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researcher

A. Zimmerman

47 papers hereh-index 4521.3k citations113 works total

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

author position
  • sole author1
  • first author8
  • middle author24
  • last author13

Across the 46 of 47 papers where every author was matched, so the position is known.

fields
  • gr-qc35
  • astro-ph.IM6
  • astro-ph.HE3
  • astro-ph.CO1
  • astro-ph.GA1
  • stat.ML1
same name
  • A. Zimmerman — 11 papers, h 10
  • A. Zimmerman — 7 papers, h 5
  • A. Zimmerman — 4 papers, h 3
  • A. Zimmerman — 3 papers, h 2
  • A. Zimmerman — 2 papers, h 2
  • A. Zimmerman — 2 papers, h 2

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
20102023
most citedThe SXS Collaboration catalog of binary black hole simulations

451 citations · 3.1k across the 46 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

gr-qc2018★ 115 cited

Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817

Chris Pankow, Katerina Chatziioannou, Eve A. Chase +9

In the coming years gravitational-wave detectors will undergo a series of improvements, with an increase in their detection rate by about an order of magnitude. Routine detections…

astro-ph.CO2018★ 239 cited

A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart

M. Fishbach, R. Gray, I. Magaña Hernandez +316

We perform a statistical standard siren analysis of GW170817. Our analysis does not utilize knowledge of NGC 4993 as the unique host galaxy of the optical counterpart to GW170817.…

gr-qc2018★ 141 cited

Measuring the neutron star tidal deformability with equation-of-state-independent relations and gravitational waves

Katerina Chatziioannou, Carl-Johan Haster, Aaron Zimmerman

Gravitational wave measurements of binary neutron star coalescences offer information about the properties of the extreme matter that comprises the stars. Despite our expectation t…

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