Image Details

Choose export citation format:

Detection of Giant Pulses from the Transitional Millisecond Pulsar J1227-4853

  • Authors: Saptarshi Sarkar, Jayanta Roy, Bhaswati Bhattacharyya, Paul S. Ray, Sanjay Kudale, Paulo C. C. Freire, Patrick Weltevrede, Matthew Kerr

Saptarshi Sarkar et al 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

Caption: Figure 3.

Three examples of GPs detected during our search. The average profile of PSR J1227−4853 is overlaid in red. The mean flux density during the observation epoch and the flux density of the GP (calculated using the radiometer equation) are also labeled. Panel (A): one of the broadest GPs (S/N = 12.54, width = 143.36 μs). Panel (B): the brightest GP (S/N = 54.98, width = 10.24 μs). Panel (C): one of the narrowest GPs (S/N = 8.57, width = 1.28 μs).

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse