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Table 4.

Properties estimated for re-detected and newly discovered pulsars.

Cluster Fc Smin Redetections S/N Sobs Sexp Spectral Scattering τscat, fref
(MHz) (mJy) (mJy) (mJy) Index Index (ms, MHz) (ms)
NGC 1851 400 0.206 A 126.6 2.717 Not measurably scattered 0.03
Terzan 5 650 0.143 A 384.2 7.491 4.08 −2.420 −3.2(1) 0.640(9), 640 5.48
C 33.4 0.915
D 12.2 0.309 0.19 −1.797
F 10.5 0.223 0.17 −1.649
H 12.2 0.310 0.07 −2.694
I 12.9 0.175 0.29(7), 700 3.57
J 18.9 0.199 0.09 −2.088
L 18.6 0.371 0.19 −3.030
M 15.0 0.503 0.26 −1.407
N 18.2 0.292 0.15 −2.314 0.56(19), 625 5.49
O 14.2 0.344 0.57 −1.138
U 10.3 0.345 −2.732
NGC 6440 650 0.099 A 178.8 4.234 1.72 −2.197 Not measurably scattered 3.25
B 10.9 0.332 0.22 −1.747
D 8.2 0.248 0.36 −1.062
NGC 6441 650 0.105 A 14.6 0.192 0.28 −1.156
B 12.9 0.432 0.17 −2.188
NGC 6539 400 0.099 A 94.1 2.263 3.08 3.80(83), 412 7.82
NGC 6544 650 0.099 A 105.9 2.628 4.05 −1.273 −4.0(5) 0.25(2), 662 0.25
B 21.2 0.414 0.42 −1.378 0.37(12), 600 0.41
NGC 6652 400 0.205 B 31.6 1.01 0.174(3), 330 0.142

Notes. Fc represents the central frequency of observation, Smin is the minimum detection threshold for each cluster, Sobs is the observed flux density, Sexp is the expected flux density (assuming spectral index of −1.4 if unspecified by ATNF catalogue), τscat is the measured scattering timescale at reference frequency fref, and is the theoretical estimate of scattering timescale at frequency fref (calculated from the relation by Bhat et al. 2004).

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