The Megamaser Cosmology Project. XI. A Geometric Distance to CGCG 074-064

As part of the survey component of the Megamaser Cosmology Project, we have discovered a disk megamaser system in the galaxy CGCG 074-064. Using the Green Bank Telescope and the Very Large Array, we have obtained spectral monitoring observations of this maser system at a monthly cadence over the course of two years. We find that the systemic maser features display line-of-sight accelerations of ∼4.4 km s^-1 yr^-1 that are nearly constant with velocity, while the high-velocity maser features show accelerations that are consistent with zero. We have also used the High-Sensitivity Array to make a high-sensitivity very long baseline interferometric map of the maser system in CGCG 074-064, which reveals that the masers reside in a thin, edge-on disk with a diameter of ∼1.5 mas (0.6 pc). Fitting a three-dimensional warped disk model to the data, we measure a black hole mass of ${2.42}_{-0.20}^{+0.22}\times {10}^{7}\,{M}_{\odot }$ and a geometric distance to the system of ${87.6}_{-7.2}^{+7.9}$ Mpc. Assuming a cosmic microwave background-frame recession velocity of 7308 ± 150 km s^-1, we constrain the Hubble constant to ${H}_{0}={81.0}_{-6.9}^{+7.4}$ (stat.) ± 1.4 (sys.) km s^-1 Mpc^-1.