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+0451 . | J0034−0534 . | B0950+08 . | J1400−1431 . | J2145−0750 . |
---|---|---|---|---|---|
T1 | 13.2 | 51.2 | 0 | 2.2 | 21.7 |
T2 | 18.1 | 11.7 | 3 | 11.7 | 30 |
slow | 21.1 | 71.2 | 0.7 | 4.6 | 28.5 |
fast | 42.5 | 44.4 | 7.8 | 26.5 | 45.5 |
wsa | 14.6 | 3.6 | 1.7 | −1.5 | 16.8 |
. | J0030+0451 . | J0034−0534 . | B0950+08 . | J1400−1431 . | J2145−0750 . |
---|---|---|---|---|---|
T1 | 13.2 | 51.2 | 0 | 2.2 | 21.7 |
T2 | 18.1 | 11.7 | 3 | 11.7 | 30 |
slow | 21.1 | 71.2 | 0.7 | 4.6 | 28.5 |
fast | 42.5 | 44.4 | 7.8 | 26.5 | 45.5 |
wsa | 14.6 | 3.6 | 1.7 | −1.5 | 16.8 |
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+0451 . | J0034−0534 . | B0950+08 . | J1400−1431 . | J2145−0750 . |
---|---|---|---|---|---|
T1 | 13.2 | 51.2 | 0 | 2.2 | 21.7 |
T2 | 18.1 | 11.7 | 3 | 11.7 | 30 |
slow | 21.1 | 71.2 | 0.7 | 4.6 | 28.5 |
fast | 42.5 | 44.4 | 7.8 | 26.5 | 45.5 |
wsa | 14.6 | 3.6 | 1.7 | −1.5 | 16.8 |
. | J0030+0451 . | J0034−0534 . | B0950+08 . | J1400−1431 . | J2145−0750 . |
---|---|---|---|---|---|
T1 | 13.2 | 51.2 | 0 | 2.2 | 21.7 |
T2 | 18.1 | 11.7 | 3 | 11.7 | 30 |
slow | 21.1 | 71.2 | 0.7 | 4.6 | 28.5 |
fast | 42.5 | 44.4 | 7.8 | 26.5 | 45.5 |
wsa | 14.6 | 3.6 | 1.7 | −1.5 | 16.8 |
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