The VIRGO Collaboration

2012

508 citations recorded by the source corpus.

Subfields: Computational Theory and Mathematics, Development, Human-Computer Interaction

View Paper: https://www.semanticscholar.org/paper/e6942f3d1b7e7ad6e2b3fa6c3d36d30a0c790dae

Citations in the corpus

• Inspiral-merger-ringdown multipolar waveforms of nonspinning black-hole binaries using the effective-one-body formalism (2011, background): “[20] are less than 3% when the total mass is 25–99M⊙, which is the mass range used in the LIGO/Virgo search [33].”
• GW231123: A Binary Black Hole Merger with Total Mass 190–265 M⊙ (2025, unknown): “…Collaboration and Virgo Collaboration 2018), DQSEGDB (Fisher et al. 2021), gwdetchar (Urban et al. 2021), hveto (Smith et al. 2011), iDQ (Essick et al. 2020), Omicron (Robinet et al. 2020), and PythonVir-goTools (Virgo Collaboration 2021) software packages and contributing software tools.”
• Tests of general relativity with GWTC-3 (2021, unknown): “[262] LIGO Scientific Collaboration, Virgo Collaboration, KAGRA collaboration, Data release for Tests of General Relativity”
• Search for Gravitational Waves from Low Mass Compact Binary Coalescence in LIGO's Sixth Science Run and Virgo's Science Runs 2 and 3 (2011, unknown): “During early 2010, monolithic suspensions were installed, which involved replacing Virgo’s test masses with new mirrors hung from fused-silica fibers [9].”
• New physics in light of the H0 tension: An alternative view (2019, unknown): “[63] LIGO Scientific, Virgo collaboration, M.”
• Overview of KAGRA: Detector design and construction history (2020, background): “The green and grey shaded regions show the target sensitivities for O3 and O4, respectively [5].”
• GW170817: Measurements of Neutron Star Radii and Equation of State. (2018, background): “—Since September 2015, the Advanced LIGO [1] and Advanced Virgo [2] observatories have opened a window on the gravitational-wave (GW) universe [3,4].”
• GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs (2018, methodology): “Wesample the posterior distribution with stochastic sampling algorithms using an implementation of Markov chain Monte Carlo [239,240] and nested sampling available in the LALI NFERENCE package [241] as part of the LSC Algorithm Library (LAL) [242].”
• Improved reconstruction of a stochastic gravitational wave background with LISA (2020, methodology): “3 We test the model independent reconstruction, using the AET channels, on three well motivated SGWB signals: a simple power law that can mimic an astrophysical GW signal coming from numerous unresolved binary mergers [21, 45] and/or a cosmological signal coming from some inflationary mechanisms [31”
• Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M ⊙ Compact Object and a Neutron Star (2024, methodology): “NumPy (Harris et al. 2020) and SciPy (Virtanen et al. 2020) were used for analyses in the manuscript.”
• Gravitational Radiation Detection with Laser Interferometry (2013, unknown): “(Somiya, 2011), GEO-HF (Affeldt et al. , 2010), Advanced Virgo (The Virgo Collaboration, 2009), and Advanced LIGO (Harry, 2010; LIGO, 2011)).”
• The third generation of gravitational wave observatories and their science reach (2010, background): “For example, at the nominal sensitivity of the advanced detectors, the expected detection rate of the GW signal generated by a binary system of coalescing neutron stars is about a few tens per year [7, 8].”