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researcher

E. Fonseca

112 papers hereh-index 5416.1k citations133 works total

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

author position
  • first author4
  • middle author77

Across the 81 of 112 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE82
  • astro-ph.GA10
  • astro-ph.IM8
  • astro-ph.SR5
  • gr-qc4
  • astro-ph.CO3
same name
  • E. Fonseca — 59 papers, h 17
  • E. Fonseca — 27 papers, h 10
  • E. Fonseca — 4 papers, h 4
  • E. Fonseca — 3 papers, h 10
  • E. Fonseca — 2 papers, h 3
  • E. Fonseca — 2 papers, h 3

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
20102024
most citedRelativistic Shapiro delay measurements of an extremely massive millisecond pulsar

1.6k citations · 18.5k across the 111 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

3 papers · 1 filter

astro-ph.CO2021★ 66 cited

CHIME/FRB Catalog 1 results: statistical cross-correlations with large-scale structure

Masoud Rafiei-Ravandi, Kendrick M. Smith, Dongzi Li +38

The CHIME/FRB Project has recently released its first catalog of fast radio bursts (FRBs), containing 492 unique sources. We present results from angular cross-correlations of CHIM…

astro-ph.CO2021★ 125 cited

Searching For Gravitational Waves From Cosmological Phase Transitions With The NANOGrav 12.5-year dataset

Zaven Arzoumanian, Paul T. Baker, Harsha Blumer +62

We search for a first-order phase transition gravitational wave signal in 45 pulsars from the NANOGrav 12.5 year dataset. We find that the data can be modeled in terms of a strong…

astro-ph.CO2010★ 54 cited

GRB 090417B and its Host Galaxy: A Step Towards an Understanding of Optically-Dark Gamma-Ray Bursts

Stephen T. Holland, Boris Sbarufatti, Rongfeng Shen +10

GRB 090417B was an unusually long burst with a T_90 duration of at least 2130 s and a multi-peaked light curve at energies of 15-150 keV. It was optically dark and has been associa…

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