Notes. Sorted by ω, the table naturally divides into two “camps” from small-scale and large-scale constraints. We exclude ω < 0 due to ghost instability. Note that Avilez & Skordis (2014) and Joudaki et al. (2022) report separate constraints with and without fixing G_m0 = G today; we only show the constraints when it is not fixed, which results in the tightest constraints. Also note that Joudaki et al. (2022) report different bounds ω > {1540, 160, 160, 350} depending on the prior used for ω in the Markov chains. See also Nagata et al. (2004), Ooba et al. (2016, 2017), Ballardini et al. (2016, 2020), Umiltà et al. (2015) for constraints on the gravitational strength and generalized BD models.