pypeit/PypeIt: Version 1.13.0

Functionality/Performance Improvements and Additions Allow user control of the local sky subtraction window Implemented a resample algorithm when generating datacubes Sensitivity function masking and output updates Improve speed in ginga visualization of traces and added pypeit_chk_tilts. Note that this script uses an update of the tilts datamodel, so it will not work on older reductions. Fixed a bug in the variance_model calculation for combined images. Datamodel Changes Removed use of the term "master", renamed to calibration frames/files. Default output directory for calibration frames is now Calibrations. Calibration frames renamed from, e.g., MasterArc* to Arc*. Names of associated calibration frames now written to spec2d file headers. Dependency Changes Deprecate support for python 3.8 with PypeIt, allow python 3.11 Make pypeit_show_2dspec (somewhat) backwards compatible. Added the option to disable strict version checking for 1d coadds. Start to deprecate use of os.path in favor of pathlib Script Changes In PypeIt files, the 'calib' column is now always added to the pypeit file, regardless of whether or not you also request the 'comb_id' and 'bkg_id' columns. In PypeIt files, the calibration group numbers can now be anything, as long as there are no more than 63 unique integers. Deprecated pypeit_parse_calib_id script, but improved the .calib file provided by pypeit_setup. The .calib file is now always written, and provides a direct association between input raw files and output calibration files. Discussed in new docs. Added coadd2d setup script Added the possibility to use dither offsets saved in the header of the science frames for coadding 2D spectra (dithoff must be part of the spectrograph metadata). Major quicklook updates; see documentation. ql_multislit.py deprecated. Instrument-specific Updates Updates to reduction parameters for LDT/DeVeny Hotfixes Hotfix to docs to ensure pypeit_loaders api doc is generated Hotfix for KCWI when using alignment (aka ContBars) frames for the astrometric correction.