14.2k citations
- University of PisaIT214 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di PisaIT211 papers
- Centre National de la Recherche ScientifiqueFR203 papers
- Sapienza University of RomeIT201 papers
- National Institute for Subatomic PhysicsNL197 papers
- University of UrbinoIT197 papers
- University of GlasgowGB196 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di NapoliIT195 papers
- Max Planck Institute for Gravitational PhysicsDE195 papers
- University of Rome Tor VergataIT194 papers
- University of SalernoIT194 papers
- California Institute of TechnologyUS193 papers
258 papers
Modeling Newtonian noise of acoustic origin in the Virgo gravitational wave detector
Lionel Maurin, François Gautier, Maël Brun +9
Since the first gravitational-wave (GW) detection of September 14th 2015 and with hundreds of gravitational-wave sources identified by the LIGO-Virgo-KAGRA network, GW have produce…
GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1839
GW240925 and GW250207 are two loud gravitational-wave signals from binary black hole coalescences observed with network signal-to-noise ratios and , respectively…
Mechanical Long Baseline Differential Gradiometers as Low Frequency Gravitational Wave Detectors
Enrico Calloni, Annalisa Allocca, Antonino Chiummo +12
We present a new differential mechanical gradiometer for the detection of low-frequency Gravitational Waves. The frequency range is 0.05 to 1 Hz, a frequency gap not covered either…
Searches for Continuous Gravitational Waves from Supernova Remnants in the first part of the LIGO-Virgo-KAGRA Fourth Observing run
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1764
We present results from directed searches for continuous gravitational waves from a sample of 15 nearby supernova remnants, likely hosting young neutron star candidates, using data…
Narrowband searches for continuous gravitational waves from known pulsars in the first two parts of the fourth LIGO--Virgo--KAGRA observing run
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1853
Rotating non-axisymmetric neutron stars (NSs) are promising sources for continuous gravitational waves (CWs). Such CWs can, if detected, inform us about the internal structure and…
Constraints on gravitational waves from the 2024 Vela pulsar glitch
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1774
Among known neutron stars, the Vela pulsar is one of the best targets for gravitational-wave searches. It is also one of the most prolific in terms of glitches, sudden frequency ch…