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Marco Bazzan

Researcher at University of Padua

Publications -  306
Citations -  68260

Marco Bazzan is an academic researcher from University of Padua. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 83, co-authored 284 publications receiving 54421 citations. Previous affiliations of Marco Bazzan include Istituto Nazionale di Fisica Nucleare & Max Planck Society.

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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).
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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.
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A study of the brightest peaks in the diffraction pattern of Fibonacci gratings

TL;DR: In this paper, the diffraction pattern of 1D aperiodic Fibonacci gratings (FGs) is investigated and a set of simple formulae which allow the finding of the positions and the intensities of the strongest diffraction peaks amongst the infinite ones present inside a given reciprocal space interval, chosen according to a user-defined threshold.
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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.
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Multilayers for directed energy accelerated lightsails

TL;DR: In this paper , the authors demonstrate that optimized multilayer structures allow ultralight spacecraft being accelerated by laser radiation pressure up to 20% of the light velocity, and eventually even above, as long as a compromise between efficiency and weight is achieved.