Pulsars detected in the GP survey in only Stokes I images

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