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A. Renzini

30 papers hereh-index 181.6k citations67 works total

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

author position
  • first author9
  • middle author15
  • last author3

Across the 27 of 30 papers where every author was matched, so the position is known.

fields
  • gr-qc15
  • astro-ph.CO9
  • astro-ph.IM4
  • astro-ph.HE2
same name
  • A. Renzini — 465 papers, h 124
  • A. Renzini — 26 papers
  • A. Renzini — 12 papers
  • A. Renzini — 2 papers
  • A. Renzini — 1 paper

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
20172026
most citedCosmology with the Laser Interferometer Space Antenna

359 citations · 936 across the 29 of their papers we have counts for

collaborators
Showing astro-ph.IMShow all

4 papers · 1 filter

astro-ph.IM2026

Narrow spectral artifact investigation and mitigation in LIGO data from the fourth LIGO-Virgo-KAGRA observing run

E. Goetz, A. Neunzert, A. M. Knee +258

We present efforts to identify, characterize, and mitigate narrow spectral artifacts in LIGO detector data during the fourth LIGO-Virgo-KAGRA observing run. Narrow spectral artifac…

astro-ph.IM2026

Advanced Virgo Plus for O5 -- Design Report Overview

F. Acernese, A. Agapito, D. Agarwal +578

This document presents an overview of the design, implementation, and expected performance of the Advanced Virgo Plus (AdV+) upgrades in view of the O5 observing run. Following the…

astro-ph.IM2024★ 60 cited

LIGO Detector Characterization in the first half of the fourth Observing run

S. Soni, B. K. Berger, D. Davis +232

Progress in gravitational-wave astronomy depends upon having sensitive detectors with good data quality. Since the end of the LIGO-Virgo-KAGRA third Observing run in March 2020, de…

astro-ph.IM2018★ 48 cited

Mapping Incoherent Gravitational Wave Backgrounds

A. I. Renzini, C. R. Contaldi

Given the recent detection of gravitational waves from individual sources it is almost a certainty that some form of background of gravitational waves will be detected in future. T…

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