From a5aaaa1d5962a63e0cb78f22fcf5774a36dd6fda Mon Sep 17 00:00:00 2001 From: William Thompson Date: Sun, 4 Feb 2024 08:46:25 -0800 Subject: [PATCH] Update index.md --- docs/src/index.md | 12 ++++++------ 1 file changed, 6 insertions(+), 6 deletions(-) diff --git a/docs/src/index.md b/docs/src/index.md index 8361d5bf..17d67dbf 100644 --- a/docs/src/index.md +++ b/docs/src/index.md @@ -22,8 +22,8 @@ You can also use Octofitter from Python using the [Python guide](@ref python). * Model stellar activity with Gaussian processes * Model stellar astrometric accerlation (Gaia-Hipparcos proper motion anomaly) * "De-orbiting": combine a sequence of images with orbital motion to detect planets -* Sample directly from images and interferometric visibilities -* experimental support for transit data based on Transits.jl +* Sample directly from images or interferometric visibilities +* Experimental support for transit data based on Transits.jl You can freely combine any of the above data types. Any and all combinations work together. @@ -72,12 +72,12 @@ journal = {The Astronomical Journal}, * Please cite the HMC sampler backend if you use `octofit`: [Xu et al 2020](http://proceedings.mlr.press/v118/xu20a.html) * Please cite the [Pigeons paper](https://arxiv.org/abs/2308.09769) if you use `octofit_pigeons`. * If you use Hipparcos-GAIA proper motion anomaly, please cite [Brandt 2021](https://ui.adsabs.harvard.edu/abs/2021ApJS..254...42B) -* If you use example data in one of the tutorials, please cite the sources listed [Brandt 2021](https://ui.adsabs.harvard.edu/abs/2021ApJS..254...42B) -* If you use one of the included functions for automatically retreiving data from a public dataset, eg HARPS RVBank, please cite the source as appropriate. +* If you use example data in one of the tutorials, please cite the sources listed +* If you use one of the included functions for automatically retreiving data from a public dataset, eg HARPS RVBank, please cite the source as appropriate (it will be displyed in the terminal) * If you adopt the O'Neil et al. 2019 observable based priors, please cite [O'Neil et al. 2019](https://ui.adsabs.harvard.edu/abs/2019AJ....158....4O). * If you use RV phase folded plot, please consider citing Makie.jl [Danisch & Krumbiegel, (2021).](https://doi.org/10.21105/joss.03349) * If you use TemporalGPs.jl to accelerate Gaussian processes modelling of stellar activity, please consider citing [Tebbutt et al 2021](https://proceedings.mlr.press/v161/tebbutt21a.html) -* If you use the pairplot functionality, please cite: +* If you use the pairplot/cornerplot functionality, please cite: ``` @misc{Thompson2023, author = {William Thompson}, @@ -89,4 +89,4 @@ journal = {The Astronomical Journal}, ## Ready? -Ready to get started? Follow our [installation guide](@ref install) and then follow our [first tutorial](@ref fit-astrometry). \ No newline at end of file +Ready to get started? Follow our [installation guide](@ref install) and then follow our [first tutorial](@ref fit-astrometry).