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C. Espinoza

43 papers hereh-index 314.7k citations70 works total

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

author position
  • sole author2
  • first author6
  • middle author21
  • last author3

Across the 32 of 43 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE33
  • astro-ph.SR4
  • physics.space-ph2
  • astro-ph1
  • astro-ph.GA1
  • gr-qc1
same name
  • C. Espinoza — 71 papers, h 22
  • C. Espinoza — 16 papers, h 10
  • C. Espinoza — 6 papers, h 6
  • C. Espinoza — 3 papers, h 3
  • C. Espinoza — 2 papers, h 2
  • C. Espinoza — 2 papers, h 1

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
20082023
most citedThe Second Fermi Large Area Telescope Catalog of Gamma-ray Pulsars

837 citations · 4.5k across the 43 of their papers we have counts for

collaborators
Showing 2012Show all

4 papers · 1 filter

astro-ph.HE2012★ 39 cited

X-ray Observations of High-B Radio Pulsars

S. A. Olausen, W. W. Zhu, J. K. Vogel +6

The study of high-magnetic-field pulsars is important for examining the relationships between radio pulsars, magnetars, and X-ray-isolated neutron stars (XINSs). Here we report on…

astro-ph.HE2012

The spin evolution of young pulsars

Cristobal M. Espinoza

The current understanding of the spin evolution of young pulsars is reviewed through a compilation of braking index measurements. An immediate conclusion is that the spin evolution…

astro-ph.SR2012★ 269 cited

Pulsar glitches: The crust is not enough

N. Andersson, K. Glampedakis, W. C. G. Ho +1

Pulsar glitches are traditionally viewed as a manifestation of vortex dynamics associated with a neutron superfluid reservoir confined to the inner crust of the star. In this Lette…

astro-ph.HE2012★ 22 cited

Fermi-LAT constraints on the Pulsar Wind Nebula nature of HESS J1857+026

R. Rousseau, M. -H. Grondin, A. Van Etten +13

Since its launch, the Fermi satellite has firmly identified 5 pulsar wind nebulae plus a large number of candidates, all powered by young and energetic pulsars. HESS J1857+026 is a…

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