Table 2.

This table shows the percentage change in calculated RMS values between cut-off angular separations of 40° and 15°, with respect to the value at 40°, for different pulsars and SW models.

J0030+0451J0034−0534B0950+08J1400−1431J2145−0750
T113.251.202.221.7
T218.111.7311.730
slow21.171.20.74.628.5
fast42.544.47.826.545.5
wsa14.63.61.7−1.516.8
J0030+0451J0034−0534B0950+08J1400−1431J2145−0750
T113.251.202.221.7
T218.111.7311.730
slow21.171.20.74.628.5
fast42.544.47.826.545.5
wsa14.63.61.7−1.516.8
Table 2.

This table shows the percentage change in calculated RMS values between cut-off angular separations of 40° and 15°, with respect to the value at 40°, for different pulsars and SW models.

J0030+0451J0034−0534B0950+08J1400−1431J2145−0750
T113.251.202.221.7
T218.111.7311.730
slow21.171.20.74.628.5
fast42.544.47.826.545.5
wsa14.63.61.7−1.516.8
J0030+0451J0034−0534B0950+08J1400−1431J2145−0750
T113.251.202.221.7
T218.111.7311.730
slow21.171.20.74.628.5
fast42.544.47.826.545.5
wsa14.63.61.7−1.516.8
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