Adjusted caption of Lya modeling best-fit parameters table

lya.ipynb

@@ -1544,7 +1544,7 @@
     "    # Add a footer to the table\n",
     "    table = table + '\\enddata\\n' \\\n",
     "        + '\\n' \\\n",
-    "        + '\\\\tablecomments{Best-fit Ly$\\\\alpha$ parameters of the magnification-uncorrected, rest-frame Ly$\\\\alpha$ profiles. From left to right: slit label, best-fit parameters for the blue peak, red peak, and central peak, presented as $\\\\alpha$/$\\mu$/$\\sigma$/$\\omega$, as described in \\S\\,\\\\ref{sssec:methods_lya_fwhm_vsep}. Apart from the stacked spectra, $\\\\alpha$ has units of $10^{-16}$ erg s$^{-1}$ cm$^{-2}$ {\\AA}$^{-1}$, and $\\mu$ and $\\sigma$ have units of km s$^{-1}$.}\\n' \\\n",
+    "        + '\\\\tablecomments{Best-fit Ly$\\\\alpha$ parameters of the magnification-uncorrected, rest-frame Ly$\\\\alpha$ profiles. From left to right: slit label, best-fit parameters for the blueshifted peak, redshifted peak, and central peak, presented as $\\\\alpha$/$\\mu$/$\\sigma$/$\\omega$, as described in \\S\\,\\\\ref{sssec:methods_lya_fwhm_vsep}. Apart from the stacked spectra, $\\\\alpha$ has units of $10^{-16}$ erg s$^{-1}$ cm$^{-2}$ {\\AA}$^{-1}$, and $\\mu$ and $\\sigma$ have units of km s$^{-1}$.}\\n' \\\n",
     "        + '\\n' \\\n",
     "        + '\\\\tablenotetext{a}{The fitted amplitudes of slit M0 are significantly different from the other observations because this observation was taken through cloud cover that prevented an accurate fluxing. See Table \\\\ref{tab:mage_log} for more information about the observing conditions.}\\n' \\\n",
     "        + '\\n' \\\n",

results/tables/lya_best_fit_model_parameters_table.tex

@@ -23,7 +23,7 @@
 M9 & $2.89_{-0.08}^{+0.08}$ / $-100_{-4}^{+5}$ / $88_{-4}^{+5}$ / $-0.001_{-0.004}^{+0.001}$ & $2.42_{-0.05}^{+0.06}$ / $170_{-3}^{+2}$ / $213_{-5}^{+5}$ / $8_{-2}^{+2}$ & $9.6_{-0.2}^{+0.2}$ / $80_{-1}^{+1}$ / $43_{-1}^{+1}$ / $-$ & $0.66_{-0.02}^{+0.02}$ 
 \enddata
 
-\tablecomments{Best-fit Ly$\alpha$ parameters of the magnification-uncorrected, rest-frame Ly$\alpha$ profiles. From left to right: slit label, best-fit parameters for the blue peak, red peak, and central peak, presented as $\alpha$/$\mu$/$\sigma$/$\omega$, as described in \S\,\ref{sssec:methods_lya_fwhm_vsep}. Apart from the stacked spectra, $\alpha$ has units of $10^{-16}$ erg s$^{-1}$ cm$^{-2}$ {\AA}$^{-1}$, and $\mu$ and $\sigma$ have units of km s$^{-1}$.}
+\tablecomments{Best-fit Ly$\alpha$ parameters of the magnification-uncorrected, rest-frame Ly$\alpha$ profiles. From left to right: slit label, best-fit parameters for the blueshifted peak, redshifted peak, and central peak, presented as $\alpha$/$\mu$/$\sigma$/$\omega$, as described in \S\,\ref{sssec:methods_lya_fwhm_vsep}. Apart from the stacked spectra, $\alpha$ has units of $10^{-16}$ erg s$^{-1}$ cm$^{-2}$ {\AA}$^{-1}$, and $\mu$ and $\sigma$ have units of km s$^{-1}$.}
 
 \tablenotetext{a}{The fitted amplitudes of slit M0 are significantly different from the other observations because this observation was taken through cloud cover that prevented an accurate fluxing. See Table \ref{tab:mage_log} for more information about the observing conditions.}