References¶

• 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;

• Citing pyRing:

  If you use pyRing in your research, please cite the following papers: arXiv:1902.07527, arXiv:1905.00869, arXiv:2010.14529.

• External libraries:

  pyRing relies on a number of open-source packages. If you use the software in your publications, please cite the references found at these links:

  • corner

  • cpnest

  • gwpy

  • lalsuite

  • matplotlib

  • numpy

  • scipy

  • pesummary