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Fig. B.2.
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Left panels show the Stokes I, Q, U, and V spectra (black) of Galactic H I 21 cm emission toward IRAS 02524+2046 (l = 158.0°, b = −33.3°) observed by FAST on 12 August 2023, with orange curves indicating the fitted baseline and standing wave models. The right panels present the spectra after subtracting these components.
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