Temporal evolution of the SRGA J1444 emission during the 2024 outburst. Upper panel: ART-XC light curve during two observations. The time and mean flux of the type I X-ray bursts are shown with the dashed line and thick streak. Bottom left: Flux evolution as observed by MAXI/GSC in the 4–10 keV energy band. Bottom right: X-ray burst recurrence time (in black, left axis) and the mean persistent flux between the bursts in the 4–25 keV energy band $F_{4-25}^{\mathrm{pst}}$ (in red, right axis) as measured by ART-XC.