From 11849296d30fb0ffb97cff805d0e18d0be3ac169 Mon Sep 17 00:00:00 2001 From: Sarah Blunt Date: Mon, 9 Sep 2024 09:55:37 -0700 Subject: [PATCH] typo fix --- paper/paper.md | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/paper/paper.md b/paper/paper.md index b6ed9c56..fb4d4b1f 100644 --- a/paper/paper.md +++ b/paper/paper.md @@ -138,7 +138,7 @@ A full descriptive list of modifications to the code is maintained in our Major new features since v1 include: -1. The functionality to jointly fit the radial velocity (RV) time series for the primary star together and the secondary companion (see Section 3 of @Blunt:2023a). For the primary star, the RV data can either be directly input into orbitize! (as explained in the [Radial Velocity Tutorial](https://orbitize.readthedocs.io/en/latest/tutorials/RV_MCMC_Tutorial.html)) or be fitted separately and then used as priors (as detailed in the [Non-orbitize! Posteriors as Priors Tutorial](https://orbitize.readthedocs.io/en/latest/tutorials/Using_nonOrbitize_Posteriors_as_Priors.html)). +1. The functionality to jointly fit the radial velocity (RV) time series for the primary star together with the secondary companion (see Section 3 of @Blunt:2023a). For the primary star, the RV data can either be directly input into orbitize! (as explained in the [Radial Velocity Tutorial](https://orbitize.readthedocs.io/en/latest/tutorials/RV_MCMC_Tutorial.html)) or be fitted separately and then used as priors (as detailed in the [Non-orbitize! Posteriors as Priors Tutorial](https://orbitize.readthedocs.io/en/latest/tutorials/Using_nonOrbitize_Posteriors_as_Priors.html)). 2. The ability to jointly fit absolute astrometry of the primary star. `orbitize!` can fit the Hipparcos-Gaia catalog of accelerations (@Brandt:2021; see the [HGCA Tutorial](https://orbitize.readthedocs.io/en/latest/tutorials/HGCA_tutorial.html)), as well as Hipparcos intermediate astrometric data and Gaia