jnkepler

A differentiable N-body model for multi-planet systems.

jnkepler is a Python package for modeling photometric and radial velocity data of multi-planet systems via N-body integration. Built with JAX, it leverages automatic differentiation for efficient computation of model gradients. This enables seamless integration with gradient-based optimizers and Hamiltonian Monte Carlo methods, including the No-U-Turn Sampler (NUTS) in NumPyro. The package is particularly suited for efficiently sampling from multi-planet posteriors involving a large number of parameters and strong degeneracy.

Subpackages

• jnkepler.jaxttv: A differentialble N-body model for analyzing transit timing variations (TTVs) and radial velocities (RVs) of multi-planet systems.
• jnkepler.nbodytransit: A differentialble photodynamical model. jaxoplanet needs to be installed for using this package.
• jnkepler.nbodyrv: A differentiable RV model taking into account mutual interactions between planets.

See readthedocs for more details.

Installation

pip install jnkepler

CPU performance note

jnkepler is primarily intended for CPU execution, and supports recent JAX releases (tested through 0.11.2). For JAX >=0.4.32, the version-specific settings below substantially improve jnkepler's performance compared with the default runtime settings.

Set XLA_FLAGS before importing JAX, jnkepler, NumPyro, or any other library that imports JAX. In notebooks, restart the kernel first if these libraries have already been imported.

JAX >=0.7: increase the small-while-loop threshold

export XLA_FLAGS="--xla_backend_extra_options=xla_cpu_small_while_loop_byte_threshold=65536"

Or in Python:

import os
os.environ["XLA_FLAGS"] = (
    "--xla_backend_extra_options="
    "xla_cpu_small_while_loop_byte_threshold=65536"
)

import jax
import jnkepler

JAX 0.4.32–0.6.x: use the legacy CPU runtime

export XLA_FLAGS="--xla_cpu_use_thunk_runtime=false"

Or in Python:

import os
os.environ["XLA_FLAGS"] = "--xla_cpu_use_thunk_runtime=false"

import jax
import jnkepler

Use only the configuration for your JAX version. When upgrading to JAX >=0.7, replace --xla_cpu_use_thunk_runtime=false with the threshold setting above.

Performance varies with the JAX version, planetary system, CPU, and workload. JAX/jaxlib 0.6.2 with the legacy runtime provides a well-tested and stable CPU performance reference. If execution is unexpectedly slow after applying the settings above, comparing against this configuration can help identify performance regressions. It can be faster for some workloads, but is not required or universally faster.

See also issue #30 for benchmarks, version comparisons, and technical details.

Note on the transit-finding algorithm (since v0.2.5)

In JaxTTV.get_transit_times_obs, the default transit-time solver is now "fast". This method is optimized for efficient evaluation near the observed transit times, which is typically sufficient for inference because models far from the data have very low likelihood. For models that are substantially offset from the observed transit times, however, the fast method can be less accurate than the Newton-based method. Use transit_time_method="newton" when robust accuracy is needed in that regime.

For this reason, when using the fast method in NUTS, initialize the sampler from a good solution, such as a least-squares optimum as in the example notebooks, rather than from a diffuse or poor initial guess. If multimodality is a major concern, consider a preliminary grid/global search before running NUTS, rather than relying on NUTS alone to discover all modes.

Examples

Start with the step-by-step tutorials: fit transit times, write a NumPyro model, and initialize, tune, and diagnose NUTS. For non-transiting planets, RVs, photodynamics, and pure Keplerian calculations, see Models and extensions.

The examples/ directory contains the notebooks listed below. See the example notebook guide for their scope and requirements.

• minimal example: examples/minimal_example.ipynb

  • computing transit times and RVs
  • plotting TTVs
  • adding a non-transiting planet

• TTV modeling (normal likelihood): examples/kep51_ttv_normal.ipynb

  • posterior sampling with NUTS
  • reproducing the result in Libby-Roberts et al. (2020)

• TTV modeling (Student's t likelihood):

  • examples/v1298tau_ttv_student.ipynb: reproducing the analysis in Livingston et al. (2026)
  • examples/trappist-1_ttv_student.ipynb: reproducing the analysis in Agol et al. (2021)

• Photodynamical modeling: examples/kep51_photodynamics_gp.ipynb

  • SVI optimization & posterior sampling with NUTS
  • noise modeling using Gaussian Process with tinygp

Applications

• TOI-1136: TTV modeling of 6-planets in a resonance chain [paper]
• TOI-2015: Joint TTV & RV modeling of a two-planet system [paper]
• Kepler-51: Four-planet modeling including JWST data [paper] [repository]
• K2-19: TTVs confirm 3:2 resonance [paper]
• TOI-4495: Photodynamical modeling of a pair of near-resonant sub-Neptunes [paper] [repository]
• V1298 Tau: Four low-density planets transiting a young star [paper] [repository]; see also examples/v1298tau_ttv_student.ipynb in this repo
• TOI-2076: TTV modeling of a young, near-resonant planetary system [paper]
• TOI-791: TTV masses of two extremely low-density, Jupiter-sized planets [paper]

References

If you use jnkepler in your research, please consider citing the references below.

• Masuda et al. (2024), A Fourth Planet in the Kepler-51 System Revealed by Transit Timing Variations, AJ 168, 294
• Masuda (2025), jnkepler: Differentiable N-body model for multi-planet systems, Astrophysics Source Code Library, ascl:2505.006.