<html><head><meta name="color-scheme" content="light dark"></head><body><pre style="word-wrap: break-word; white-space: pre-wrap;">\documentclass[journal]{rmaa}


\usepackage{multirow}
\newcommand{\casitiny}{\fontsize{6}{7}\selectfont}


\title{Upper Main Sequence Stars with Anomalous Abundances. The HgMn stars HR 3273, HR 8118, HR 8567 and HR 8937}

\author{C. Saffe, N. N\'u\~nez, and  H. Levato\affil{Instituto de Ciencias Astron\'omicas, de la Tierra y del Espacio (ICATE) \\
and Facultad de Ciencias Exactas, F\'isicas y Naturales \\ Universidad Nacional de San Juan, Argentina}}


\fulladdresses{
\item C. Saffe, N. N\'u\~nez and H. Levato: Instituto de Ciencias Astron\'omicas, de la Tierra y del Espacio, C.C 467, 5400, San Juan, 
Argentina. CS and HL are members of the Carrera del Investigador Cient\'ifico, Consejo Nacional de Investigaciones Cient\'{i}ficas y 
T\'{e}cnicas de la Rep\'{u}blica Argentina (csaffe,~nnunez,~hlevato@icate-conicet.gob.ar).}


\shortauthor{Saffe, N\'u\~nez, \&amp; Levato}

\shorttitle{The HgMn stars HR 3273, HR 8118, HR 8567 and HR 8937}


\listofauthors{C.~Saffe, N.~N\'u\~nez, \&amp; H.~Levato}

\indexauthor{Saffe, C.}
\indexauthor{N\'u\~nez, N.}
\indexauthor{Levato, H.}


\SetYear{2011}
\ReceivedDate{2010 December 13}
\AcceptedDate{2011 April 14}


\abstract{This work is part of our current study for verifying a possible relation between abundances of HgMn stars with stellar parameters, 
rotation and age. We present an analysis of the stars HR 3273, HR 8118, HR 8567 and HR 8937. We used echelle spectra taken with the CASLEO 
2.1~m telescope and ATLAS9 model atmospheres. HeI was underabundant for the HgMn stars. O was slightly underabundant in HR~3273 and HR 8567. 
MgII was underabundant except for HR 8118. SiII was close to solar in HR 8118 and HR 8937, and underabundant in HR 3273 and HR 8567. Fe was 
slightly underabundant in HR 3273 and HR 8567, and slightly overabundant in HR 8118 and HR 8937. The species Sc, Ti, Cr, Mn, Sr, Y and Zr were 
overabundant while Ni was underabundant.\medskip}

\resumen{Este trabajo es parte de un estudio para verificar posibles tendencias de las abundancias en estrellas HgMn con los par\'ametros 
estelares, rotaci\'on y edad. Presentamos un an\'alisis de las estrellas HR 3273, HR 8118, HR 8567 y HR 8937. Utilizamos espectros echelle 
tomados con el telescopio de 2.1~m del CASLEO y modelos de atm\'osferas de ATLAS9. El He result\'o por debajo del valor solar para las 
estrellas HgMn. El O result\'o levemente sobreabundante en HR 3273 y HR 8567. MgII result\'o por debajo excepto para HR 8118. El SiII 
result\'o aproximadamente solar en HR 8118 y HR~8937, y por debajo en HR 3273 y HR~8567. El Fe result\'o levemente sobreabundante en HR 8118 
y HR 8937 y subabundante en HR 3273 y HR 8567. Las especies Sc, Ti, Cr, Mn, Sr, Y y Zr resultaron sobreabundantes mientras que el Ni result\'o 
estar por debajo del valor solar.\smallskip}


