APA (7th ed.) Citation

Porras-Valverde, A. J., Forbes, J. C., Somerville, R. S., Stevens, A. R. H., Holley-Bockelmann, K., Berlind, A. A., & Genel, S. Why Do Semianalytic Models Predict Higher Scatter in the Stellar Mass–Halo Mass Relation Than Cosmological Hydrodynamic Simulations? IOP Publishing.

Chicago Style (17th ed.) Citation

Porras-Valverde, Antonio J., John C. Forbes, Rachel S. Somerville, Adam R. H. Stevens, Kelly Holley-Bockelmann, Andreas A. Berlind, and Shy Genel. Why Do Semianalytic Models Predict Higher Scatter in the Stellar Mass–Halo Mass Relation Than Cosmological Hydrodynamic Simulations? IOP Publishing.

MLA (9th ed.) Citation

Porras-Valverde, Antonio J., et al. Why Do Semianalytic Models Predict Higher Scatter in the Stellar Mass–Halo Mass Relation Than Cosmological Hydrodynamic Simulations? IOP Publishing.