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researcher

N. Bhat

4 papers here

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

author position
  • middle author4

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

fields
  • astro-ph.SR2
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • N. Bhat — 65 papers, h 57
  • N. Bhat — 6 papers, h 11
  • N. Bhat — 5 papers, h 21
  • N. Bhat — 4 papers, h 30
  • N. Bhat — 3 papers
  • N. Bhat — 2 papers

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

collaborators

4 papers

astro-ph.HE2025

The ONs and OFFs of Pulsar Radio Emission: Characterizing the Nulling Phenomenon

Garvit Grover, N. D. Ramesh Bhat, Samuel J. McSweeney +4

Radio emission from pulsars is known to exhibit a diverse range of emission phenomena, among which nulling, where the emission becomes temporarily undetectable, is an intriguing on…

astro-ph.IM2025

Improving pulsar search efficiency in next-generation pulsar surveys with artificial intelligence

Qiuyang Fu, Mengyao Xue, Weiwei Zhu +12

Pulsar searching with next-generation radio telescopes requires efficiently sifting through millions of candidates generated by search pipelines to identify the most promising ones…

astro-ph.SR2025

Relevance of Murchison Widefield Array Interplanetary Scintillation Observations to Heliospheric Transient Catalogues

A. Waszewski, J. S. Morgan, M. C. M. Cheung +6

We have conducted a comprehensive comparison of interplanetary scintillation (IPS) observations taken by the Murchison Widefield Array (MWA) with several heliospheric transient eve…

astro-ph.SR2025

Latitudinal dependence of the solar wind during periods of high and low activity through interplanetary scintillation

A. Waszewski, J. S. Morgan, R. Ekers +5

We present a study of the solar wind over different periods of the solar cycle, specifically focussing on the minimum between solar cycles 24 and 25, and the active, ascending phas…

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