  We represent noise strength analysis of Anomalous X-Ray Pulsars (AXPs) 4U
0142+61, 1RXS J170849.9-400910, 1E 1841-045, 1E 2259+586 and Soft Gamma
Repeaters (SGRs) SGR J1833-0832, SWIFT J1822.3-1606 and SWIFT J1834.9-0846
together with the X-Ray binaries GX 1+4 and 4U 1907+09 for comparison with
accreting sources. Using our timing solutions, we extracted residuals of pulse
arrival times after removal of spin down trends and we calculated assoicated
noise strength of each source. Our preliminary results indicate that the noise
strength is scaling up with spin-down rate. This indicates that, increase in
spin-down rate leads to more torque noise on the magnetars. In addition, we
present our analysis with Bayesian statistics on the previously reported
transient QPO feature of 4U 1907+09.
