GitHub repository: jdhenshaw/scousepy
Description: ScousePy

ScousePy version 2.1.2: tag_name: v2.1.2
body: Minor bug fix for catching NaNs during automated fitting
ScousePy version 2.1.1: tag_name: v2.1.1
body: Minor bug fixes, mainly revolving around checking spectra fit during stage 2
ScousePy version 2.1.0: tag_name: v2.1.0
body: Key changes:

* addition of flagging for post-processing of the data - see scousespatial.py
* minor tweaks to methodology including using the flagged spectrum output from noisy for the fitting - leads to better, more accurate results
* minor bug fixes, nan catching, mad_std as backstop for rms calculations, lmfit convergence issues
ScousePy version 2.0.0: tag_name: v2.0.0
body: scousepy has undergone some major updates in the latest release, namely:

* Workflow update -- scousepy now uses config files for set up. These control basic parameters for use throughout the workflow
* GUI for S1 - basic functionality is the same. Can also be run without using the config files
* GUI for S2 - added derivative spectroscopy for providing initial guesses
* Former S4 now merged into S3
* Former S5 and S6 now merged
* GUI for S3 - adaptive fit checker and fitting functionality

ScousePy version 1.0.0 : tag_name: v1.0.0
body: ScousePy functionality complete