I treated the 15 power columns as the merged spectra and fit them jointly with a linear baseline per spectrum and a shared Lorentzian center and width. The fitted Lorentzian height scales as \(I=54.19P^{0.694}\), with \(P\) in µW. The position fit is constant at \(x_c=1.61176\) eV, so its allometric exponent is 0.

The fitted center is above the scan’s upper energy limit (1.60570 eV), and the joint spectral fit has \(R^2=0.354\). The data therefore do not resolve an interior peak; the reported Lorentzian heights and allometric exponent are model-dependent.

- [Peak intensity vs power plot](<<BENCH>/raw/commercial/luna-high/bench/t-pl/run-11/peak_intensity_vs_power.png>)
- [Peak position vs power plot](<<BENCH>/raw/commercial/luna-high/bench/t-pl/run-11/peak_position_vs_power.png>)
- [Fitted intensity and position for each power](<<BENCH>/raw/commercial/luna-high/bench/t-pl/run-11/lorentzian_peak_results.csv>)

RESULT: b = 0.694 ± 0.015