v1.0: Major release that breaks backward compatibility in favor of simplicity and efficiency

What's Changed

• Calibrated MIRI spectra by @kevin218 in #585
• Accounting for light travel time in starry model by @taylorbell57 in #587
• Logging Eureka! version and CRDS pmap by @taylorbell57 in #581
• Default to only compute median frame for 1st batch by @taylorbell57 in #582
• Addresses Errors in Stage 5 using LD coefficients from a file by @kevin218 in #589
• Fixing S3 Pickling Bug, S6 Plotting Bug, and Adding S5 LTT Option by @taylorbell57 in #604
• Assorted HST and JWST enhancements by @kevin218 in #600
• Upgrade binData() --> binData_time() by @hdiamondlowe in #584
• Resolved libGL ImportError by removing opencv-python dependency by @taylorbell57 in #612
• Computing uncertainty on Allan variance plots using mc3 package by @taylorbell57 in #615
• Switching plots from tight_layout to constrained_layout by @taylorbell57 in #613
• Stage 1 Jump Step Parallelization by @taylorbell57 in #611
• Switching from celerite to celerite2 by @taylorbell57 in #614
• Updating instructions for newer exotic-ld versions by @taylorbell57 in #616
• Fix emcee old_chain for white-light curve fit bug by @evamariaa in #622
• Removing 390Hz noise from LRS SLITLESSPRISM data by @taylorbell57 in #556
• Ms no longer used in starry models; batman w parameter no long must be between (0,360); minor tweaks by @taylorbell57 in #625
• Rearranging bright2flux ancillary file look-ups by @taylorbell57 in #623
• Update background subtraction method options to address waterfall effect in lightcurves by @BriDave in #599
• Adding a PyMC3 compatible GP using celerite2 by @taylorbell57 in #624
• Allowing for custom stellar intensity files to be fed into S4 for limb darkening calculations by @erinmmay in #598
• deepcopy instead of assignment to fix median frame curvature bug by @erinmmay in #629
• Correcting typo in Stage 4 flowchart by @taylorbell57 in #630
• Fixing new POET bugs, and old bugs with multwhite fits, masked values in fits, nbin_plot in S5, and S6 model loading by @taylorbell57 in #631
• POET transit and eclipse models, SPAM LD by @kevin218 in #609
• Moving meta.scandir to data.scandir for WFC3 data by @taylorbell57 in #618
• Updating environment.yml files for Apple M2 computers by @taylorbell57 in #637
• Create exception for MC3 failed import by @kevin218 in #641
• Update copyright.rst by @kevin218 in #642
• Upgrading to jwst==1.14.0 and Python>=3.10, and bug fixes by @taylorbell57 in #640
• Adding Hexagonal photometry apertures by @jbrande in #644
• Fixing issue where GP model with masked data failed by @taylorbell57 in #646
• Fix check on time_avg by @kevin218 in #648
• Bug Patch: S6 with similar variable names and S3 undefined aperture_shape by @taylorbell57 in #652
• Removing trailing spaces/tabs from all files by @taylorbell57 in #657
• Flags fully saturated pixel columns as DO_NOT_USE by @gianninapr in #651
• Adding the ability to skip fully-masked data in Stage 5-6 by @taylorbell57 in #656
• Alternate Stage 3 Inputs by @AarynnCarter in #603
• Fixing our readthedocs pages by @taylorbell57 in #671
• Allow setting of matplotlib backend and layout engine by @taylorbell57 in #665
• Adding _ch to channel tag and _pl to planet tag in S5 variable names by @taylorbell57 in #659
• Adding stage-specific MetaClass objects and organizing default ECF values by @taylorbell57 in #632
• Adding an astrophysical model to combine all physical models, adding quasi-Lambertian phase curve by @taylorbell57 in #663
• Bug patches by @taylorbell57 in #677
• Bug fixes by @kevin218 in #678
• NIRCam enhancements from v1 testing by @kevin218 in #682
• Bugfix in HSTRampModel, corrected nchan assignment by @jbrande in #684
• Minor documentation edits to reflect pre-1.0 testing by @jbrande in #681
• Enables custom bad pixel masks (S1), user supplied wavelength files (S4), adds joint white light curve fitting parameters to docs (S5) by @erinmmay in #654
• Two Enhancements from Testing v1.0 by @kevin218 in #693
• Bug patches and docs improvements for v1.0 by @taylorbell57 in #686
• Handling missing scan segments in HST data by @taylorbell57 in #689
• Compute nightside flux with POET by @kevin218 in #698
• Adding a dark mode to the readthedocs page by @taylorbell57 in #700
• Changing Stage 3 masking convention to mask=True where there is bad data by @taylorbell57 in #697
• Enable modeling of starspots with both Fleck and Starry by @erinmmay in #627
• Better documenting multi-channel and multi-planet EPF settings by @taylorbell57 in #701
• Minor bug patches before v1.0 by @taylorbell57 in #705

New Contributors

• @hdiamondlowe made their first contribution in #584
• @BriDave made their first contribution in #599

Full Changelog: v0.10...v1.0