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R. Flaminio

Researcher at National Institutes of Natural Sciences, Japan

Publications -  540
Citations -  89428

R. Flaminio is an academic researcher from National Institutes of Natural Sciences, Japan. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 103, co-authored 510 publications receiving 71841 citations. Previous affiliations of R. Flaminio include University of Tokyo & University of Savoy.

Papers
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Search for continuous gravitational wave emission from the Milky Way center in O3 LIGO-Virgo data

The Ligo Scientific Collaboration, +1649 more
TL;DR: In this paper , the authors present a directed search for continuous gravitational wave (CW) signals emitted by spinning neutron stars located in the inner parsecs of the Galactic Center (GC).
Proceedings ArticleDOI

A micromechanical resonator to reach the quantum regime

TL;DR: In this article, a new micromechanical resonator for the observation of its quantum ground state (QGS) is presented, which takes advantage from the high intrinsic quality factor of single crystal quartz and is designed to obtain a high resonance frequency as well as a low mass (a few tens of µg).
Posted Content

Constraints on the cosmic expansion history from GWTC-3.

R. Abbott, +1674 more
TL;DR: In this article, the authors used 47 gravitational-wave sources from the Third LIGO-Virgo-KAGRA Gravitational-Wave Transient Catalog (GWTC-3) to estimate the Hubble parameter $H(z), including its current value, the Hubble constant $H_0.
Journal ArticleDOI

All-sky search for continuous gravitational waves from isolated neutron stars in the early O3 LIGO data

Richard J. Abbott, +1570 more
- 15 Oct 2021 - 
TL;DR: In this article, an all-sky search for continuous gravitational waves in the frequency band 20-2000 Hz and with a frequency time derivative in the range of $[-1.0, +0.1]\times10^{-8}$ Hz/s.
Journal ArticleDOI

Testing Virgo burst detection tools on commissioning run data

Fausto Acernese, +121 more
TL;DR: The C5 Virgo commissioning run, completed in December 2004, provided data suitable both in quantity and quality for extended analysis as mentioned in this paper, using tools developed either for gravitational wave burst event detection or data characterization.