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CHANGELOG.md 7.51 KiB
All notable changes will be documented in this file
Unreleased
Added
- Added PTMCMCSampler
[0.3.4] 2019-01-10
Changes
- Renamed the "basic_tutorial.py" example to "fast_tutorial.py" and created a "standard_15d_cbc_tutorial.py"
- Renamed "prior" to "priors" in bilby.gw.likelihood.GravtitationalWaveTransient for consistency with bilby.core. WARNING: This will break scripts which use marginalization.
- Fixed definition of matched_filter_snr, the interferometer method has become
ifo.inner_product
.
Added
- log-likelihood evaluations for pymultinest
[0.3.3] 2018-11-08
Changes currently on master, but not under a tag.
- Removed unnecessary arguments (
ra
,dec
,geocent_time
,psi
) from source functions and replaced them with**kwargs
where appropriate. - Renamed
PriorSet
toPriorDict
- Renamed
BBHPriorSet
toBBHPriorDict
- Renamed
BNSPriorSet
toBNSPriorDict
- Renamed
CalibrationPriorSet
toCalibrationPriorDict
- Added method to result to get injection recovery credible levels
- Added function to generate a pp-plot from many results to core/result.py
- Fixed a bug which caused
Interferometer.detector_tensor
not to update whenlatitude
,longitude
,xarm_azimuth
,yarm_azimuth
,xarm_tilt
,yarm_tilt
were updated. - Extracted time and frequency series behaviour from
WaveformGenerator
andInterferometerStrainData
and moved it toseries.gw.CoupledTimeAndFrequencySeries
Changes
- Switch the ordering the key-word arguments in
result.read_in_result
to putfilename
first. This allows users to quickly read in results by filename - Result object no longer a child of
dict
. Additionally, the list of attributes and saved attributes is standardised - The above changes effect the saving of posteriors. Users can expect that opening files made in python 2(3) which where written in 3(2) may no longer work. It was felt that the overheads of maintaining cross-version compatibility were too much. Note, working in only python 2 or 3, we do not expect users to encounter issues.
- Intermediate data products of samples, nested_samples are stored in the h5
- Time marginalised GravitationalWaveTransient works with arbitrary time priors.
[0.3.1] 2018-11-06
Changes
- Make BBH/BNS parameter conversion more logical
- Source frame masses/spins included in posterior
- Make filling in posterior with fixed parameters work
- Bug fixes
[0.3] 2018-11-02
Added
- Joint-likelihood added
- PyMC3 works with the GravitationalWaveTransient likelihood
- flake8 syntax checking in CI
- Binary neutron star source model
- Allow units to be included in parameter labels
- Add nested samples to dynesty output
- Add more __repr__ methods
- Add ability to plot max likelihood and draws from the posterior
- Document samplers in more detail
- Added the CPNest sampler
- Adds custom titles to corner plots
- Adds plotting of the prior on 1D marginal distributions of corner plots
- Adds a method to plot time-domain GW data
- Added pipenv as a dependency manager
- Hyperparameter estimation now enables the user to provide the single event evidences
- Add nested samples to nestle output
- Prior and child classes now implement the __eq__ magic method for comparisons
- Added default kwargs for each sampler class
- Added NestedSampler and MCSampler helper classes
- Added sampler_requirements.txt file
- Add AlignedSpin gw prior
- Add units to know prior files
- Add pipenv functionality
- Tests run in custom dockerfiles
Changes
- Fix construct_cbc_derived_parameters
- Autocorrelation calculation moved into parent class
- Fix interpretation of kwargs for dynesty
- PowerSpectralDensity structure modified
- Fixed bug in get_open_data
- Modified how sampling in non-standard parameters is done, the
non_standard_sampling_parameter_keys
kwarg has been removed - .prior files are no longer created. The prior is stored in the result object.
- Removed external_sampler and external_sampler_function attribute from Sampler
- Made conversion of number of livepoint kwargs consistent and streamlined throughout the Nested sampler classes
- Fix label creation in plot_multiple, evidences and repeated plots.
- Changed the way repr works for priors. The repr can now be used to re-instantiate the Prior in most cases
- Users can now choose to overwrite existing result files, rather than creating a .old file.
- Make likelihood values stored in the posterior correct for dynesty and nestle
- pymultinest output now stored in {outdir}/pm_{label}/
Removed
- Removes the "--detectors" command line argument (not a general CLI requirement)
[0.2.2] 2018-09-04
Added
- Add functionality to sample in redshift and reconstruction of source frame masses.
- Add functionality to combine result objects.
- Enable initial values for emcee to be specified.
- Add support for eccentric BBH
Changed
- Specifying detectors by name from the default command line options has been removed.
- The prior on polarisation phase has been reduced to [0, pi].
- More prior distributions added.
- More samplers supported, pymc3
- More core likelihoods, Poisson, Student's-t
- Result print function fixed
- Add snr functions as methods of
Interferometer
- The paths between imports where changed so that calls such as
bilby.WaveformGenerator
no longer work. Instead, we need to usebilby.gw.WaveformGenerator
. This was done to keep things cleaner going forward (when, for example, there may be multiple wfg's). - Samplers reorganised into individual files.
[0.2.1] 2018-07-18
Added
- InterferometerStrainData now handles both time-domain and frequencu-domain data
- Adds documentation on setting data (https://lscsoft.docs.ligo.org/bilby/transient-gw-data.html)
- Checkpointing for
dynesty
: the sampling will be checkpointed every 10 minutes (approximately) and can be resumed. - Add functionality to plot multiple results in a corner plot, see
bilby.core.result.plot_multiple()
. - Likelihood evaluations are now saved along with the posteriors.
Changed
- Changed to using
setuptools
for installation. - Clean up of real data handling: all data is now windowed with a 0.4s roll off (unless set otherwise) and low-pass filtered.
- Add explicit method to create a power spectral density from time-domain data
- Clean up of
PowerSpectralDensity()
- adddsset_from
methods to handle various ways to define the PSD. - Clean up of
detectors.py
: adds anInterferometerStrainData
to handle strain data andInterferometerSet
to handle multiple interferometers. All data setting should primarily be done through theInterferometer.set_strain_data..
methods. - Fix the comments and units of
nfft
andinfft
and general improvement to documentation of data. - Fixed a bug in create_time_series
- Enable marginalisation over calibration uncertainty in Inteferemeter data.
- Fixed the normalisation of the marginalised
GravtitationalWaveTransient
likelihood. - Fixed a bug in the detector response.
[0.2.0] 2018-06-17
First pip
installable version https://pypi.org/project/BILBY/ .
Added
- Reoriganisation of the directory into
bilby.core
andbilby.gw
. - Reading of frame files.
- Major effort to update all docstrings and add some documentation.
- Marginalized likelihoods.
- Examples of searches for gravitational waves from a Supernova and using a sine-Gaussian.
- A
PriorSet
to handle sets of priors and allows reading in from a standardised prior file (see https://lscsoft.docs.ligo.org/bilby/prior.html). - A standardised file for storing detector data.
Removed
- All chainconsumer dependency as this was causing issues.