Cite
The high-mass end of the red sequence at z ~ 0.55 from SDSS-III/BOSS: completeness, bimodality and luminosity function.
MLA
Montero-Dorta, Antonio D., et al. “The High-Mass End of the Red Sequence at z ~ 0.55 from SDSS-III/BOSS: Completeness, Bimodality and Luminosity Function.” Monthly Notices of the Royal Astronomical Society, vol. 461, no. 2, Sept. 2016, pp. 1131–53. EBSCOhost, https://doi.org/10.1093/mnras/stw1352.
APA
Montero-Dorta, A. D., Bolton, A. S., Brownstein, J. R., Swanson, M., Dawson, K., Prada, F., Eisenstein, D., Maraston, C., Thomas, D., Comparat, J., Chia-Hsun Chuang, McBride, C. K., Favole, G., Hong Guo, Rodríguez-Torres, S., & Schneider, D. P. (2016). The high-mass end of the red sequence at z ~ 0.55 from SDSS-III/BOSS: completeness, bimodality and luminosity function. Monthly Notices of the Royal Astronomical Society, 461(2), 1131–1153. https://doi.org/10.1093/mnras/stw1352
Chicago
Montero-Dorta, Antonio D., Adam S. Bolton, Joel R. Brownstein, Molly Swanson, Kyle Dawson, Francisco Prada, Daniel Eisenstein, et al. 2016. “The High-Mass End of the Red Sequence at z ~ 0.55 from SDSS-III/BOSS: Completeness, Bimodality and Luminosity Function.” Monthly Notices of the Royal Astronomical Society 461 (2): 1131–53. doi:10.1093/mnras/stw1352.