Changelog

pyirf 0.11.1.dev48+ga80291a (2024-11-15)

API Changes

Bug Fixes

New Features

Maintenance

Refactoring and Optimization

pyirf v0.12.0 (2024-11-15)

API Changes

  • Make it possible to pass multiple quantiles to pyirf.benchmarks.angular_resolution, calculating all of them.

    The column name(s) in the output now include(s) the percentage value of the calculated quantile, e.g. angular_resolution_68. [#290]

Bug Fixes

  • Fix pyirf.irfs.energy_dispersion.energy_dispersion_to_migration. This function was not adapted to the now correct normalization of the energy dispersion matrix, resulting in wrong results on the now correct matrices. [#273]

New Features

  • Add 3D effective area functions for lon/lat and theta/phi coordinates and some necessary utiliy functions. [#281]

Maintenance

  • Make pyirf compatible with numpy 2.0.

pyirf v0.11.0 (2024-05-14)

Bug Fixes

  • Fix pyirf.benchmarks.energy_bias_resolution_from_energy_dispersion. This function was not adapted to the now correct normalization of the energy dispersion matrix, resulting in wrong results on the now correct matrices. [#268]

New Features

  • Adds an extrapolator for parametrized compontents utilizing blending over visible edges, resulting in a smooth extrapolation compared to the NearestSimplexExtrapolator. [#253]

  • Ignore warnings about invalid floating point operations when calculating n_signal and n_signal_weigthed because the relative sensitivty is frequently NaN. [#264]

  • Add basic combinatoric fill-value handling for RAD_MAX estimation. [#282]

Maintenance

  • Clarified some documentation. [#266]

  • Add support for astropy 6.0. [#271]

  • Added filling of CREF keyword (IRF axis order) in the output files [#275]

Refactoring and Optimization

pyirf v0.10.1 (2023-09-15)

Bug Fixes

  • Fix PowerLaw.from_simulation for the new format of SimulatedEventsInformation, it was broken since splitting the single viewcone into viewcone_min and viewcone_max. [#258]

Pyirf v0.10.0 (2023-08-23)

This release contains an important bug fix for the energy dispersion computation, it was wrongly normalized before.

API Changes

  • In prior versions of pyirf, the energy dispersion matrix was normalized to a sum of 1 over the migration axis. This is wrong, the correct normalization is to an integral of 1, which is fixed now.

    The internal API of the interpolation functions had to be adapted to take in additional keywords, mainly the bin edges and the kind of normalization (standard or solid angle cone sections). [#250]

  • Replace single viewcone argument of SimulationInfo with viewcone_min and viewcone_max, e.g. to correctly enable ring wobble simulations. [#239]

Bug Fixes

  • See above on the energy dispersion change.

New Features

  • Add option to specify which containment to use for angular resolution. [#234]

pyirf 0.9.0 (2023-07-19)

API Changes

  • Change the interpolation API to top-level estimator classes that instantiate inter- and extrapolator objects. Drops the interpolate_xyz functions originally used to interpolate a xyz IRF component in favour of a XYZEstimator class. Moves data checks from intepolator to estimator classes.

    Direct usage of interpolator objects is now discuraged, use estimator objects instead. [#228]

Bug Fixes

  • Correctly fill n_events in angular_resolution, was always 0 before. [#231]

  • Remove condition that relative sensitivity must be > 1. This condition was added by error and resulted in returning nan if the flux needed to fulfill the conditions is larger than the reference flux used to weight the events. [#241]

New Features

  • Add moment morphing as second interpolation method able to handle discretized PDF components of IRFs. [#229]

  • Add a base structure for extrapolators similar to the interpolation case as well as a first extrapolator for parametrized components, extrapolating from the nearest simplex in one or two dimensions. [#236]

  • Add an extrapolator for discretized PDF components, extrapolating from the nearest simplex in one or two dimensions utilizing the same approach moment morphing interpolation uses. [#237]

