M33 UV Extinction paper release

What's Changed

• Add hst wfc3 F225W band by @petiay in #163
• refactor reading in the spectra by @karllark in #161
• removing old multiple spectra plotting by @karllark in #164
• Mocking of continuum and output of individual stis gratings by @karllark in #165
• add all the MIRI imaging bands by @karllark in #166
• add individual gratings by @karllark in #167
• adding in MIRI bandpasses by @karllark in #168
• update plot limits and fix final plot in doc by @karllark in #169
• MW foreground sampling by @karllark in #170
• fixing a plotting bug by @karllark in #172

New Contributors

• @petiay made their first contribution in #163

Full Changelog: v1.4...v1.5

M31 UV Extinction paper release

What's Changed

• Finalize NIRCam spectra support, updates for STIS, etc. by @karllark in #119
• Add WD Hubeny models by @karllark in #123
• Add option to fit sed with G23 only by @Chamani8 in #124
• Add niriss mocking by @karllark in #126
• Use spectral wavelength for relative "band" by @karllark in #125
• finer control of tlusty mocking by @karllark in #130
• Add iue miri lrs and improve iue support by @karllark in #127
• adding conversion functions and tests by @karllark in #133
• Fitting with B3 by @karllark in #128
• Correctly compute reddened photometry by @karllark in #137
• updating to normalize to all the data by @karllark in #136
• Separate stellar param fitting by wavelength region by @Chamani8 in #139
• New model setup/specification by @karllark in #140
• Set weight=0 for obsdata = nans or infs by @Chamani8 in #141
• Usability updates by @karllark in #142
• saving fit parameters as tables in extensions by @karllark in #143
• Add Ly-alpha plots by @karllark in #144
• adding MIRI FND info by @karllark in #146
• Improve mocking by @karllark in #145
• adding Teff,logg uncs and other usability improvements by @karllark in #147
• Allow model data to have more bands than data by @karllark in #149
• can resume from previously saved chain by @karllark in #150
• Mcmc tools by @karllark in #151
• Use Rv bounds for G23 Rv range by @Chamani8 in #152
• adding in pix=3 normalized ralph version by @karllark in #153
• fixing recently introduced bug by @karllark in #154
• adding in initfrac mcmc option by @karllark in #155
• Fix bugs when normalizing by A(55) or E(44-55) by @karllark in #156
• handling case where request equals one of the models by @karllark in #158
• Add WFC3 grism mocking for models by @karllark in #159
• Enhance model plot by @karllark in #160

New Contributors

• @Chamani8 made their first contribution in #124

Full Changelog: v1.3...v1.4

SMC STIS expanded sample paper release

What's Changed

• Updating dust columns to always be tuples with uncertainties by @karllark in #98
• update python and numpy versions in tests by @karllark in #104
• Add rebinning to a constant resolution for spectra and extinction data by @karllark in #100
• enabling labels in extinction plotting by @karllark in #108
• adding commas by @karllark in #110
• fix lnlike by @karllark in #112
• Fully adding in STIS optical, MIRI IFU, and NIRCam spectra by @karllark in #111
• Add plotting for merging stis spectra by @karllark in #114
• including B3 for FM90_B3 fit by @karllark in #113
• black all code by @karllark in #115
• Enhance extinction curve averaging by @karllark in #117
• tox fixes by @karllark in #120
• update A(V) calc to use latest - Decleir et al. (2022) by @karllark in #118

Full Changelog: v1.2...v1.3

NIR SpeX paper release

Release for NIR SpeX paper (Decleir et al. 2022)

What's Changed

• Add wavenum plot option by @karllark in #81
• Save uncertainties by @mdecleir in #80
• Dereddening for standards by @karllark in #66
• Allow models to be saved w/o parameters specified by @karllark in #76
• Plot tweaks by @mdecleir in #82
• Updates to make fitting using a model more robust by @karllark in #83
• STIS LSFs used in mocking of spectra by @karllark in #86
• Fixing minor flux unit issue in docs by @karllark in #88
• Merging changes from diverging versions of the code by @mdecleir in #89
• Add more flexibility to plotting settings by @mdecleir in #90
• Rebinning extinction curves by @mdecleir in #92
• Adding the A(V) unc to E(lam-V) to A(lam)/A(V) calculation by @karllark in #93
• Use flexible output name by @mdecleir in #94
• add parameter check function for model fitting by @karllark in #95
• Plot fitted models in A(lambda)/A(V) by @mdecleir in #96
• Added a keyword for the inverse of R(V) by @mdecleir in #99

Full Changelog: v1.1...v1.2

NIR/MIR enhancements join UV capabilities

NIR/MIR enhancements for two papers on the NIR (Decleir et al. 2021) and MIR (Gordon et al. 2021) Milky Way extinction. This package has now been used to measure UV through NIR/MIR extinction.