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A. Gallego Cadavid, Y. Rodriguez, and L. G. Gómez, Generalized SU(2) Proca theory reconstructed and beyond, Phys. Rev. D 102
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Then

L. Heisenberg, R. Kase, and S. Tsujikawa, Beyond generalized Proca theories, Phys. Lett. B 760
Original
2016
Later among the works it cites.
Y. Rodriguez and A. A. Navarro, Scalar and vector Galileons, J. Phys. Conf. Ser. 831
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2017
Later among the works it cites.
K. Yagi and N. Yunes, Approximate Universal Relations for Neutron Stars and Quark Stars, Phys. Rept. 681
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2017
Later among the works it cites.
V. Cardoso, E. Franzin, A. Maselli, P. Pani, and G. Raposo, Testing strong-field gravity with tidal Love numbers, Phys. Rev. D 95
Original
2017
Later among the works it cites.
C. M. Will, Theory and Experiment in Gravitational Physics (Cambridge University Press, 2018)

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2022

I-Love-Q in Ho\v{r}ava-Lifshitz Gravity

Ajith, Siddarth, Yagi, Kent, Yunes, Nicolás

Understand

Ho\v{r}ava-Lifshitz gravity is an alternative theory to general relativity which breaks Lorentz invariance in order to achieve an ultraviolet complete and power-counting renormalizable theory of gravity.

In the low energy limit, Ho\v{r}ava-Lifshitz gravity coincides with a vector-tensor theory known as khronometric gravity.
The deviation of khronometric gravity from general relativity can be parametrized by three coupling constants: $\alpha$, $\beta$, and $\lambda$.
Solar system experiments and gravitational wave observations impose stringent bounds on $\alpha$ and $\beta$, while $\lambda$ is still relatively unconstrained ($\lambda\lesssim 0.01$).