All notable changes to this project will be documented in this file.
- Support for NIRSpec/BOTS observations.
- Functions to refine SOSS timestamps for limb asymmetry studies.
- Light curve fitting with exoUPRF.
- Updates to documentation.
- NIRSpec/G395H reduction tutorial.
- Misc. bug fixes.
- Light curve plotting routines
- juliet dependencies.
- Light curve fitting tutorial.
- Package name changed to exoTEDRF.
- Allow the trace mask width to be specified directly during 1/f correction.
- More support for SUBSTRIP96, particularly in plotting routines.
- Add possibility for flux offset in background correction.
- Best-fitting models are now automatically saved in Stage 4.
- Patch of ATOCA implementation to circumvent occasional error in estimation of wavelength grid.
- supreme-SPOON end-of-life notices.
- Misc. bug fixes.
- Trace masking functionality in TracingStep.
- Fixed implementation of STScI up-the-ramp JumpStep which would not run consistently.
- Made it easier to select stellar models to use for limb-darkening calculation in Stage 4.
- Compatibility with v1.12.5 of the STScI jwst package.
- Variety of utility functions to supplement pipeline functionalities.
- Further improvements in bad pixel correction.
- Updated intrapixel box extraction algorithm.
- Optimization of box extraction width.
- Multiple new 1/f corrections, including chromatic and windowed methods.
- Dark current subtraction step in Stage 1.
- Re-addition of reference pixel correction in Stage 1.
- Some improvements to diagnostic plotting.
- Automated differential background scaling.
- Misc. bug fixes.
- Useless GroupScaleStep.
- Several unneeded functions.
- Best fitting transit models are saved by default.
- Limb-darkening coefficients are automatically calculated at desired binning during light curve fitting.
- Streamline process for fitting (free or prior) or fixing LD coefficients during fits.
- Incorporate PASTASOSS to calculate SOSS wavelength solution based on pupil wheel position.
- Option to specify background estimation region.
- Improvements to bad pixel interpolation.
- extra_functions.py for potentially helpful functions not directly used by the pipeline.
- Misc. bug fixes.
- Stability calculations via the cross-correlation method.
- Streamline installation process.
- Swap order of FlatFieldStep and BackgroundStep, which were somehow backwards.
- Corrected calculation of errors in transit/eclipse fitting.
- Misc. bug fixes.
- RefPixStep. Functionality is redundant.
- Buggy automatic stellar parameter searching.
- Support for eclipse fitting.
- Misc. bug fixes.
- Compatibility with jwst v1.8.5.
- Major updates in nearly every step for speed and self-consistency.
- Vastly simplified ATOCA extraction.
- Added plotting capabilities to most steps.
- Added PCA method for assessing trace stability.
- Automatic detection and masking of Order 0 contaminants if an F277W filter exposure is available.
- New box extraction routine as jwst Extract1dStep has removed this functionality.
- Refinement of wavelength solution.
- When running pipeline via script, a copy of the config file will now be saved in the output directory.
- Misc. bug fixes.
- LightCurveEstimateStep. Functionality now added to TracingStep.
- Large wrapper around ATOCA extraction is removed.
- SOSSSolverStep.
- LightCurveStep. Functionality now added to Extract1dStep
- Various now outdated utility functions.
- Preparation for first release.
- New fancy printing.
- Misc. bug fixes.
- Correction of bug pointing to throughputs for wrong order when calculating LD coefficients.
- Switch default stellar models to 3D grid for LD calculation.
- Simplify LD coefficient calculation.
- Misc. bug fixes.
- Unnecessary functionality to calculate LD coefficients on grid of stellar models to derive errors.
- Add time-domain jump detection for ngroup=2 observations.
- Allow for integration-level correction of 1/f noise.
- Paralellization of stability parameter calculations.
- Allow for piecewise subtraction of background.
- Updated run_DMS script to accept yaml config file.
- TracingStep can now calculate changes in x and y position of the trace as well as the FWHM.
- BackgroundStep has been moved to Stage 2.
- Background is re-added after 1/f noise correction during Stage 1 such that it is properly treated by the non-linearity correction.
- Speed improvements for 1/f and hot pixel corrections.
- stage4.py: code including routines for light curve binning and parallelized fitting using ray and juliet (transit only currently).
- fit_lightcurves.py: script to fit spectrophotometric light curves.
- fit_lightcurves.yaml: config file for fit_lightcurves.py.
- Redundant plotting routines.
- Multiple depreciated utility functions.
- Base prerelease code for Stages 1 - 3.