This project is mirrored from https://git.ligo.org/lscsoft/bilby.git.
Pull mirroring updated .
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v2.2.27afbc747 · ·
## [2.2.2] 2023-11-29 Version 2.2.2 release of Bilby This is a bugfix release reverting a change from 2.2.1 ### Changes - Revert !1284 (!1306)
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v2.2.141f1f300 · ·
## [2.2.1] 2023-1111 Version 2.2.1 release of Bilby This release is a bugfix release. ### Changes - Ensure inteferometer metadata is not empty (!1281) - Make interrupted pools exit more quickly (!1284) - Fix conditional sampling with DeltaFunction conditions (!1289) - The triangular prior raised an error with numpy (!1294) - Make sure strain data resampling works (!1295) - Dynesty logging (!1296) - A bug with saving lists that contain None (!1301) - Preparatory fix an upcoming change in dynesty (!1302)
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v2.2.0ecc90767 · ·
## [2.2.0] 2023-07-24 Version 2.2.0 release of Bilby This release contains one new feature and drops support for Python 3.8. ### Added - New waveform interface to support the SEOBNRv5 family of waveforms (!1218) - Enable default noise + injection function for non-CBC signals (!1263) - Fallback to result pickle loading to match result writing (!1291) ### Changes - Additional error catching for plotting (!1261, !1271) - Improve plotting options for corner plots (!1270) - Fix bugs in closing the pool for emcee (!1274) - Generalize MPI support (!1278) - Fix a bug with saving hdf5 results when conda isn't present (!1290) ### Deprecated - Drop support for py38 (!1277)
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v2.0.24f9c778f · ·
## [2.0.2] 2023-03-21 Version 2.0.2 release of Bilby This is a bugfix release after the last major update. ### Changes - Fix to bilby-MCMC implementation of prior boundary (!1237) - Fix to time calibration (!1234) - Fix nessai sampling time (!1236)
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v2.0.17e977737 · ·
## [2.0.1] 2023-03-13 Version 2.0.1 release of Bilby This is a bugfix release after the last major update. Users may notice changes in inferred binary neutron star masses after updating to match [lalsuite](https://git.ligo.org/lscsoft/lalsuite/-/merge_requests/1658). ### Changes - Make sure quantities that need to be conserved between dynesty iterations are class-level attributes (!1225). - Fix massive memory usage in post-processing calculation of SNRs (!1227). - Update value for the solar mass (!1229). - Make `scikit-learn` an explicit dependence of `bilby[GW]` (!1230).
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v2.0.063c71cb7 · ·
## [2.0.0] 2023-02-29 Version 2.0.0 release of Bilby This major version release has a significant change to the behaviour of the `dynesty` wrapper. There are also a number of bugfixes and some new features in sampling and GW utilities. ### Added - Add marginalized time reconstruction for the ROQ likelihood (!1196) - Generate the `dynesty` posterior using rejection sampling by default (!1203) - Add optimization for mass ratio prior peaking at equal masses (!1204) - Add option to sample over a number of precomputed calibration curves (!1215) ### Changes - Optimize weight calculation for `MultiBandGravitationalWaveTransient` (!1171) - Add compatibility with pymc 5 (!1191) - A bug fix of the stored prior when using a marginalized likelihood (!1193) - Various bug fixes to improve the reliability of the `RelativeBinningGravitationalWaveTransient` (!1198, !1211) - A hack fix for samplers that are not compatible with `numpy>1.23` (!1194) - Updates to some reference noise curves (!1206, !1207) - Fix the broken time+calibration marginalization (!1201) - Fix a bug when reading GW frame files (!1202) - Fix the normalization of the whitened strain attribute of `Interferometer` (!1205) - Optimize ROQ waveform and calibration calls (!1216) - Add different proposal distribution and MCMC length for `dynesty` (!1187, !1222)
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