Searching for dark matter with a spin-based interferometer

Fig. 10, panel (1)

$95\%$ C.L. $\kappa(\omega_a,\phi_x,\phi_y)$ against frequency $f$ (Hz) on a logarithmic axis, with a black dashed line at $\kappa = 1$. The left plot of the printed figure.

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This panel was recovered from the published vector figure. The plot shown here is re-rendered for interactive viewing and analysis. See the paper for the original figure and full scientific context.

License: CC BY 4.0.

Nat. Commun. 16, 4953 (2025) · DOI: 10.1038/s41467-025-60178-6 · arXiv: 2408.02668

Other panels of Fig. 10: (2) (3)

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