\addkeyword{stars: chemically peculiar} 
\addkeyword{stars: individual (HR 3273, HR 8118, HR~8567, HR 8937)}


\begin{document}

\maketitle

\section{Introduction} 

The mercury-manganese (HgMn) stars belong to a group of chemically peculiar (CP) stars observed in the upper main sequence. Their hydrogen spectral 
types are usually B7-B9 with effective temperatures between 10000~K and 15000~K. HgMn stars show typically intensified lines of Hg (up to $\sim$5~dex), 
Mn (up to $\sim$3~dex) and a deficiency of He. This group shows an unusually high proportion of multiple systems: more than two thirds of them are 
spectroscopic binaries (SBs), many of which are double-lined systems \citep[e.g., ][]{hubrig-mathys95}. They are usually slow rotators (e.g., Abt, 
Chaffee, \&amp; Suffolk 1972) and they show no evidence of large-scale organized magnetic fields \citep[e.g., ][]{auriere07,auriere10,maka11}.


%%%%% TABLA 1

\begin{table*}[!t]
\centering
\setlength{\tabnotewidth}{0.9\textwidth}
\tablecols{6}
\setlength{\tabcolsep}{1.2\tabcolsep}
\caption{Observational Data for the sample of HgMn stars}
\label{obsdata}
\small
\begin{tabular}{lccccc}
\toprule
\multicolumn{1}{c}{Parameter}  &amp; HR 3273 &amp; HR 8118 &amp; HR 8567 &amp; HR 8937 &amp; References \\
\midrule
$B-V$     &amp; $-$0.08~  &amp; $-$0.08~   &amp; $-$0.04~  &amp; $-$0.10~ &amp; R1,R6,R8  \\
$U-B$     &amp; $-$0.38~  &amp; $-$0.32~   &amp; $-$0.37~  &amp; $-$0.37~ &amp; R1,R6  \\
$V$       &amp;   ~6.42~  &amp;   ~6.76~   &amp;   ~6.36~  &amp;   ~4.37~ &amp; R1,R6,R9    \\
$b-y$     &amp; $-$0.020  &amp; $-$0.028   &amp; $-$0.018  &amp; $-$0.046 &amp; R2   \\
$m_1$     &amp;   ~0.090  &amp;   ~0.117   &amp;   ~0.101  &amp;   ~0.125 &amp; R2   \\
$c_1$     &amp;   ~0.710  &amp;   ~0.801   &amp;   ~0.678  &amp;   ~0.677 &amp; R2   \\
$\beta$   &amp;   ~2.704  &amp;   ~2.780   &amp;   ~2.737  &amp;   ~2.776 &amp; R2   \\
$J$       &amp;   ~6.515  &amp;   ~6.848   &amp;   ~6.410  &amp;   ~4.477 &amp; R7 \\
$H$       &amp;   ~6.607  &amp;   ~6.925   &amp;   ~6.493  &amp;   ~4.669 &amp; R7 \\
$K$       &amp;   ~6.585  &amp;   ~6.907   &amp;   ~6.467  &amp;   ~4.611 &amp; R7 \\
\noalign{\medskip}
Sp. Type  &amp; B9p (HgMn) &amp; B9p Hg(Mn?) &amp; B8(Mn), HgMn &amp; B9.5 IVp (HgMn) &amp; R3,R4,R5\\
          &amp;            &amp;             &amp;              &amp;                 &amp; R10, R11\\
\bottomrule
\tabnotetext{}{References: R1: \citet{cousins-stoy62}, R2: \citet{hauck-mermilliod98}, R3: \citet{andersen-nordstrom77}, 
R4: \citet{renson-manfroid09}, R5: \citet{wolff-wolff74}, R6: \citet{corben-stoy68} , R7: \citet{cutri03}, R8: \citet{crawford63}, 
R9: \citet{corben71}, R10: \citet{cowley69}, R11: \citet{houk82}.}
\end{tabular}
\vspace{0.4cm}
\end{table*}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


