Table 3.

This table shows the average time derivative of DM after subtracting solar wind amplitudes and the median DM uncertainty of our data. The time derivative is calculated after binning the data SW model subtracted data for >10° elongation angle.

J0030+0451J0034−0534B0950+08B1257+12J1400−1431J2145−0750
|$\frac{\mathrm{ d}\mathrm{ (DM)}}{\mathrm{ d}t} \left(\times 10^{-5} \frac{\mathrm{ pc}}{\mathrm{ cm}^{3}\, \mathrm{ yr}^{1}}\right)$|6.5 ± 1.2−5.0 ± 1.10.5 ± 1.9−31.5 ± 5.328.0 ± 1.210.5 ± 1.6
|$M(\mathrm{ eDM})\ (\times 10^{-5} \,{\mathrm{ pc}}\,{\mathrm{ cm}^{-3}})$|3.00.652.675.980.942.53
J0030+0451J0034−0534B0950+08B1257+12J1400−1431J2145−0750
|$\frac{\mathrm{ d}\mathrm{ (DM)}}{\mathrm{ d}t} \left(\times 10^{-5} \frac{\mathrm{ pc}}{\mathrm{ cm}^{3}\, \mathrm{ yr}^{1}}\right)$|6.5 ± 1.2−5.0 ± 1.10.5 ± 1.9−31.5 ± 5.328.0 ± 1.210.5 ± 1.6
|$M(\mathrm{ eDM})\ (\times 10^{-5} \,{\mathrm{ pc}}\,{\mathrm{ cm}^{-3}})$|3.00.652.675.980.942.53
Table 3.

This table shows the average time derivative of DM after subtracting solar wind amplitudes and the median DM uncertainty of our data. The time derivative is calculated after binning the data SW model subtracted data for >10° elongation angle.

J0030+0451J0034−0534B0950+08B1257+12J1400−1431J2145−0750
|$\frac{\mathrm{ d}\mathrm{ (DM)}}{\mathrm{ d}t} \left(\times 10^{-5} \frac{\mathrm{ pc}}{\mathrm{ cm}^{3}\, \mathrm{ yr}^{1}}\right)$|6.5 ± 1.2−5.0 ± 1.10.5 ± 1.9−31.5 ± 5.328.0 ± 1.210.5 ± 1.6
|$M(\mathrm{ eDM})\ (\times 10^{-5} \,{\mathrm{ pc}}\,{\mathrm{ cm}^{-3}})$|3.00.652.675.980.942.53
J0030+0451J0034−0534B0950+08B1257+12J1400−1431J2145−0750
|$\frac{\mathrm{ d}\mathrm{ (DM)}}{\mathrm{ d}t} \left(\times 10^{-5} \frac{\mathrm{ pc}}{\mathrm{ cm}^{3}\, \mathrm{ yr}^{1}}\right)$|6.5 ± 1.2−5.0 ± 1.10.5 ± 1.9−31.5 ± 5.328.0 ± 1.210.5 ± 1.6
|$M(\mathrm{ eDM})\ (\times 10^{-5} \,{\mathrm{ pc}}\,{\mathrm{ cm}^{-3}})$|3.00.652.675.980.942.53
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