  • Add a DiscretePDFNearestNeighborSearcher and a ParametrizedNearestNeighborSearcher to support nearest neighbor approaches as alternatives to inter-/ and extrapolation [#232]

Maintenance

  • Drop python 3.8 support in accordance with NEP 29 [#243]

pyirf 0.8.1 (2023-03-16)

New Features

  • Migrating the interpolation methods from pyirf.interpolation to interpolator objects, allowing for later inheritance for new algorithms and reusability. [#210]

Maintenance

  • Add and enable towncrier in CI. [#207]

  • Add a fixture containing three IRFs from the prod5 IRF data-release for unit testing. Specifically the fixture contains the contents of:

    • Prod5-North-20deg-AverageAz-4LSTs.180000s-v0.1.fits.gz.

    • Prod5-North-40deg-AverageAz-4LSTs.180000s-v0.1.fits.gz

    • Prod5-North-60deg-AverageAz-4LSTs.180000s-v0.1.fits.gz

    The user has to download these irfs to irfs/ using download_irfs.py, github’s CI does so automatically and caches them for convenience. [#211]

Older releases

For releases between v0.4.1 and v0.8.1, please refer to the GitHub releases page.

0.4.1 (2021-03-22)

Summary

  • Released March 22nd, 2021

  • 1 Contributors

Contributors

  • Maximilian Nöthe

Merged Pull Requests

  • #135 Add functions to convert pyirf results to the corresponding gammapy classes

  • #137 Add example notebook for calculating point-lile IRFs from the FACT open data

0.4.0 (2020-11-09)

Summary

  • Released November 11th, 2020

  • 2 Contributors

Contributors

In order of number of commits:

  • Maximilian Nöthe

  • Michele Peresano

Description

This release is an important update that introduces three changes in the cut optimization, background estimation and sensitivity calculation.

Together, these changes bring the calculated sensitivities much closer to the ones calculated by EventDisplay.

  • Scale the relative flux calculated to reach the target sensitivity up if the requirements on the minimum number of signal events are not met. Essentially, instead of always calculating the flux that yields target_sensitivity and then checking if the two other conditions are met, we increase the required flux to meet the other requirements. This can result in new sensitivities where before pyirf would report no sensitivities, and report better sensitivities everywhere where the event number conditions where not met before at the target significance. The best sensitivity now is the lowest flux that just barely satisfies all requirements (so is at the minimum requirement of one of the three).

  • Differentiate between reco_source_fov_offset and true_source_fov_offset, using the former for background rates and the latter for everything concerning signal events.

  • Change optimize_gh_cut to do the optimization in terms of efficiency and limit this efficiency to max. 80 % in the EventDisplay comparison.

Smaller improvements also include:

  • It is now possible to include a particle_type column in the event lists, which will result in additionally reporting all event counts also per particle_type. E.g. if particle_type is included in the background table consisting of both electrons and protons, estimate_background will not only report n_background(_weighted) but also n_electron(_weighted) and n_proton(_weighted)

  • relative_sensitivity now supports vectorized application and broadcasting of inputs, as previously wrongly advertized in the docstring.

Merged Pull Requests

Feature changes

  • #110 Optimize cuts in efficiency steps with maximum efficiency of 80% for EventDisplay comparison

  • #104 Scale flux for conditions, differenatiate reco and true source_fov_offset

  • #108 Add counts / weighted counts per particle type

  • #107 Small update to installation instructions

  • #106 Use vectorize for relative_sensitivity

Project maintenance

  • #102 Require astropy >= 4.0.2

  • #100 Fix deploy condition in travis yml

0.3.0 (2020-10-05)

Summary

  • Released October 5th, 2020

  • 5 Contributors

Contributors

In order of number of commits:

  • Maximilian Nöthe

  • Michele Peresano

  • Noah Biederbeck

  • Lukas Nickel

  • Gaia Verna

Description

This release is the result of the IRF sprint week in September 2020. Many bug fixes and improvements were made to the code.

