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James M. Anderson

4 papers hereh-index 6243 citations6 works total

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

author position
  • middle author2

Across the 2 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA1
  • astro-ph.HE1
  • astro-ph.IM1
  • astro-ph.SR1
same name
  • James M. Anderson — 12 papers, h 24
  • James M. Anderson — 2 papers, h 8

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
20152020
most citedThe impact of Solar wind variability on pulsar timing

55 citations · 104 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2020★ 55 cited

The impact of Solar wind variability on pulsar timing

C. Tiburzi, G. M. Shaifullah, C. G. Bassa +22

High-precision pulsar timing requires accurate corrections for dispersive delays of radio waves, parametrized by the dispersion measure (DM), particularly if these delays are varia…

astro-ph.GA2019★ 49 cited

First detection of frequency-dependent, time-variable dispersion measures

J. Y. Donner, J. P. W. Verbiest, C. Tiburzi +11

Context. High-precision pulsar-timing experiments are affected by temporal variations of the Dispersion Measure (DM), which are related to spatial variations in the interstellar el…

astro-ph.IM2018

Testing the accuracy of the ionospheric Faraday rotation corrections through LOFAR observations of bright northern pulsars

N. K. Porayko, A. Noutsos, C. Tiburzi +13

Faraday rotation of polarized emission from pulsars measured at radio frequencies provides a powerful tool to investigate the interstellar and interplanetary magnetic fields. Howev…

astro-ph.SR2015

LOFAR discovery of a quiet emission mode in PSR B0823+26

C. Sobey, N. J. Young, J. W. T. Hessels +91

PSR B0823+26, a 0.53-s radio pulsar, displays a host of emission phenomena over timescales of seconds to (at least) hours, including nulling, subpulse drifting, and mode-changing.…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.