Cosmological Constraints from Type Ia Supernovae Peculiar Velocity Measurements

We detect the correlated peculiar velocities of nearby type Ia supernovae (SNe), while highlighting an error in some of the literature. We find ${\sigma }_8=0.79\pm 0.22$ from SNe, and examine the potential of this method to constrain cosmological parameters in the future. We demonstrate that a survey of 300 low-$z$ SNe (such as the nearby SNfactory) will underestimate the errors on $w$ by $\sim 35\%$ if the coherent peculiar velocities are not included.