activity
20102020
most citedBeating the spin-down limit on gravitational wave emission from the Vela pulsar

167 citations · 647 across the 10 of their papers we have counts for

collaborators

10 papers

physics.optics2020★ 39 cited

Optical frequency combs in quadratically nonlinear resonators

I. Ricciardi, S. Mosca, M. Parisi +7

Optical frequency combs are one of the most remarkable inventions of the last decades. Originally conceived as the spectral counterpart of the train of short pulses emitted by mode…

physics.optics2015★ 1 cited

Direct generation of optical frequency combs in nonlinear cavities

S. Mosca, I. Ricciardi, M. Parisi +4

Quadratic nonlinear processes are currently exploited for frequency comb transfer and extension from the visible and near infrared regions to other spectral ranges where direct com…

physics.optics2014★ 108 cited

Frequency comb generation in quadratic nonlinear media

Iolanda Ricciardi, Simona Mosca, Maria Parisi +4

We experimentally demonstrate and theoretically explain the onset of optical frequency combs in a simple cavity-enhanced second-harmonic-generation system, exploiting second-order…

astro-ph.CO2011★ 110 cited

Directional limits on persistent gravitational waves using LIGO S5 science data

J. Abadie, B. P. Abbott, R. Abbott +712

The gravitational-wave (GW) sky may include nearby pointlike sources as well as astrophysical and cosmological stochastic backgrounds. Since the relative strength and angular distr…

gr-qc2011

Characterization of the Virgo Seismic Environment

The Virgo Collaboration, T. Accadia, F. Acernese +180

The Virgo gravitational wave detector is an interferometer (ITF) with 3km arms located in Pisa, Italy. From July to October 2010, Virgo performed its third science run (VSR3) in co…

astro-ph.HE2011★ 167 cited

Beating the spin-down limit on gravitational wave emission from the Vela pulsar

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Abadie +747

We present direct upper limits on continuous gravitational wave emission from the Vela pulsar using data from the Virgo detector's second science run. These upper limits have been…

gr-qc2011

Search for gravitational waves from binary black hole inspiral, merger and ringdown

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Abadie +721

We present the first modeled search for gravitational waves using the complete binary black hole gravitational waveform from inspiral through the merger and ringdown for binaries w…

astro-ph.HE2010★ 114 cited

Search for Gravitational Wave Bursts from Six Magnetars

J. Abadie, B. P. Abbott, R. Abbott +765

Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized b…

gr-qc2010★ 99 cited

Calibration and sensitivity of the Virgo detector during its second science run

The Virgo Collaboration, T. Accadia, F. Acernese +175

The Virgo detector is a kilometer-length interferometer for gravitational wave detection located near Pisa (Italy). During its second science run (VSR2) in 2009, six months of data…

gr-qc2010★ 9 cited

Virgo calibration and reconstruction of the gravitational wave strain during VSR1

The Virgo collaboration, T. Accadia, F. Acernese +171

Virgo is a kilometer-length interferometer for gravitational waves detection located near Pisa. Its first science run, VSR1, occured from May to October 2007. The aims of the calib…