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Table B.1

List of the 100 pulsars and their rotational and derived parameters.

PSR Name P Ṗ Epoch LBA Epoch HBA Epoch D M eph D M HBA log τ log B log Ė Notes
[s] [s s-1] [MJD] [MJD] [MJD] [cm-3 pc] [cm-3 pc] [yr] [G] [s-1 erg]
B0011+47 1.241 5.647e - 16 55 316 55 858 30.67(7)[1] 30.3(5) 7.54 11.93 31.07 WESd
B0031−07 0.943 4.081e - 16 55 857 56 630 11.28(8)[1] 10.9(4) 7.56 11.80 31.28 WESd
J0051+0423 0.355 7.047e - 18 49 800 56 318 13.9(1)[2] 13.93(1) 8.90 10.70 30.79 LOTAASb
B0059+65 1.679 5.970e - 15 56 475 55 859 65.85(2)[1] 65.8(8) 6.65 12.51 31.70 EPNd
B0105+65 1.284 1.292e - 14 54 578 55 859 30.6(5)[1] 30.6(2) 6.20 12.62 32.38 P- 2004c
B0114+58 0.101 5.846e - 15 55 829 55 859 49.462(4)[1] 49.42(1) 5.44 11.89 35.34 EPNd
B0136+57 0.272 1.069e - 14 54 589 55 859 73.776(6)[1] 73.83(1) 5.61 12.24 34.32 P-, L- 2004b
B0138+59 1.223 3.910e - 16 54 266 55 924 55 859 34.74(1)[1] 34.92(2) 7.70 11.84 30.93 P- 2004c
B0301+19 1.388 1.295e - 15 55 743 55 859 15.851(9)[1] 15.65(4) 7.23 12.13 31.28 WESd
B0320+39 3.032 6.358e - 16 54 125 55 924 55 859 25.99(3)[1] 26.19(1) 7.88 12.15 29.95 P- 2002c
B0329+54 0.715 2.046e - 15 53 850 55 859 55 859 26.7941(1)[3] 26.7653(<1) 6.74 12.09 32.35 P- 2000c
B0331+45 0.269 7.331e - 18 55 899 55 859 47.149(3)[1] 47.15(1) 8.76 10.65 31.17 EPNd
B0339+53 1.934 1.342e - 14 55 804 55 859 67.28(6)[1] 67.5(2) 6.36 12.71 31.86 WESd
B0355+54 0.156 4.395e - 15 53 813 55 859 57.1226(3)[4] 57.14(1) 5.75 11.92 34.66 P- 2003c
B0402+61 0.595 5.576e - 15 56 097 55 859 65.303(7)[1] 65.39(3) 6.23 12.27 33.02
B0410+69 0.391 7.656e - 17 54 418 55 859 27.471(4)[1] 27.44(1) 7.91 11.24 31.70 P- 2004c
B0447−12 0.438 1.028e - 16 55 203 56 568 37.04(1)[1] 37.01(1) 7.83 11.33 31.68 P- 2003c
B0450+55 0.341 2.377e - 15 54 139 55 924 55 861 14.483(7)[1] 14.59(7) 6.36 11.96 33.38 P-, L- 2004c
B0450−18 0.549 5.755e - 15 55 203 56 603 39.903(3)[1] 39.91(2) 6.18 12.25 33.14 P- 2004c
B0523+11 0.354 7.362e - 17 55 202 56 568 79.423(3)[1] 79.43(4) 7.88 11.21 31.81 P- 2006c
B0525+21 3.746 4.004e - 14 54 457 55 924 56 596 50.96(2)[1] 50.87(2) 6.17 13.09 31.48 P- 2003, L- 2004c
B0540+23 0.246 1.542e - 14 54 748 55 859 77.631(2)[1] 77.7(9) 5.40 12.29 34.61 P- 2006c
B0609+37 0.298 5.980e - 17 54 590 55 859 27.136(4)[1] 27.15(3) 7.90 11.13 31.95 P- 2006c
B0611+22 0.335 5.911e - 14 55 604 56 681 96.94(7)[1] 96.92(1) 4.95 12.65 34.79 WESd
B0626+24 0.477 1.985e - 15 55 071 55 859 84.19(4)[1] 84.18(3) 6.58 11.99 32.86 P- 2004c
B0643+80 1.214 3.799e - 15 54 855 55 859 33.33(2)[1] 33.3(1) 6.70 12.34 31.92 P- 2004c
B0809+74 1.292 1.660e - 16 53 508 56 046 55 916 5.733(1)[3] 5.75(3) 8.09 11.67 30.48 WESd
B0818−13 1.238 2.105e - 15 55 507 56 603 40.949(3)[1] 40.98(1) 6.97 12.21 31.64 WESd
B0820+02 0.865 1.047e - 16 55 508 56 301 23.717(6)[1] 23.76(7) 8.12 11.48 30.81 WESd
B0823+26 0.531 1.679e - 15 55 419 55 889 55 966 19.464(4)[1] 19.4711(<1) 6.70 11.98 32.65 WESd
B0834+06 1.274 6.799e - 15 55 507 55 883 55 881 12.891(6)[1] 12.8735(<1) 6.47 12.47 32.11 WESd
