Pulsars detected in the GP survey in both imaging and beamforming searches.

SI is the mean flux density of the pulsars in Stokes I image from this work, SV is the Stokes V for the pulsars that were detected in Stokes V image in this work and Slit is the low-frequency flux density available in the literature: ’M’ stands for MWA-image detection by Murphy et al.(2017), ’X’ stands for MWA-incoherent beam detection by Xue et al. (2017), ’S’ stands for MWA SMART survey detections by Bhat et al. (2023b) and ’K’ stands for LOFAR detection by Kondratiev et al. (2016). α is the spectral index of the pulsars. α is calculated using the flux densities of the pulsars in MWA Stokes I image (154 MHz) and the RACS Stokes I image (888 MHz).