Broad-band noises in GX 339-4 during the 2021 outburst observed with Insight-HXMT and NICER

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Fig. 3.

Representative power density spectrum with the Insight-HXMT LE (1–10 keV) data. The dotted lines show the best fit with each component of a multiple-Lorentzian function. The QPO component has been shown while the three broad-band noise components are represented with the L₁, L₂, and L₃.

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