Methods:
The code is mainly based on the formalism described in Carullo et al., arXiv:1902.07527. For signals extending below a pure ringdown emission, it uses the truncated formulation of Isi et al., arXiv:1905.00869 (see also their longer follow-up, arXiv:2107.05609). Additional details on the methodology can be found in the GWTC-2 Testing GR LVK catalog, arXiv:2010.14529.
Additional studies using pyRing:
Impact of noise on overtone detection in GW150914: arXiv:2201.00822;
GWTC-3 Testing GR LVK catalog: arXiv:2112.06861;
GW190521 waveforms consistency and astrophysical implications: arXiv:2112.06856;
Models and constraints of ringdown in the presence of U(1) black hole charges: arXiv:2109.13961;
Constraints on braneworld gravity: arXiv:2106.05558;
Verification of the Bekenstein-Hod bound: arXiv:2103.06167;
Constraints on alternative theories of gravity using the ParSpec formalism: arXiv:2102.05939;
Investigations and observational constraints on the area quantisation hypothesis: arXiv:2011.03816;
GW190521 discovery: arXiv:2009.01075 and physics implications: arXiv:2009.01190;
Spectroscopy of Rotating Black Holes Pierced by Cosmic Strings: arXiv:2002.01695.
Probing the Purely Ingoing Nature of the Black-hole Event Horizon arXiv:1912.07058;
pyRing
:If you use pyRing
in your research, please cite the following papers: arXiv:1902.07527, arXiv:1905.00869, arXiv:2010.14529.
External libraries: