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researcher

J. Rankin

43 papers hereh-index 344.2k citations179 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author2
  • first author8
  • middle author9
  • last author21

Across the 40 of 43 papers where every author was matched, so the position is known.

fields
  • astro-ph18
  • astro-ph.HE16
  • astro-ph.GA4
  • astro-ph.SR4
  • astro-ph.IM1
same name
  • J. Rankin — 104 papers, h 25
  • J. Rankin — 16 papers, h 17
  • J. Rankin — 6 papers, h 2
  • J. Rankin — 4 papers, h 6
  • J. Rankin — 4 papers, h 4
  • J. Rankin — 3 papers, h 13

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19992023
most citedTopology and Polarisation of Subbeams Associated With Pulsar 0943+10's ``Drifting''-Subpulse Emission: I. Analysis of Arecibo 430- and 111-MHz Observations

220 citations · 1.6k across the 43 of their papers we have counts for

collaborators
Showing 2006Show all

3 papers · 1 filter

astro-ph2006★ 17 cited

A model for double notches and bifurcated components in radio profiles of pulsars and magnetars - Evidence for the parallel acceleration maser in pulsar magnetosphere

J. Dyks, B. Rudak, Joanna M. Rankin

Averaged pulse profiles of three nearby pulsars: B1929+10, J0437-4715 and B0950+08 exhibit unusual `double notches'. These W-like looking features consist of two adjacent V-shaped…

astro-ph2006★ 53 cited

The bright spiky emission of pulsar B0656+14

P. Weltevrede, G. A. E. Wright, B. W. Stappers +1

We present a detailed study of the single radio pulses of PSR B0656+14, a pulsar also known to be a strong pulsed source of high-energy emission. Despite the extensive studies at h…

astro-ph2006★ 49 cited

Bistable Profile Illumination in Pulsars B0919+06 & B1859+07

Joanna M. Rankin, Cameron Rodriguez, Geoffrey A. E. Wright

A new single pulse behaviour has been identified in two pulsars, B0919+06 and B1859+07. Normally both starts emit bright subpulses in a region near the trailing edge of heir profil…

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