Relationship between the component width (deg) and $log(\dot{E})$ (erg/s) across eight frequency subbands. Each subband is represented by a different color according to the viridis color map, with corresponding linear regression fits shown as dashed lines. The data reveal a positive correlation, suggesting that pulsars with a higher Ė tend to exhibit wider emission components. The scatter in component widths is more pronounced at higher Ė values, particularly above 10³⁶ erg/s.