Minor fix

docs/notebooks/Aurora/README.md

@@ -23,34 +23,34 @@ Install the requirements with:
 
 The whole pipeline is:
 
-- [`1. Download and prepare RGB star catalogue.ipynb`](1. Download and prepare RGB stars catalogue.ipynb)
+- `1. Download and prepare RGB star catalogue.ipynb`
   - Download the Andrae R. et al. (2023) catalogue of RGB stars
   - Make the transformation from Galactic to Galactocentric frame
-- [`1a. Plot kinematics.ipynb'](1a. Plot kinematics.ipynb) (optional)
+- `1a. Plot kinematics.ipynb` (optional)
   - Clean the RGB star catalogue of globular clusters (Vasiliev & Baumgardt 2021), SMC and LMC
   - Use AGAMA for potential estimate
   - Make cool plots
-- [`2. Extinctions.ipynb'](2. Extinctions.ipynb)
+- `2. Extinctions.ipynb`
   - Estimate extinctions in G, RP and, BP bands
   - Estimate monochromatic exctinction A_0
   - Fit A_G(A_0) A_BP(A_0) and A_RP(A_0) neglecting the T_eff dependency
-- [`3. Luminosity function.ipynb'](3. Luminosity function.ipynb)
+- `3. Luminosity function.ipynb`
   - Take NGC 6397 globular cluster from Vasiliev & Baumgardt (2021) catalogue
   - Correct the magnitudes for extinctions
   - Extract luminosity function of the RGB stars
-- [`4. Parallax errors.ipynb'](4. Parallax errors.ipynb)
+- `4. Parallax errors.ipynb`
   - Query and count Gaia source (GS) stars on the HEALPix vs G grid
   - Count XP stars on the HEALPix vs G grid
   - Count number of visits and bin parallax errors
   - Fit the parallax error vs G magnitude
-- [`5. Domain.ipynb'](5. Domain.ipynb)
+- `5. Domain.ipynb`
   - Define the computational domain
   - Calculate map from (l, b, D) to (x, y, z)
-- [`6. XP selection function.ipynb'](6. XP selection function.ipynb)
+- `6. XP selection function.ipynb`
   - Query XP statistics over the sky and the G band
   - Estimate subsample selection function
-- [`7. Probability transformation function.ipynb'](7. Probability transformation function.ipynb)
+- `7. Probability transformation function.ipynb`
   - Join together the extinction A_G, the XP selection function, the parallax error model and the luminosity function
   - Estimate the transformation function for PDF, from model to observable
-- [`8. Aurora model.ipynb'](8. Aurora model.ipynb)
+- `8. Aurora model.ipynb`
   One example of the Aurora + GS/E model