From ca1d251e32cb681f9852305bf35d15a0b871892e Mon Sep 17 00:00:00 2001 From: Sujay Shankar Date: Wed, 15 May 2024 12:28:50 -0400 Subject: [PATCH] Fix link formatting weirdness --- docs/tutorials/best_fit_for_fixed_template.ipynb | 4 ++-- 1 file changed, 2 insertions(+), 2 deletions(-) diff --git a/docs/tutorials/best_fit_for_fixed_template.ipynb b/docs/tutorials/best_fit_for_fixed_template.ipynb index 2641ad4..108f968 100644 --- a/docs/tutorials/best_fit_for_fixed_template.ipynb +++ b/docs/tutorials/best_fit_for_fixed_template.ipynb @@ -6,7 +6,7 @@ "source": [ "# Finding the best fit rotational broadening and radial velocity\n", "\n", - "[NOTE] For this tutorial, you'll need to have our sibling package [`muler`](https://muler.readthedocs.io/en/latest/) installed, which can be done with `pip install muler`.\n", + "[NOTE] For this tutorial, you'll need to have our sibling package [muler](https://muler.readthedocs.io/en/latest/) installed, which can be done with `pip install muler`.\n", "\n", "A common occurrence in astronomy is when we have a data spectrum and we want to find the best fit $v\\sin(i)$ and $v_r$.\n", "\n", @@ -38,7 +38,7 @@ "\n", "Let's use data of an A0V star from [HPF](https://hpf.psu.edu). \n", "\n", - "You can get free example data from the [`muler_example_data`](https://github.com/OttoStruve/muler_example_data) GitHub repo.\n", + "You can get free example data from the [muler_example_data](https://github.com/OttoStruve/muler_example_data) GitHub repo.\n", "\n", "The example data is preloaded into `gollum`'s repo; it was downloaded from [this link](https://github.com/OttoStruve/muler_example_data/blob/main/HPF/01_A0V_standards/Goldilocks_20210517T054403_v1.0_0060.spectra.fits)." ]