B0906−17 0.402 6.693e - 16 54 887 56 603 15.885(3)[1] 15.87(1) 6.98 11.72 32.61 WESd
B0917+63 1.568 3.608e - 15 53 883 55 925 55 860 13.21(2)[1] 13.14(2) 6.84 12.38 31.57 EPNd
B0919+06 0.431 1.372e - 14 55 870 56 315 27.256(6)[1] 27.3(1) 5.70 12.39 33.83 WESd
B0943+10 1.098 3.546e - 15 54 226 55 925 55 869 15.2(5)[1] 15.32(1) 6.69 12.30 32.02 EPNd
B0950+08 0.253 2.165e - 16 51 541 55 889 56 603 2.961(3)[1] 2.9696(<1) 7.27 11.37 32.72 EPNd
B1112+50 1.656 2.493e - 15 54 121 55 925 56 233 9.202(8)[1] 9.18(1) 7.02 12.31 31.34 WESd
B1133+16 1.188 3.733e - 15 56 235 55 925 55 916 4.8611(1)[3] 4.8262(<1) 6.70 12.33 31.94 WESd
B1237+25 1.382 9.596e - 16 46 498 55 925 55 860 9.254(6)[1] 9.2538(<1) 7.36 12.07 31.16 WESd
J1238+21 1.119 1.445e - 15 55 507 55 860 17(2)[1] 17.97(3) 7.09 12.11 31.61
J1313+0931 0.849 8.000e - 16 50 984 55 860 12.0(1)[5] 12.05(2) 7.23 11.92 31.71
B1322+83 0.670 5.675e - 16 53 763 55 860 13.3(2)[1] 13.31(3) 7.27 11.80 31.87 WESd
B1508+55 0.740 5.007e - 15 55 168 55 906 55 860 19.59(2)[1] 19.6179(<1) 6.37 12.29 32.69 WESd
B1530+27 1.125 7.791e - 16 56 508 55 859 14.76(2)[1] 14.7(2) 7.36 11.98 31.33 WESd
B1540−06 0.709 8.810e - 16 55 962 55 892 56 605 18.403(4)[1] 18.3788(<1) 7.11 11.90 31.99 WESd
B1541+09 0.748 4.328e - 16 55 508 55 892 55 859 35.24(3)[1] 34.97(3) 7.44 11.76 31.61 WESd
B1604−00 0.422 3.063e - 16 54 696 55 892 56 346 10.687(5)[1] 10.69(1) 7.34 11.56 32.21 WESd
B1612+07 1.207 2.360e - 15 55 508 56 354 21.39(3)[1] 21.41(1) 6.91 12.23 31.72 WESd
J1627+1419 0.491 3.930e - 16 48 957 55 859 33.8(6)[6] 32.18(9) 7.30 11.65 32.12
B1633+24 0.491 1.192e - 16 55 508 56 517 55 859 24.33(4)[1] 24.27(1) 7.81 11.39 31.60 EPNd
B1642−03 0.388 1.770e - 15 55 643 56 605 35.738(3)[1] 35.7556(<1) 6.54 11.92 33.08 WESd
J1645+1012 0.411 8.203e - 17 52 814 56 276 36.4(6)[6] 36.18(3) 7.90 11.27 31.67
J1652+2651 0.916 6.542e - 16 55 507 55 860 41.0(2)[2] 40.79(2) 7.35 11.89 31.53 WESd
B1737+13 0.803 1.441e - 15 55 507 55 870 48.672(4)[1] 48.67(1) 6.95 12.04 32.04 WESd
B1749−28 0.563 8.000e - 15 54 111 56 606 50.39(8)[1] 50.38(1) 6.05 12.33 33.25 WESd
B1818−04 0.598 6.347e - 15 56 445 56 606 84.42(2)[1] 84.34(3) 6.17 12.29 33.07 WESd
B1821+05 0.753 2.267e - 16 55 508 56 286 66.777(3)[1] 66.79(2) 7.72 11.62 31.32 LOTAASb
B1822−09 0.769 5.249e - 14 56 183 55 892 56 605 19.36(4)[1] 19.36(2) 5.37 12.81 33.66 WESd
B1831−04 0.290 7.250e - 17 55 508 56 605 79.302(8)[1] 79.39(4) 7.80 11.17 32.07 WESd
B1839+09 0.381 1.089e - 15 55 541 55 870 49.145(8)[1] 49.1501(<1) 6.74 11.81 32.89 WESd
B1839+56 1.653 1.495e - 15 55 508 55 892 55 870 26.71(1)[1] 26.7540(<1) 7.24 12.20 31.12 WESd
B1842+14 0.375 1.873e - 15 55 817 55 864 55 870 41.512(4)[1] 41.48(1) 6.50 11.93 33.15 WESd
B1848+12 1.205 1.137e - 14 55 835 56 276 70.61(2)[1] 70.6(8) 6.23 12.57 32.41 LOTAASb, WESd
B1848+13 0.346 1.493e - 15 55 508 56 276 60.149(8)[1] 60.1(1) 6.56 11.86 33.15 LOTAASb, EPNd
B1857−26 0.612 2.050e - 16 55 508 55 870 37.993(5)[1] 37.92(3) 7.68 11.55 31.55 WESd
B1905+39 1.236 5.408e - 16 55 507 55 870 30.96(3)[1] 30.98(5) 7.56 11.92 31.05 WESd
