The 15 columns are the spectra at each listed power. I fitted two spectral peaks in each spectrum with a Lorentzian plus a local linear background. The CSV contains each peak’s fitted intensity, position \(x_c\), and fit uncertainty for every power.

- [Peak intensity vs power](<<BENCH>/raw/commercial/luna-high/bench/t-pl/run-25/peak_intensity_vs_power.png>)
- [Peak position vs power](<<BENCH>/raw/commercial/luna-high/bench/t-pl/run-25/peak_position_vs_power.png>)
- [Lorentzian fit results for every power](<<BENCH>/raw/commercial/luna-high/bench/t-pl/run-25/lorentzian_peak_fits.csv>)

The allometric model was \(y=aP^b\), fitted in log space. For the dominant peak’s intensity, \(b=0.913\pm0.014\) (\(R^2=0.997\)). The weaker peak’s intensity is less consistent with an allometric trend (\(b=0.850\pm0.085\)).

RESULT: b = 0.913 ± 0.014