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researcher

J. Ellis

44 papers hereh-index 337.1k citations80 works total

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

author position
  • sole author1
  • first author5
  • middle author26
  • last author2

Across the 34 of 44 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE16
  • astro-ph.IM15
  • astro-ph.GA5
  • astro-ph.SR3
  • gr-qc3
  • astro-ph.CO1
same name
  • J. Ellis — 497 papers, h 123
  • J. Ellis — 28 papers, h 15
  • J. Ellis — 18 papers, h 11
  • J. Ellis — 18 papers, h 18
  • J. Ellis — 13 papers, h 26
  • J. Ellis — 9 papers, h 5

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
20122023
most citedRelativistic Shapiro delay measurements of an extremely massive millisecond pulsar

1.6k citations · 7.8k across the 42 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.IM2013★ 228 cited

The stochastic background: scaling laws and time to detection for pulsar timing arrays

Xavier Siemens, Justin Ellis, Fredrick Jenet +1

We derive scaling laws for the signal-to-noise ratio of the optimal cross-correlation statistic, and show that the large power-law increase of the signal-to-noise ratio as a functi…

astro-ph.IM2013★ 61 cited

A Bayesian analysis pipeline for continuous GW sources in the PTA band

Justin Ellis

The direct detection of Gravitational Waves (GWs) by Pulsar Timing Arrays (PTAs) is very likely within the next decade. While the stochastic GW background is a promising candidate…

astro-ph.IM2013★ 37 cited

An Efficient Approximation to the Likelihood for Gravitational Wave Stochastic Background Detection Using Pulsar Timing Data

Justin Ellis, Xavier Siemens, Rutger van Haasteren

Direct detection of gravitational waves by pulsar timing arrays will become feasible over the next few years. In the low frequency regime (10−7 Hz -- 10−9 Hz), we expect…

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