.6 ± 0.5 | 330 | 153–556 | −1.7 ± 0.2 | 0.04 |
| B1839+09 | 59–4850 | 13 | 500 | 14.0 | −0.6 ± 0.8 | 229 | 135–294 | −1.9 ± 0.2 | 0.06 |
| B1839+56 | 20–4850 | 30 | 300 | 32.0 | −4.8 ± 1.4 | 39 | 35–41 | −1.6 ± 0.1 | 0.23 |
| B1919+21 | 16–4850 | 92 | 300 | 250.0 | −0.4 ± 0.2 | 135 | 120–149 | −2.7 ± 0.1 | 0.21 |
| B1929+10 | 20–43 000 | 98 | 900 | 110.0 | −0.3 ± 0.4 | 342 | 240–511 | −1.74 ± 0.09 | 0.23 |
| B2016+28 | 25–10 700 | 55 | 500 | 150.0 | −0.1 ± 0.2 | 331 | 293–379 | −2.27 ± 0.09 | 0.13 |
| B2020+28 | 45–32 000 | 47 | 1200 | 24.0 | −0.6 ± 0.6 | 307 | 225–430 | −1.6 ± 0.1 | 0.21 |
| B2306+55 | 59–4850 | 13 | 500 | 15.0 | −0.7 ± 0.5 | 357 | 178–532 | −2.0 ± 0.2 | 0.07 |
| B2310+42 | 25–10 700 | 34 | 500 | 130.0 | −0.1 ± 0.3 | 645 | 498–909 | −2.1 ± 0.3 | 0.18 |
| B2315+21 | 25–4850 | 16 | 400 | 17.0 | −0.6 ± 0.5 | 186 | 167–231 | −2.1 ± 0.2 | 0.06 |
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