Fig. 1.
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Ratan radio and Insight-HXMT X-ray observations of Swift J1727.8−1613 in the period MJD 60195−60215. Each point corresponds to an individual GTI. From top to bottom, the panels show, respectively, the Ratan radio fluxes at three frequencies (Ingram et al. 2024), the LE 2 − 10 keV light curve, the HE 28 − 200 keV light curve, and the corresponding hardness ratio. The shaded green region indicates the observations we use in this paper.
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