Kim, Alex, Aldering, G., Antilogus, P., Bahmanyar, A., BenZvi, S., Courtois, H., Davis, T., Ferraro, S., Gontcho, S. Gontcho, Graur, O., Graziani, R., Guy, J., Harper, C., Hlozek, R., Howlett, C., Huterer, D., Ju, C., Leget, P. F., Linder, E. V., McDonald, P. Nordin, Nugent, P., Perlmutter, S., Regnault, N., Rigault, M., Shafieloo, A., Slosar, A., Tully, R. B., White, M., and Wood-Vasey, M. Testing Gravity Using Type Ia Supernovae Discovered by Next-Generation Wide-Field Imaging Surveys. Retrieved from https://par.nsf.gov/biblio/10120208. Bulletin of the American Astronomical Society .

Kim, Alex, Aldering, G., Antilogus, P., Bahmanyar, A., BenZvi, S., Courtois, H., Davis, T., Ferraro, S., Gontcho, S. Gontcho, Graur, O., Graziani, R., Guy, J., Harper, C., Hlozek, R., Howlett, C., Huterer, D., Ju, C., Leget, P. F., Linder, E. V., McDonald, P. Nordin, Nugent, P., Perlmutter, S., Regnault, N., Rigault, M., Shafieloo, A., Slosar, A., Tully, R. B., White, M., & Wood-Vasey, M. Testing Gravity Using Type Ia Supernovae Discovered by Next-Generation Wide-Field Imaging Surveys. Bulletin of the American Astronomical Society, (). Retrieved from https://par.nsf.gov/biblio/10120208.

Kim, Alex, Aldering, G., Antilogus, P., Bahmanyar, A., BenZvi, S., Courtois, H., Davis, T., Ferraro, S., Gontcho, S. Gontcho, Graur, O., Graziani, R., Guy, J., Harper, C., Hlozek, R., Howlett, C., Huterer, D., Ju, C., Leget, P. F., Linder, E. V., McDonald, P. Nordin, Nugent, P., Perlmutter, S., Regnault, N., Rigault, M., Shafieloo, A., Slosar, A., Tully, R. B., White, M., and Wood-Vasey, M. "Testing Gravity Using Type Ia Supernovae Discovered by Next-Generation Wide-Field Imaging Surveys". Bulletin of the American Astronomical Society (). Country unknown/Code not available. https://par.nsf.gov/biblio/10120208.

@article{osti_10120208,
place = {Country unknown/Code not available}, title = {Testing Gravity Using Type Ia Supernovae Discovered by Next-Generation Wide-Field Imaging Surveys}, url = {https://par.nsf.gov/biblio/10120208}, abstractNote = {In the next decade the peculiar velocities of SNe Ia in the local z<0.3 Universe will provide a measure of γ to ±0.01 precision that can definitively distinguish between General Relativity and leading models of alternative gravity.}, journal = {Bulletin of the American Astronomical Society}, author = {Kim, Alex and Aldering, G. and Antilogus, P. and Bahmanyar, A. and BenZvi, S. and Courtois, H. and Davis, T. and Ferraro, S. and Gontcho, S. Gontcho and Graur, O. and Graziani, R. and Guy, J. and Harper, C. and Hlozek, R. and Howlett, C. and Huterer, D. and Ju, C. and Leget, P. F. and Linder, E. V. and McDonald, P. Nordin and Nugent, P. and Perlmutter, S. and Regnault, N. and Rigault, M. and Shafieloo, A. and Slosar, A. and Tully, R. B. and White, M. and Wood-Vasey, M.}, }