PHOEBE 2.4.17

• Fix support for numpy 2.0. [#982]

PHOEBE 2.4.16

• Fix handling of floating-point precision near the aligned case that used to result in error from libphoebe. [#965]
• Updates to phoebe-server to be compatible with modern browser requirements. [#959]
• Fix support for python 3.13, remove official support for python 3.7. [#968]

PHOEBE 2.4.15

• Fix handling of include_times for RVs with compute_times/phases. [#889]
• GPs on models computed in phase-space will be properly computed based on residuals in time space. [#899]
• Fix units of requivfrac. [#894]
• Fix adopting mask_phases from lc_geometry. [#896]
• Fix population of wavelength array in load function for passbands. [#914]
• Temporarily cap numpy dependency < 2.0. [#930]
• Fix installation of phoebe-server CLI script to launch from UI. [#929]
• Fix passing compute to export_solver with features attached. [#922]
• sigmas_lnf: change handling of noise-nuissance parameter for RVs to no longer depend on the RV amplitude. [#901]
• Remove duplicated phoebe-server code. [#940]
• Fix python 3.12+ support by updating invalid escape sequences. [#948]
• Improved precision in calculation of constraints. [#945]

PHOEBE 2.4.14

• Fix MPI off to not broadcast if never enabled
• Fix warning message in dynesty solver
• Fix multi-compute with enabled/disabled datasets
• Fix error message in compute_ld_coeffs
• Fix segfaults in macos-14
• Now requires C++14-compatible compiler

PHOEBE 2.4.13

• optimization: dynamical RVs avoid unnecessary meshing
• run_checks no longer requires ck2004 atmosphere tables if no datasets use ck2004
• fix treatment of distance for alternate backends (ellc, jktebop)

PHOEBE 2.4.12

• upgrade the build system to pyproject.toml with setuptools as backend and pip as frontend.
• drop the dependency on the obsolete distutils module.
• swap nosetests for pytest.
• small build-related bugfixes throughout the code.

PHOEBE 2.4.11

• fix jktebop backend handling of mass-ratio and eccentricity for RVs.
• bumps version requirements in pip for numpy, scipy, astropy.
• allows sma@star and asini@star to flip to solve for q
• fixes handling of spots on rotating single stars.
• fixes constraint migration for 2.3 -> 2.4

PHOEBE 2.4.10

• fixes implementation of gravitational redshift.
• fixes an unitialized value problem in gradients resulting in nans for effective temperatures.
• minor updates to passband exporting to support upcoming 2.5 release on the passbands server.
• allows setting SelectParameter to an array or tuple (in addition to a list).

PHOEBE 2.4.9

• fixes bug introduced in 2.4.8 and ensures that temperatures are recomputed for spots when the star is rotating asynchronously.

PHOEBE 2.4.7

• fix bug where wavelength arrays that did not include the central wavelength were returning nans for fluxes.