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A VLA Search for the Geminga Pulsar: A Bayesian Limit on a Scintillating Source

  • Authors: M. A. McLaughlin, J. M. Cordes, T. H. Hankins, and D. A. Moffett

McLaughlin et al. 1999 The Astrophysical Journal 512 929.

  • Provider: AAS Journals

Caption: Fig. 1.

Left: The upper seven plots show the 64 bin folded pulse profiles for the individual data sets. The y‐axis has units of millijanskys (one tick mark=10 mJy) and have been normalized to zero mean. The profiles have been shifted so that the first bin of each profile corresponds to the same pulse phase. The bottom plot shows the profiles from all seven individual phase‐referenced scans summed. Right: The upper seven plots show ﹩f_{F}( F) ﹩ for the individual Geminga scans. The lower plot shows ﹩f_{F}( F) ﹩ for the summed profile.

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