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Table 2

Previous observations of the ten pulsars for scintillation parameters.

PSRs Freq. Δνd Δtd Reference PSRs Freq. Δνd Δtd Reference
(MHz) (MHz) (min) (MHz) (MHz) (min)
B0329+54 327 0.165 5.12 Bhat et al. (1999b) B0540+23 430 0.0019 – Cordes et al. (1985)
327 0.02a – Wolszczan (1983) 1380 0.150 – Cordes et al. (1985)
330 0.016a – Wolszczan et al. (1981) 1410 0.31 – Cordes et al. (1985)
340 0.023a – Armstrong & Rickett (1981) 1420 0.28 – Cordes et al. (1985)
408 0.047 3.23 Gupta et al. (1994) 1420 0.317 – Cordes et al. (1985)
408 0.083 4.5 Lyne & Smith (1982) 4750 – 8 Malofeev et al. (1996)
410 0.056a – Armstrong & Rickett (1981) 10550 – 8 Malofeev et al. (1996)
410 0.07a – Rickett (1970) B0740−28 660 – 0.97 Johnston et al. (1998)
410 0.100 – Rickett (1977) 4750 – 5 Malofeev et al. (1996)
480 0.103 – Wolszczan (1983) 4800 8.83 10.63 Johnston et al. (1998)
610 0.13 4.43 Safutdinov et al. (2017) 8400 40.0 37.67 Johnston et al. (1998)
610 0.22 5.34 Safutdinov et al. (2017) 10550 – 3.5 Malofeev et al. (1996)
610 0.348a – Rickett (1970) B1508+55 327 0.168 2.63 Bhat et al. (1999b)
610 0.349 5.90 Stinebring et al. (1996) 327 0.226 2.73 Bhat et al. (1999b)
960 0.92 12.94 Smith & Wright (1985) 340 0.139a – Armstrong & Rickett (1981)
1410 2 – Wolszczan et al. (1974) 408 0.8 3 Smith & Wright (1985)
1420 5.93 15.52 Safutdinov et al. (2017) 408 1.67 – Lyne & Smith (1982)
1540 14 16.9 Wang et al. (2005) 410 0.13a – Rickett (1970)
1540 9.2 17.1 Wang et al. (2008) 930 – 1.35 Lyne & Smith (1982)
4750 – 21 Malofeev et al. (1996) B1933+16 1410 0.125 – Wolszczan et al. (1974)
4800 – 42.7 Lewandowski et al. (2011) 1416 0.037a – Wolszczan (1983)
10550 – 23 Malofeev et al. (1996) 1420 0.1 – Rickett (1977)
B0355+54 325 0.06 1.01 Safutdinov et al. (2017) 1670 0.110 0.75 Roberts & Ables (1982)
408 – 1.83 Lyne & Smith (1982) B2154+40 1000 0.195 0.503 Cordes (1986)
410 0.018a – Armstrong & Rickett (1981) 1420 0.20 0.55 Safutdinov et al. (2017)
930 0.765 – Lyne & Smith (1982) B2310+42 327 0.114 5.15 Bhat et al. (1999b)
960 0.613 4.31 Smith & Wright (1985) B2324+60 – – – –
1410 0.575 – Wolszczan et al. (1974) B2351+61 10550 – 15 Malofeev et al. (1996)
4750 – 12.5 Malofeev et al. (1996)
10550 – 13.5 Malofeev et al. (1996)

Notes. (a) Decorrelation bandwidths rescaled to the half-maximum of the correlation functions according to Cordes et al. (1985) by assuming Kolmogorov irregularity for the interstellar medium.

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