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M. E. Gonzalez

7 papers hereh-index 00 citations0 works total

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

author position
  • first author2
  • middle author3

Across the 5 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.HE2
  • astro-ph.GA1
  • astro-ph.IM1
  • astro-ph.SR1
same name
  • M. E. Gonzalez — 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

activity
20062016
most citedThe NANOGrav Nine-year Data Set: Limits on the Isotropic Stochastic Gravitational Wave Background

321 citations · 766 across the 7 of their papers we have counts for

collaborators
Showing 2015Show all

3 papers · 1 filter

astro-ph.IM2015★ 64 cited

The NANOGrav Nine-Year Data Set: Noise Budget for Pulsar Arrival Times on Intraday Timescales

M. T. Lam, J. M. Cordes, S. Chatterjee +21

The use of pulsars as astrophysical clocks for gravitational wave experiments demands the highest possible timing precision. Pulse times of arrival (TOAs) are limited by stochastic…

astro-ph.GA2015★ 321 cited

The NANOGrav Nine-year Data Set: Limits on the Isotropic Stochastic Gravitational Wave Background

Zaven Arzoumanian, Adam Brazier, Sarah Burke-Spolaor +45

We compute upper limits on the nanohertz-frequency isotropic stochastic gravitational wave background (GWB) using the 9-year data release from the North American Nanohertz Observat…

astro-ph.SR2015★ 107 cited

Testing Theories of Gravitation Using 21-Year Timing of Pulsar Binary J1713+0747

W. W. Zhu, I. H. Stairs, P. B. Demorest +17

We report 21-yr timing of one of the most precise pulsars: PSR J1713+0747. Its pulse times of arrival are well modeled by a comprehensive pulsar binary model including its three-di…

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