A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations

MLA

Cantiello, Michele, et al. A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations. 2018. EBSCOhost, https://doi.org/10.3847/2041-8213/aaad64.

APA

Cantiello, M., Jensen, J. B., Blakeslee, J. P., Berger, E., Levan, A. J., Tanvir, N. R., Raimondo, G., Brocato, E., Alexander, K. D., Blanchard, P. K., Branchesi, M., Cano, Z., Chornock, R., Covino, S., Cowperthwaite, P. S., D’Avanzo, P., Eftekhari, T., Fong, W., Fruchter, A. S., … Williams, P. K. G. (2018). A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations. https://doi.org/10.3847/2041-8213/aaad64

Chicago

Cantiello, Michele, J. B. Jensen, J. P. Blakeslee, E. Berger, A. J. Levan, N. R. Tanvir, G. Raimondo, et al. 2018. “A Precise Distance to the Host Galaxy of the Binary Neutron Star Merger GW170817 Using Surface Brightness Fluctuations.” doi:10.3847/2041-8213/aaad64.