B1907+00 1.017 5.513e - 15 55 770 56 354 112.776(6)[1] 113(1) 6.47 12.38 32.32 LOTAASb, WESd
B1907+02 0.990 5.492e - 15 53 773 56 339 171.722(9)[1] 172(1) 6.46 12.37 32.35 LOTAASb, WESd
B1907+10 0.284 2.644e - 15 55 729 55 870 149.756(4)[1] 149.9(1) 6.23 11.94 33.66 WESd
B1911−04 0.826 4.069e - 15 55 705 56 354 89.38(1)[1] 89.38(3) 6.51 12.27 32.46 LOTAASb, WESd
B1914+09 0.270 2.518e - 15 55 931 55 870 60.981(6)[1] 61.01(6) 6.23 11.92 33.70 WESd
B1915+13 0.195 7.194e - 15 55 745 55 870 94.54(4)[1] 94.65(3) 5.63 12.08 34.59 WESd
B1917+00 1.272 7.675e - 15 55 695 56 354 90.27(2)[1] 90(1) 6.42 12.50 32.17 LOTAASb, WESd
B1918+26 0.786 3.414e - 17 54 142 55 870 27.68(9)[1] 27.7(1) 8.56 11.22 30.44 EPNd
B1919+21 1.337 1.349e - 15 55 969 55 860 55 859 12.4632(1)[3] 12.4453(<1) 7.20 12.13 31.35 WESd
B1920+21 1.078 8.169e - 15 55 507 55 859 217.08(2)[1] 217.0(1) 6.32 12.48 32.41 WESd
B1923+04 1.074 2.459e - 15 55 445 56 339 102.24(2)[1] 102.2(9) 6.84 12.22 31.89 LOTAASb, WESd
B1929+10 0.227 1.157e - 15 55 830 55 913 55 859 3.178(4)[1] 3.18(1) 6.49 11.71 33.59 WESd
B1953+50 0.519 1.374e - 15 55 508 55 864 55 858 31.974(3)[1] 31.98(1) 6.78 11.93 32.59 EPNd
B2021+51 0.529 3.066e - 15 55 889 55 858 22.634(6)[1] 22.55(1) 6.44 12.11 32.91 WESd
B2022+50 0.373 2.515e - 15 55 507 55 859 33.036(3)[1] 33.0(2) 6.37 11.99 33.28 WESd
B2043−04 1.547 1.471e - 15 55 311 56 324 35.81(1)[1] 36(1) 7.22 12.18 31.20 WESd
B2044+15 1.138 1.823e - 16 55 507 56 293 39.86(1)[1] 39.8(1) 8.00 11.66 30.69 LOTAASb, P-2004c
B2106+44 0.415 8.606e - 17 55 855 56 602 139.83(1)[1] 140(1) 7.88 11.28 31.68 WESd
B2110+27 1.203 2.623e - 15 55 424 56 602 25.119(4)[1] 25.1(1) 6.86 12.25 31.77 WESd
B2113+14 0.440 2.895e - 16 55 696 55 859 56.15(7)[1] 56.2(1) 7.38 11.56 32.13 WESd
B2122+13 0.694 7.677e - 16 55 507 56 332 30.1(1)[1] 30.3(2) 7.16 11.87 31.96 LOTAASb, EPNd
B2148+63 0.380 1.707e - 16 55 769 55 858 129.704(1)[7] 129.7(2) 7.55 11.41 32.09 WESd
B2154+40 1.525 3.439e - 15 55 334 55 858 70.86(1)[1] 71.14(6) 6.85 12.37 31.58 WESd
B2217+47 0.538 2.767e - 15 56 228 55 860 55 858 43.49(1)[1] 43.4811(<1) 6.49 12.09 32.84 WESd
B2224+65 0.683 9.647e - 15 55 964 55 858 36.08(9)[1] 36.33(5) 6.05 12.41 33.08 WESd
B2227+61 0.443 2.255e - 15 55 859 55 858 124.62(2)[1] 124.7(1) 6.49 12.00 33.01 WESd
J2248−0101 0.477 6.596e - 16 56 405 56 304 29.06(3)[1] 29.1(4) 7.06 11.75 32.38 LOTAASb, WESd
J2253+1516 0.792 6.653e - 17 49 079 56 354 29.182(9)[8] 29(1) 8.28 11.37 30.72 LOTAASb
B2255+58 0.368 5.749e - 15 55 671 55 858 151.082(6)[1] 151.2(1) 6.01 12.17 33.66 WESd
B2303+30 1.576 2.893e - 15 54 584 55 892 55 858 49.56(2)[1] 49.58(5) 6.94 12.33 31.47 WESd
B2306+55 0.475 1.995e - 16 55 384 55 858 46.535(8)[1] 46.54(2) 7.58 11.49 31.87 WESd
B2310+42 0.349 1.123e - 16 54 363 55 860 56 606 17.274(1)[1] 17.27(1) 7.69 11.30 32.02 EPNd
B2315+21 1.445 1.047e - 15 56 407 55 858 20.874(7)[1] 20.87(6) 7.34 12.10 31.14 P- 2004c
B2334+61 0.495 1.933e - 13 55 508 55 858 58.41(2)[1] 58.43(3) 4.61 13.00 34.80 WESd

