Cite
The SZ flux-mass (Y–M) relation at low-halo masses: improvements with symbolic regression and strong constraints on baryonic feedback.
MLA
Wadekar, Digvijay, et al. “The SZ Flux-Mass (Y–M) Relation at Low-Halo Masses: Improvements with Symbolic Regression and Strong Constraints on Baryonic Feedback.” Monthly Notices of the Royal Astronomical Society, vol. 522, no. 2, June 2023, pp. 2628–43. EBSCOhost, https://doi.org/10.1093/mnras/stad1128.
APA
Wadekar, D., Thiele, L., Hill, J. C., Pandey, S., Villaescusa-Navarro, F., Spergel, D. N., Cranmer, M., Nagai, D., Anglés-Alcázar, D., Ho, S., & Hernquist, L. (2023). The SZ flux-mass (Y–M) relation at low-halo masses: improvements with symbolic regression and strong constraints on baryonic feedback. Monthly Notices of the Royal Astronomical Society, 522(2), 2628–2643. https://doi.org/10.1093/mnras/stad1128
Chicago
Wadekar, Digvijay, Leander Thiele, J Colin Hill, Shivam Pandey, Francisco Villaescusa-Navarro, David N Spergel, Miles Cranmer, et al. 2023. “The SZ Flux-Mass (Y–M) Relation at Low-Halo Masses: Improvements with Symbolic Regression and Strong Constraints on Baryonic Feedback.” Monthly Notices of the Royal Astronomical Society 522 (2): 2628–43. doi:10.1093/mnras/stad1128.