The relation of the anomalous abundances and stellar parameters is not totally clear. Some authors found no correlation between the total HgII abundance 
and the effective temperature \citep[e.g., ][]{smith97,woolf-lambert99}, while Dolk, Wahlgren, \&amp; Hubrig (2003) found a possible correlation for a 
sample of 31 HgMn stars. On the other hand, \citet{smith-dworetsky93} and later Jomaron, Dworetsky, \&amp; Allen (1999) found a dependence between MnI and 
MnII abundances and temperature. The authors suggest that difussion takes place in the atmospheres of these stars, but probably affected by other factors 
such as rotation and evolutionary state. This research is part of our current program for deriving elemental abundances among field CP stars and members 
of open clusters. The motivation of our work is to derive abundances for a sample of HgMn stars to determine possible relations with their fundamental 
parameters and other factors such as rotation, evolutionary state and age. In particular in this paper we report the results of four CP stars of the HgMn 
class, HR 3273, HR 8118, HR 8567 and HR 8937.

\vspace{0.15cm}

The star HR 3273 was classified as an HgMn star by \citet{andersen-nordstrom77}. They studied $\sim$70 bright southern stars using coud\'e spectrograms 
of 20~\AA/mm, taken with the ESO 1.5~m telescope at La Silla, Chile. The authors identified HR 3273 as a B9p (HgMn) star, with no definite variation in 
their spectra. $UBV$ photoelectric photometry was published by \citet{cousins-stoy62}. $uvby-\beta$ photometry was provided by \citet{hauck-mermilliod98}, 
\citet{eggen77} and \citet{gronbech-olsen76}. $JHK$ infrared photometry was presented by \citet{cutri03}.

\vspace{0.15cm}

The star HR 8118 was classified as Hg(Mn?) star in the spectroscopic study of the Bright Star Catalogue by \citet{cowley68}. They identified the line 
HgII $\lambda\lambda$3984 in the spectra taken at the Yerkes observatory with a dispersion of 125~\AA/mm. Then the star was listed and classified as B9p 
Hg(Mn?) in the study of A bright stars \citep{cowley69}. $UBV$ photometry was obtained by \citet{crawford63} and \citet{corben71}. $uvby-\beta$ photometry 
was published by \citet{gronbech-olsen77} and \citet{hauck-mermilliod98}.

The star HR 8567 was classified as HgMn star by \citet{wolff-wolff74}. They studied 194 stars of types B4-B9 and identified in their sample 24 HgMn stars. 
The authors used UV spectrograms with a dispersion of 50~\AA/mm in the region 3440--3500~\AA. In this spectral range there are several strong lines of MnII. 
HR 8567 was classified as B8(Mn) star in the catalog of \citet{renson-manfroid09} and listed as HgMn star in the catalog of \citet{schneider81}. $UBV$ 
photoelectric photometry was published by \citet{rybka69} and \citet{corben-stoy68}. $uvby-\beta$ photometry was obtained by \citet{hauck-mermilliod98}, 
\citet{gronbech-olsen76} and \citet{eggen77}, and $JHK$ infrared photometry was presented by \citet{cutri03}.

The star HR 8937 was classified as B9p by \citet{bertaud58} and then listed as B9.5 IVp (HgMn) in the Michigan Catalogue of Two Dimensional Spectral Types 
\citep{houk82}. $UBV$ photoelectric photometry have been provided by \citet{abt-golson62} and \citet{irwin61}. $uvby$ photometry was published by Crawford, 
Barnes, \&amp; Golson (1970) and \citet{hauck-mermilliod98}, and their $\beta$ photometric index were determined by \citet{strauss-ducati81}.

Table~\ref{obsdata} presents some relevant observational data for the sample of HgMn stars, HR 3273, HR~8118, HR 8567 and HR 8937.


