Image Details
Caption: Fig. 5.
The pdfs for phase‐averaged intrinsic source flux density S, given the measured phase‐averaged fluxes (from Fig. 2), are shown for our two test pulsars . For PSR B0329+54, ﹩N_{\mathrm{ISS}\,}=371﹩, and for PSR B0950+08, ﹩N_{\mathrm{ISS}\,}=1.095﹩.
© 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.