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.