v0.2.6

Full Changelog: v0.2.5...v0.2.6

v0.2.5

Full Changelog: v0.2.4...v0.2.5

v0.2.3

Full Changelog: v0.2.2...v0.2.3

special v0.1.5

What's Changed

• Typo fix in bibliography by @dfm in #3
• Bug fix in case of instru_idx not provided when instru_res is provided by @VChristiaens
• Recommended version for the exoplanet data challenge - phase 2.

Full Changelog: v0.1.4...v0.1.5

special v0.1.4

What's Changed

• Edits for JOSS review by @dfm in #2
• Updated warning when trying to calculate spectral indices with low spectral resolution spectra by @VChristiaens in f628f3f
• Minor improvements to the Jupyter notebook tutorial (clarifications regarding where to download the notebook, the assumed flux unit convention, etc.) by @VChristiaens in 04a0b95 and 4e2531f

Full Changelog: v0.1.3...v0.1.4

special v0.1.3

What's Changed

• Improved spectrum resampling routine, for faster handling of high-resolution models to be convolved+resampled considering multiple different resolving powers by @VChristiaens in #1

Full Changelog: v0.1.2...v0.1.3

special v0.1.2

• Nested sampling: full compatibility added to ultranest sampler for inference of spectral model parameters
• Improved cropped model spectrum before resampling - too conservative crop led to discarding a large fraction of template spectra in template fit
• Improved behaviour for calculation of spectral indices on low spectral resolution spectra
• Updated tutorial with ultranest example and optimized template fitting
• More accurate documentation
• Added JOSS draft + associated workflow for paper compilation
• Version associated to the JOSS paper.

special v0.1.1

• resample_model: slightly updated behaviour when spectral resolution is provided to convolve the model spectrum - now considers that the input value is the average resolving power over the wavelength range probed by the instrument;
• resample_model: more conservative crop of the model spectrum before resampling - to avoid possible edge effects;
• Minimum version required for exoplanet data challenge - phase 2.

special v0.1.0

• Updated all occurrences of instru_fwhm into instru_res (expected input for IFS data is now the spectral resolution, instead of the spectral FWHM in nm).
• Added the possibility to use the ultranest sampler.

special v0.0.5

• Moved the routine to combine specrtal correlation matrices into spec_corr.py
• Added new spectral indices
• Adapted the name and documentation of spectral indices routines to avoid confusion