Skip to content

Commit

Permalink
Updated README.md
Browse files Browse the repository at this point in the history
  • Loading branch information
hpparvi committed Feb 3, 2024
1 parent 8b37d30 commit 5d3a3fe
Showing 1 changed file with 0 additions and 30 deletions.
30 changes: 0 additions & 30 deletions README.md
Original file line number Diff line number Diff line change
Expand Up @@ -65,36 +65,6 @@ transmission spectrum light curves.

Read the docs at [pytransit.readthedocs.io](https://pytransit.readthedocs.io).

## News
- **21.10.2020, version 2.5**
- Version 2.5 makes modelling of TTVs trivial with ``pytransit.RoadRunnerModel`` and ``pytransit.QuadraticModel``.
- See the [TTV modelling example notebook](https://github.com/hpparvi/PyTransit/blob/master/notebooks/ttv_model_example.ipynb) for an example of how to evaluate the models for a TTV analysis.

- **14.10.2020, version 2.4**
- Version 2.4 adds ``pytransit.EclipseModel`` to model secondary eclipses with as little hassle as possible.
- See the [secondary eclipse model example notebook](https://github.com/hpparvi/PyTransit/blob/master/notebooks/example_eclipse_model.ipynb)
for an example of how to use it.

- **16.9.2020, Version 2.3**
- Version 2.3 adds ``OblateStarModel`` to model transits over gravity-darkened rapidly rotating star as presented by Barnes (2009).
- See the [oblate star model example notebook](https://github.com/hpparvi/PyTransit/blob/master/notebooks/osmodel_example_1.ipynb)
for an example of usage.

- **13.9.2020, Version 2.2**
- Version 2.2 brings a significant speedup to the evaluation speed of all models. The normalised planet-star distances are
now calculated using a Taylor-series expansion of the planet's (x,y) sky-plane position. The method gives a 2-6 x speedup to the transit
model evaluation and is detailed in Parviainen & Korth (2020, submitted to MNRAS)

- **7.7.2020, Version 2.1**
- Version 2.1 introduces the *RoadRunner* transit model (Parviainen, submitted to MNRAS, 2020), a fast exoplanet transit model
that can use any radially symmetric function to model stellar limb darkening while still being faster to evaluate than
the analytical transit model for quadratic limb darkening.
- See the [basic example notebook](https://github.com/hpparvi/PyTransit/blob/master/notebooks/roadrunner/roadrunner_model_example_1.ipynb),
the [custom limb darkening notebook](https://github.com/hpparvi/PyTransit/blob/master/notebooks/roadrunner/roadrunner_model_example_2.ipynb),
and the [LDTk limb darkening model example notebook](https://github.com/hpparvi/PyTransit/blob/master/notebooks/roadrunner/roadrunner_model_example_3.ipynb).



Installation
------------
### PyPI
Expand Down

0 comments on commit 5d3a3fe

Please sign in to comment.