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Table B.2.
Fit results for pulsars with a single PL spectrum.
| PSR | Frequency | # of | Ref. | Ref. | Spectral | Fitted | PSR | Frequency | # of | Ref. | Ref. | Spectral | Fitted |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| span | points, | freq., | flux, | index, | flux | span | points, | freq., | flux, | index, | flux | ||
| (MHz) | Np | ν0 | S0 | α | scatter, | (MHz) | Np | ν0 | S0 | α | scatter, | ||
| (MHz) | (mJy) |  |
(MHz) | (mJy) |  |
||||||||
| B0011+47 | 59–4850 | 19 | 500 | 11.0 | −0.9 ± 0.1 | 0.11 | J1238+21 (♯) | 25–430 | 6 | 100 | 22.0 | −0.8 ± 0.3 | ... |
| B0053+47 | 20–4850 | 10 | 300 | 4.7 | −1.3 ± 0.2 | 0.43 | J1313+0931 (♯) | 59–1400 | 4 | 300 | 6.2 | −2.3 ± 0.3 | ... |
| B0226+70 | 59–1420 | 10 | 300 | 3.8 | −1.6 ± 0.2 | 0.08 | J1645+1012 (♯) | 59–430 | 4 | 200 | 14.0 | −2.1 ± 0.4 | ... |
| J0611+30 (♯) | 45–430 | 4 | 100 | 38.0 | −1.9 ± 0.4 | ... | J1758+3030 | 59–800 | 9 | 200 | 20.0 | −1.4 ± 0.3 | 0.11 |
| B0609+37 | 59–4850 | 13 | 500 | 5.2 | −1.4 ± 0.2 | 0.30 | B1842+14 | 47–4850 | 21 | 500 | 14.0 | −1.95 ± 0.09 | 0.05 |
| B0655+64 | 45–1408 | 15 | 300 | 14.0 | −2.0 ± 0.2 | 0.34 | B1953+50 | 59–4850 | 13 | 500 | 17.0 | −1.2 ± 0.1 | 0.08 |
| B0751+32 | 59–4850 | 10 | 500 | 4.4 | −1.4 ± 0.2 | 0.13 | B2022+50 | 59–32 000 | 15 | 1400 | 1.9 | −1.10 ± 0.08 | 0.07 |
| B0917+63 | 45–1408 | 10 | 300 | 6.3 | −1.4 ± 0.2 | 0.07 | B2224+65 | 45–10 700 | 26 | 700 | 7.7 | −1.62 ± 0.07 | 0.07 |
Notes. (♯)These pulsars have also broken PL fit, with break frequency fixed at the frequency of the largest measured flux density. See Table B.3 for the values of fitted parameters.
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