Searching for dark matter with a spin-based interferometer

Fig. 3, panel (1)

Histogram of the measured noise, p.d.f. against the normalized combined Fourier amplitude $|A^{K+M}(\omega)/\Delta A^{K+M}(\omega)|$, for the frequency bins between $\omega_E$ and 0.01 Hz. A blue vertical line marks the bin at $\omega_E$, drawn as a downward arrow in the print, and the red dashed line is the local 95% detection threshold.

Files

• Data: data.csv

Provenance

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

All figures of this paper

All papers · About · Statistics · Submit data · API