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Aberration/Retardation Analysis of PSR B1451-68’s Profiles from Decimeter to Meter Wavelengths: Emission Heights and Implications for ‘Radius-to-Frequency Mapping’

  • Authors: N. D. Ramesh Bhat, Christopher P. Lee, Joanna M. Rankin

N. D. Ramesh Bhat et al 2026 The Astrophysical Journal 1010 .

  • Provider: AAS Journals

Caption: Figure 1.

Integrated pulse profiles of PSR B1451−68 at multiple observing bands spanning across 72 MHz–8.6 GHz. The profiles have been aligned by eye using the central component as a reference. Observations at lower frequencies (72–231 MHz) are obtained with the MWA, and those at higher frequencies (620–8612 MHz) are archival data from the Parkes/Murriyang (PKS) telescope. The profiles at the lowest and highest frequency bands are shown with 512 phase bins across the period, and those in between with 1024 phase bins.

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