Fig. 6.

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Spectroscopic model fitting (red) to the spectra (black) collected using SOAR/Goodman for two objects in our sample. Top panel: ZTF-sdBV1, a typical rm-sdBV spectrum. Bottom panel: ZTF-sdBV12, a spectrum revealing a BLAP atmosphere. Notable hydrogen and helium lines are marked above each panel, in blue, at their rest wavelengths.
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