Kcwidrp

-Now uses python 3.12, allowing reductions on Apple Silicon CPUs, in addition to Intel and AMD
-Added check_cals.py, which allows users to check whether they have the calibration files needed
before starting a full reduction
-Allows for using input files with arbitrary names (no longer need to use only files as they
were named when they were first written to disk)
-Fixes a bug that prevented two concurrent instances of the pipeline from running at the same time
-Adds additional standard star spectra for use in fluxing

-Adds support for the red arm of KCWI

-Changed headers in mflat and mbias to only store file names, not whole paths
-Enabled -i CLI option
-Fixed bug where bad pixels would cause entire slices to be masked, instead of single pixels
-Added changelog

-Added filter to remove bias frames with expime > 0 (bad focus images)
-Config file adjusted to allow fits files of any name
-Conda env file now explicitly describes channels to be used
-Implemented astroscrappy for ccr, instead of lacosmicx
-Added pipeline and script for running the DRP in real time at Keck
-Changed logging to print more information about what files are being read when
-Change ccdproc source to conda-forge to get latest version
-Integrate TWIFLAT and DOMEFLAT frames into group mode
-Enable recurring events option, allowing unordered files to be processed (sometimes)

-Release