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Releases: flaresimulations/synthesizer

PyPI deployment now active + documentation updates

13 Feb 18:01
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What's Changed

  • Update installation instructions in light of working PyPI deployment by @WillJRoper in #839
  • Added version 3.13 to testing suite by @WillJRoper in #838

Full Changelog: v0.8.4-beta...v0.8.5-beta

v0.8.4-beta

13 Feb 13:05
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v0.8.4-beta Pre-release
Pre-release

Still debugging the deployment but maybe there now.

What's Changed

Full Changelog: v0.8.3-beta...v0.8.4-beta

v0.8.3-beta

12 Feb 20:10
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v0.8.3-beta Pre-release
Pre-release

More deployment testing (this time with a small change associated)

What's Changed

Full Changelog: v0.8.2-beta...v0.8.3-beta

v0.8.2-beta

12 Feb 19:56
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v0.8.2-beta Pre-release
Pre-release

Testing deployment again

Full Changelog: v0.8.1-beta...v0.8.2-beta

v0.8.1-beta

12 Feb 19:24
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v0.8.1-beta Pre-release
Pre-release

We need twine in the workflow to deploy... this might qualify as the smallest change between releases ever!

Transformations and PyPi Deployment

12 Feb 19:09
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Full Changelog: v0.7.0-beta...v0.8.0-beta

v0.7.0-beta (introduced velocity shift + pre EmissionModel change checkpoint)

10 Feb 14:42
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What's Changed

New Contributors

Full Changelog: v0.6.0-beta...v0.7.0-beta

Emission models, optimisations and various bugfixes

02 Oct 09:53
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This tag serves as an intermediate tag including lots of bug fixes and improvements to the spectra generation using EmissionModel templates.

Note, that this tag should be used if you have any scripts that don't use units for all applicable inputs. After this tag, the version on main will require all applicable arguments to be passed with units.

For a full summary of the changes see the changelog below.

What's Changed

New Contributors

Full Changelog: v0.5.0-beta...v0.6.0-beta

Pre-EmissionModel checkpoint

19 Jun 14:21
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This is a checkpoint release. After this the process of getting spectra will be simplified by the introduction of EmissionModels, this will be a large breaking change that will render any non-updated pipelines unusable. To continue running those pipelines, this tag should be used.

Primarily this release introduces shared memory parallelism in spectra generation, updates to line emission, miscellaneous updates to documentation and workflows, and a number of small bug fixes. In addition lots of ground work has been put into the final release at this point with the next releases being smaller in scope and more converged on the final release version.

What's Changed

Full Changelog: v0.4.0-beta...v0.5.0-beta

Imaging improvements, apertures, `Grid` truncation, and development QOL

26 Mar 12:23
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This release includes:

  • Introduction of a PhotometryCollection for manipulating photometry.
  • Complete rewrite of the imaging functionality improving flexibility.
  • Particle based objects can now be masked using spatial apertures.
  • Parametric young populations have been introduced.
  • Filter objects (and collections) now initialise their wavelength arrays smartly and the ability to unify a Grid and FilterCollection has been implemented (allowing unification in both directions depending on the user's focus).
  • Grids can now be truncated to useful wavelength ranges to limit memory usage.
  • Linting and formatting is now done with ruff.
  • Developers can now use a pre-commit hook to ensure their code is formatted correctly.