Canuto et al. 1980

Canuto, V., S.-H. Hsieh, and J.R. Owen, 1980: Possible determination of the deceleration parameter using lunar occultations and laser ranging observations. Astrophys. J., 241, 886-888, doi:10.1086/158401.

Using recent determination of the atomic and tidal lunar acceleration, we propose a model evaluate q₀. Our conclusion is that the universe is open for values of H_{0 close to 50 km/s/Mpc.}

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Canuto, V., Hsieh, S.-H., and Owen, J.R.: Possible determination of the deceleration parameter using lunar occultations and laser ranging observations, Astrophys. J., 241, 886-888, doi:10.1086/158401, 1980.

Canuto, V., S.-H. Hsieh, and J.R. Owen (1980), Possible determination of the deceleration parameter using lunar occultations and laser ranging observations, Astrophys. J., 241, 886-888, doi:10.1086/158401.

Canuto, V., S.-H. Hsieh, and J.R. Owen, 1980: Possible determination of the deceleration parameter using lunar occultations and laser ranging observations. Astrophys. J., 241, 886-888, doi:10.1086/158401.

Canuto, V., Hsieh, S.-H., & Owen, J.R. 1980, Astrophys. J., 241, 886, doi:10.1086/158401.

Canuto V, Hsieh S-H, Owen JR. Possible determination of the deceleration parameter using lunar occultations and laser ranging observations, Astrophys J 1980;241:886-888. doi:10.1086/158401.

V. Canuto, S.-H. Hsieh, J.R. Owen, Astrophys. J. 241, 886-888, doi:10.1086/158401 (1980).