Distance PDF for G136.84+01.12, a 6.7 GHz methanol maser at ﹩v=-45﹩ km s⁻¹ from the Pestalozzi et al. (2005) catalog. The (l, b, v)_src values associate it with the Perseus spiral arm centered near 2.4 kpc (red dashed line). This information, coupled with association with the parallax source G133.95+01.05 (blue dotted line), favors the distance estimate of 1.96 ± 0.04 kpc over the arm center. Note that the kinematic distance (green dotted–dashed line) suggests a much greater distance of 3.7 kpc, as it does for many sources in this part of the Perseus arm which is known to be kinematically anomalous.