Raw Data for Fig. 1, Fig. 2, Fig. 3 and Fig. S3 and R code of Moore Modified Rayleigh Test (MMRT) in the manuscript Australian Bogong moths Employ a Light-Dependent Magnetic Compass for Nocturnal Long-Distance Migration by Chen et al. 2025.

The four Excel files respectively show the raw data underpinning Figures 1, 2, 3 and Figures S3 of the following manuscript:Chen, H., Rosberg, L., Dreyer, D., Leberecht, B., Mouritsen, H., Warrant, E.J. (2025). Australian Bogong moths Employ a Light-Dependent Magnetic Compass for Nocturnal Long-Distance Migration.The Excel files corresponding to Figures 1, 2, 3, and S3 contain raw data used to generate the circular plots presented in these figures. The data detail the mean directions, r-values, standard deviations, and p-values of individual Bogong moths tested in a flight arena under various experimental conditions.Figure 1A–C: Laboratory Experiments with Modified Magnetic FieldsRaw data for moths tested in the laboratory under three conditions:<br>Geomagnetic field with azimuth at 0°, panorama-walled arena, randomized stars, full spectrum of stellar illuminationGeomagnetic field with azimuth at 180° , panorama-walled arena, randomized stars, full spectrum of stellar illuminationNulled magnetic field, panorama-walled arena, randomized stars, full spectrum of stellar illuminationEach dataset includes mean direction, r-value, standard deviation, and p-value for moths in each condition.Figure 2A–F: Moth flew under light manipulation experimentsRaw data for moths tested:<br>1. Moth tested in the laboratory under conditions of geomagnetic field (azimuth 0°) , UV-blue light eliminated from the stellar illumination, randomized stars, panorama-walled arena.2.In the field within transparent arenas enclosed by filters transmitting different light wavelengths: λ &gt; 310 nm, λ &gt; 380 nm, and λ &gt; 480 nm.Data include mean direction, r-value, standard deviation, and p-value for each experimental group.Figure 3A–D: Radio Frequency Field ExperimentsRaw data for moths tested in the laboratory under a geomagnetic field (azimuth 0°), randomized starry sky, panorama-walled arena with radio frequency (RF) fields applied or switched off. Each dataset reports mean direction, r-value, standard deviation, and p-value.Figure S3A–C: Sky Stimulation and Light Wavelength TestsRaw data for moths went through ABA test in the laboratory under:<br>Nulled magnetic field, natural starry sky, full-spectrum lightNulled magnetic field, natural starry sky, light with wavelength λ &gt; 480 nmNulled magnetic field, natural starry sky, full-spectrum lightData present mean direction, r-value, standard deviation, and p-value for each condition.<br>The MMRT code is an R script file for the Moore Modified Rayleigh Test (MMRT), developed based on the version authored by Massy et al., 2021. <i>https://doi.org/10.1098/rspb.2021.1805</i>