Intensity-resolved and flare-resolved pulse profiles of RX J0520.5–6932 from AstroSat/LAXPC during the 2024 outburst. Left: Dynamic pulse profiles across different intensity intervals. The color map shows normalized pulse shapes, revealing notable structural changes in pulse morphology. The intensity-average pulse profile is overplotted as a dashed line for comparison. Right: Pulse profiles extracted for three distinct flux states identified in Fig. 2: pre-flare, flare, and post-flare intervals. The secondary peak is clearly visible before and after the flare but disappears during the flare, suggesting a change in the emission geometry.