Fig. 8

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Example of the HotPayne fit for a B-type star (top) and an early A-type star (bottom). The LAMOST spectra are shown in black, and the best-fit HotPayne models are shown in red. The masked telluric bands, the DIB, the interstellar absorption of Na and Ca, and the dichroic region are marked by shaded regions. For the case of early A-type stars, the wavelength windows of hydrogen lines (Balmer and Paschen series) are also masked (see text).
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