Merge branch 'master' into fit-white-noise

nanograv · Oct 2, 2023 · d20d761 · d20d761
2 parents a754626 + 2c1aa12
commit d20d761
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diff --git a/CHANGELOG-unreleased.md b/CHANGELOG-unreleased.md
@@ -20,6 +20,7 @@ the released changes.
 - Added radial velocity methods for binary models
 - Support for wideband data in `pint.bayesian` (no correlated noise).
 - Added `DMWaveX` model (Fourier representation of DM noise)
+- Piecewise orbital model (`BinaryBTPiecewise`)
 - Optionally return the the log normalization factor of the likelihood function from the `Residuals.calc_chi2()` method.
 - `DownhilWLSFitter` can now estimate white noise parameters and their uncertainties.
 ### Fixed

diff --git a/src/pint/models/__init__.py b/src/pint/models/__init__.py
@@ -20,7 +20,7 @@
 
 # Import all standard model components here
 from pint.models.astrometry import AstrometryEcliptic, AstrometryEquatorial
-from pint.models.binary_bt import BinaryBT
+from pint.models.binary_bt import BinaryBT, BinaryBTPiecewise
 from pint.models.binary_dd import BinaryDD, BinaryDDS, BinaryDDGR
 from pint.models.binary_ddk import BinaryDDK
 from pint.models.binary_ell1 import BinaryELL1, BinaryELL1H, BinaryELL1k