v1.2.0

What's Changed

• Implements the Doppler imaging model described in https://github.com/rodluger/paparazzi
• Implements transits across oblate stars by @rodluger and @shashankdholakia in #289
• Minor bugfixes

Full Changelog: v1.1.2...v1.2.0

v1.1.3

Patch for #292.

v1.1.2

Fixes issue with the nexsci extension, which previously checked for new planet data on import. Changes to the online database were causing starry to crash when imported. This patch fixes the issue and delays nexsci database checks to the first call of the from_nexsci method (instead of on import).

v1.1.1

• Implement compatibility with aesara, the reincarnation of theano in the upcoming pymc3 release
• Miscellaneous bugfixes

v1.1.0

This version fixes several issues with the code and introduces several new features:

• Implements phase curves and occultations in reflected light
• Fixes several compatibility issues with theano and pymc3
• Removes all dependencies on healpy; now computing spherical harmonic transforms in-house
• Deprecates the add_spot method in favor of a new spot method adapted from the algorithm developed in starry_process
• Makes starry.Map objects picklable
• Allows the show method to be called within a pymc3 model
• Fixes an issue with RVs for multi-planet systems
• Fixes several small bugs, closes several GitHub issues

Minor improvements to the beta version

v0.3.1

Relaxing the kepler tolerance

Version 0.3.0

Final release of the code before publication of the paper in the Astronomical Journal. Minor bug fixes, speed-ups, and improvements.

Version 0.2.2

Release of the code for submission of the paper to the arXiv. Minor bugfixes here and there, speed-ups in the case of pure limb darkening, and improvements to some gradient calculations.

Version 0.2.1

First official release of the code for resubmission of the paper to AJ and submission to the arXiv. This is a major code re-write with a redesigned user interface and faster flux routines, particularly for gradient evaluation.

Beta release

Beta release of the code for submission of the paper to ApJ.