Posterior samples to reproduce plots in 'Impact of sky localization uncertainty on ringdown inference'

This archive contains the datasets associated with the code repository:https://github.com/kallolD/skyRingThe GitHub repository contains the source code and instructions neededto reproduce the analysis. Contained within the .zip file are 5 directories: full-sky - Contains the posteriors for the full-sky run for GW250114 and GW190521 as .npy files. The posteriors for these events with different starting times are arranged into different directories - GW250114-t-shift-posteriors - for GW250114 (221+220) model GW250114-220-t-shift-posteriors - for GW250114 (220) model GW190521-t-shift-posteriors - for GW190521 (330+220) model GW190521-220-t-shift-posteriors - for GW190521 (220) model fixed-sky - Contains the posteriors for the fixed-sky run for GW250114 and GW190521 as .npy files. The posteriors for these events with different starting times are arranged into different directories - GW250114-t-shift-posteriors - for GW250114 (221+220) model GW250114-220-t-shift-posteriors - for GW250114 (220) model GW190521-t-shift-posteriors - for GW190521 (330+220) model GW190521-220-t-shift-posteriors - for GW190521 (220) model informed-sky - Contains the posteriors for the informed-sky run for GW250114 simulations_220_221 - Contains the posteriors for the full-sky and fixed-sky run for a (220)+(221) injection simulations_220_330 - Contains the posteriors for the full-sky and fixed-sky run for a (220)+(330) injection The IMR samples for the two events are also included in the posterior_files directory. The notebook to use these samples to produce corner plots can be found in the examples directory in GitHub repository.