Fig. 1.

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Light curve of the 2024 outburst of SRGA J1444 observed by the Monitor of All-sky X-ray Image (MAXI, Matsuoka et al. 2009). We converted 2–20 keV observed count rates into 2–10 keV flux values assuming that the spectrum is described by a power law with a photon index Γ = 1.9 absorbed by an equivalent hydrogen column of NH = 2.9 × 1022 cm−2 (Ng et al. 2024). The horizontal bars indicate the time intervals covered by observations of the instruments.
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