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We investigate constraints on early dark energy (EDE) using ACT DR4, SPT-3G 2018, Planck polarization, and restricted Planck temperature data (at $\ell<650$), finding a $3.3\sigma$ preference ($\Delta\chi^2=-16.2$ for 3 additional degrees of freedom) for EDE over $\Lambda$CDM.
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Lloyd Knox and Marius Millea, “Hubble constant hunter’s guide,” Phys. Rev. D 101
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S. S. Wilks, “The Large-Sample Distribution of the Likelihood Ratio for Testing Composite Hypotheses,” Annals Math. Statist. 9
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Andrew Gelman and Donald B. Rubin, “Inference from Iterative Simulation Using Multiple Sequences,” Statist. Sci. 7
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R. E. Smith, J. A. Peacock, A. Jenkins, S. D. M. White, C. S. Frenk, F. R. Pearce, P. A. Thomas, G. Efstathiou, and H. M. P. Couchmann (VIRGO Consortium), “Stable clustering, the halo model and nonlinear cosmological power spectra,” Mon. Not. Roy. Astron. Soc. 341
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