As the target for the sprint week was to reproduce the approach of EventDisplay and the resulting IRFs, one scheme of cut optimization is implemented. The examples/calculate_eventdisplay_irfs.py should follow the approach of EventDisplay closely and shows what is currently implemented in pyirf. In the central and upper energy range, pyirf now reproduces the EventDisplay sensitivity exactly, the lower energy bins still show some disagreement. The cut optimization seems not yet to be the same as EventDisplay’s and will be further investigated. This example could be used as a starting point if you also want to do cut optimization for best sensitivity.

At least one version of each IRF is now implemented and can be stored in the GADF format. Computation of full-enclosure IRFs should be possible but is of now not yet tested on a reference dataset.

Merged Pull Requests

  • #97 Store correct signal amount, store information on which checks failed for sensitivity bins (Maximilian Nöthe)

  • #96 Add integration test (Michele Peresano)

  • #98 Remove option point_like for psf (Maximilian Nöthe)

  • #95 Cut updates (Maximilian Nöthe)

  • #91 Fix conditions to take relative sensitivity into account, fixes #90 (Maximilian Nöthe)

  • #89 Fix brentq returning the lower bound of 0 for flat li ma function (Maximilian Nöthe)

  • #85 Improve comparison to EventDisplay (Maximilian Nöthe)

  • #75 Add a function to check a table for required cols / units (Maximilian Nöthe)

  • #86 Fix Li & Ma significance for n_off = 0 (Maximilian Nöthe)

  • #76 Feature resample histogram (Noah Biederbeck, Lukas Nickel)

  • #79 Fix integration of power law pdf in simulations.py (Gaia Verna)

  • #80 Estimate unique runs taking pointing pos into account (Maximilian Nöthe)

  • #71 Background estimation (Maximilian Nöthe)

  • #78 Change argument order in create_rad_max_hdu (Lukas Nickel)

  • #77 Calculate optimized cut on only the events surviving gh separation (Maximilian Nöthe)

  • #68 Effective area 2d (Maximilian Nöthe)

  • #67 Add method integrating sim. events in FOV bins (Maximilian Nöthe)

  • #63 Verify hdus using ogadf-schema (Maximilian Nöthe)

  • #58 Implement Background2d (Maximilian Nöthe)

  • #52 Add sections about tests, coverage and building docs to docs (Maximilian Nöthe)

  • #46 Add PyPI deploy and metadata (Maximilian Nöthe)

0.2.0 (2020-09-27)

Summary

  • Released September 27th, 2020

  • 4 Contributors

Contributors

In order of number of commits:

  • Maximilian Nöthe

  • Michele Peresano

  • Lukas Nickel

  • Hugo van Kemenade

Description

For this version, pyirf’s API was completely rewritten from scratch, merging code from several projects (pyirf, pyfact, fact-project/irf) to provide a library to compute IACT IRFs and sensitivity and store them in the GADF data format.

The class based API using a configuration file was replaced by a finer grained function based API.

Implemented are point-like IRFs and sensitivity.

This release was the starting point for the IRF sprint week in September 2020, where the refactoring continued.

Merged Pull Requests

  • #36 Start refactoring pyirf (Maximilian Nöthe, Michele Peresano, Lukas Nickel)

  • #35 Cleanup example notebook (Maximilian Nöthe, Michele Peresano, Lukas Nickel)

  • #37 Move to python >= 3.6 (Hugo van Kemenade)

0.1.0 (2020-09-16)

This is a pre-release.

  • Released September 16th, 2020

0.1.0-alpha (2020-05-27)

Summary

This is a pre-release.

  • Released May 27th, 2020

  • 3 contributors

Description

  • Started basic maintenance

  • Started refactoring

  • First tests with CTA-LST data

Contributors

In alphabetical order by last name:

  • Lea Jouvin

  • Michele Peresano

  • Thomas Vuillaume