====================== Simple-PE publications ====================== .. _papers: There are numerous papers which describe the analyses available in the Simple-PE repository. Localization ------------ Codes for localization of sources are based upon the methods developed in the papers: * `Triangulation of gravitational wave sources with a network of detectors <https://doi.org/10.1088/1367-2630/11/12/123006>`_ * `Source localization with an advanced gravitational wave detector network <https://doi.org/10.1088/0264-9381/28/10/105021>`_ * `Localization of transient gravitational wave sources: beyond triangulation <https://doi.org/10.1088/1361-6382/aab675>`_ Results from these analyses are presented in the above papers and also * `Improved source localization with LIGO India <https://doi.org/10 .1088/1742-6596/484/1/012007>`_ * `Localization of binary neutron star mergers with second and third generation gravitational-wave detectors <https://doi.org/10.1103/PhysRevD .97.104064>`_ * `Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo <https://arxiv.org/abs/1304.0670v3>`_ * `Comparison of Gravitational Wave Detector Network Sky Localization Approximations <https://doi.org/10.1103/PhysRevD.89.042004>`_ Parameter Estimation -------------------- The simple-pe analysis is described in the paper * `Simple parameter estimation using observable features of gravitational-wave signals <https://doi.org/10.1103/PhysRevD.108.082006>`_ The method brings together insights developed in earlier papers, including the localization work above and also: * `Degeneracy between mass and spin in black-hole-binary waveforms <https://doi.org/10.1103/PhysRevD.87.024035>`_ * `Constraining the Inclinations of Binary Mergers from Gravitational-wave Observations <https://doi.org/10.3847/1538-4357/ab0b3e>`_ * `Two-harmonic approximation for gravitational waveforms from precessing binaries <https://doi.org/10.1103/PhysRevD.102.024055>`_ * `Measuring gravitational-wave higher-order multipoles <https://doi .org/10.1103/PhysRevD.103.024042>`_