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researcher

V. Kalogera

114 papers hereh-index 7028.1k citations262 works total

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

author position
  • sole author7
  • first author13
  • middle author41
  • last author18

Across the 79 of 114 papers where every author was matched, so the position is known.

fields
  • astro-ph53
  • gr-qc19
  • astro-ph.HE18
  • astro-ph.CO10
  • astro-ph.SR10
  • astro-ph.IM3
same name
  • V. Kalogera — 123 papers, h 87
  • V. Kalogera — 60 papers, h 29
  • V. Kalogera — 52 papers
  • V. Kalogera — 8 papers, h 10
  • V. Kalogera — 5 papers
  • V. Kalogera — 5 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
19952019
most citedGravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

3.6k citations · 19.7k across the 112 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

3 papers · 1 filter

astro-ph.IM2017

Science-Driven Optimization of the LSST Observing Strategy

LSST Science Collaboration, Phil Marshall, Timo Anguita +102

The Large Synoptic Survey Telescope is designed to provide an unprecedented optical imaging dataset that will support investigations of our Solar System, Galaxy and Universe, acros…

astro-ph.IM2013★ 68 cited

Reconstructing the sky location of gravitational-wave detected compact binary systems: methodology for testing and comparison

Trevor Sidery, Ben Aylott, Nelson Christensen +20

The problem of reconstructing the sky position of compact binary coalescences detected via gravitational waves is a central one for future observations with the ground-based networ…

astro-ph.IM2012★ 95 cited

A Parallel Monte Carlo Code for Simulating Collisional N-body Systems

Bharath Pattabiraman, Stefan Umbreit, Wei-Keng Liao +4

We present a new parallel code for computing the dynamical evolution of collisional N-body systems with up to N~10^7 particles. Our code is based on the the Henon Monte Carlo metho…

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