Notes.

(a)

For each DM measurement and its error we quote the reference paper: 1, 2, 3, 4, 5, 6, 7, and 8.

(b)

Observations from the LOTAAS survey (Coenen et al. 2014).

(c)

Year of the P- and/or L-band data from WSRT observations. L-band data were obtained from Lovell observations in all but the three cases where the year of the WSRT observations is indicated. All the L-band observations using the Lovell telescope were performed between October 2011 and November 2013.

(d)

Where P-band data were available from Weltevrede et al. (2005), but no absolute reference was available to align the data with LOFAR data, reference is made to their paper as WES and the corresponding profile in Fig. B.1 was aligned by eye. For completeness, where the pulsar was not in WES, then EPN indicates that the profile in P-band was obtained from the EPN pulsar database and was also only aligned by eye. In this latter case, the observations are not later than 2002. In the cases where nothing is specified, for the P-band the profile is either missing in all the databases used here or the Lovell data were used and the profile aligned with the standard procedure as described in the text.

Reference. (1) Hobbs et al. (2004); (2) Sayer et al. (1997); (3) Hassall et al. (2012); (4) Janssen & Stappers (2006); (5) Lommen et al. (2000); (6) Lewandowski et al. (2004); (7) Hamilton & Lyne (1987); (8) Camilo & Nice (1995).

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