Pulsars detected in the GP survey in only Stokes I images

The known pulsars detected in the GP survey in only Stokes I images. The mean flux density of the pulsars from the Stokes I image from this work is denoted by SI and the flux density from the Stokes V image is denoted by SV. α refers to the spectral index of the pulsars. Only two of the pulsars, PSRs J1614- 5048 and J1644-4559 have a previously recorded flux density below 300 MHz by Frail et al. (2016). For the 14 remaining pulsars, this is the first low-frequency detections below 300 MHz.