text tweaks

docs/notebooks/RedClump_GSP-Spec_SF.ipynb

@@ -9,6 +9,7 @@
     "\n",
     "We start with this query, which selects stars whose location in a colour-absolute magnitude diagram (not corrected for extinction) is within 0.4 mag of the fiducial line corresponding to the red clump:\n",
     "\n",
+    "```sql\n",
     "    select * from\n",
     "    ( select ra,dec,l,b,phot_g_mean_mag,phot_bp_mean_mag,phot_rp_mean_mag,\n",
     "    nu_eff_used_in_astrometry, pseudocolour, ecl_lat, astrometric_params_solved,\n",
@@ -20,8 +21,9 @@
     "    where phot_g_mean_mag<14 and parallax>0)\n",
     "    as subquery\n",
     "    where subquery.gabs<(subquery.poly5+0.4) and subquery.gabs>(subquery.poly5-0.4)\n",
+    "```\n",
     "    \n",
-    "We limited the query to G<14 to save time, because we know that later in this analysis we will be working with the stars with the most precise chemical abundances, and we know that none of them are fainter than 14.\n",
+    "We limited the query to $G<14$ to save time, because we know that later in this analysis we will be working with the stars with the most precise chemical abundances, and we know that none of them are fainter than 14.\n",
     "\n",
     "The resulting file `rc14_04-result.fits.gz` (220MB) can be downloaded from Zenodo: https://zenodo.org/records/10628724\n",
     "\n",
@@ -31,7 +33,7 @@
     "\n",
     "https://ui.adsabs.harvard.edu/abs/2021A%26A...649A...4L/abstract\n",
     "\n",
-    "and retain stars within 0.3 mag of the fiducial line. The typical parallax uncertainties in this sample is 0.015 mas. **Given the parallax and error distribution within the sample, the $\\pm$0.3 mag selection is expected to miss less than 0.015% of the red clump stars due to parallax noise.**"
+    "and retain stars within 0.3 mag of the fiducial line. The typical parallax uncertainties in this sample is 0.015 mas. **Given the parallax and error distribution within the sample, the $\\pm0.3$ mag selection is expected to miss less than 0.015% of the red clump stars due to parallax noise.**"
    ]
   },
   {