\section{Observational material and line identifications} 

The stellar spectra of the stars were obtained at Complejo Astr\'onomico El Leoncito (CASLEO) between April 21 and 23, 2004. We used the \emph{Jorge Sahade} 
2.15~m telescope that fed the EBASIM echelle spectrograph through an optical fiber. The spectra were recorded on a TEK1024 ($1024 \times 1024$~pixels) CCD 
detector. The EBASIM spectrograph uses gratings as cross dispersers. We have used one grating with 226 lines mm$^{-1}$ centered at $\sim$5000~\AA. Three spectra 
of each star were obtained, covering the visual range $\sim$$\lambda\lambda$3800--5900~\AA. The S/N ratio of the spectra is around 250 and the resolving power 
of the spectrograph is approximately 40000. Table~\ref{ranges} gives the spectral coverage of the 55 orders of the EBASIM spectrograph\footnote{Due to modifications 
in the configuration of the EBASIM spectrograph, the spectral coverage could slightly vary in different observing runs.}. It contain echelle orders overlapping 
in $\sim$$\lambda\lambda$3762--5644~\AA\ and increasing gaps of 1--4~\AA\ for $\lambda \gtrsim 5645$~\AA.


%%%%%% TABLA 2

\begin{table}[!t]
\vspace{0.1cm}
\centering
\setlength{\tabcolsep}{1.25\tabcolsep}
\caption{Spectral coverage for the EBASIM echelle spectrograph using the grating of 226 lines \lowercase{mm$^{-1}$}}
\label{ranges}
\small
\begin{tabular}{ccccc}
\toprule
Order     &amp;    Range [\AA]   &amp;     &amp; Order      &amp; Range [\AA]    \\
\cmidrule{1-2}
\cmidrule{4-5}
~1  &amp;  3762--3798  &amp; &amp;  29  &amp;  4625--4670  \\
~2  &amp;  3787--3823  &amp; &amp;  30  &amp;  4663--4708  \\
~3  &amp;  3813--3849  &amp; &amp;  31  &amp;  4702--4748  \\
~4  &amp;  3839--3875  &amp; &amp;  32  &amp;  4741--4788  \\
~5  &amp;  3865--3902  &amp; &amp;  33  &amp;  4781--4828  \\
~6  &amp;  3891--3929  &amp; &amp;  34  &amp;  4822--4869  \\
~7  &amp;  3918--3956  &amp; &amp;  35  &amp;  4864--4911  \\
~8  &amp;  3946--3984  &amp; &amp;  36  &amp;  4906--4954  \\
~9  &amp;  3973--4012  &amp; &amp;  37  &amp;  4949--4998  \\
10  &amp;  4002--4041  &amp; &amp;  38  &amp;  4993--5042  \\
11  &amp;  4030--4070  &amp; &amp;  39  &amp;  5037--5087  \\
12  &amp;  4059--4099  &amp; &amp;  40  &amp;  5083--5133  \\
13  &amp;  4088--4129  &amp; &amp;  41  &amp;  5129--5180  \\
14  &amp;  4118--4159  &amp; &amp;  42  &amp;  5176--5227  \\
15  &amp;  4149--4190  &amp; &amp;  43  &amp;  5224--5276  \\
16  &amp;  4179--4221  &amp; &amp;  44  &amp;  5273--5325  \\
17  &amp;  4210--4252  &amp; &amp;  45  &amp;  5323--5375  \\
18  &amp;  4242--4284  &amp; &amp;  46  &amp;  5374--5426  \\
19  &amp;  4274--4317  &amp; &amp;  47  &amp;  5425--5478  \\
20  &amp;  4307--4350  &amp; &amp;  48  &amp;  5478--5533  \\
21  &amp;  4340--4383  &amp; &amp;  49  &amp;  5533--5588  \\
22  &amp;  4373--4417  &amp; &amp;  50  &amp;  5588--5644  \\
23  &amp;  4407--4451  &amp; &amp;  51  &amp;  5645--5701  \\
24  &amp;  4442--4486  &amp; &amp;  52  &amp;  5703--5760  \\
25  &amp;  4478--4522  &amp; &amp;  53  &amp;  5762--5820  \\
26  &amp;  4514--4558  &amp; &amp;  54  &amp;  5822--5881  \\
27  &amp;  4550--4594  &amp; &amp;  55  &amp;  5884--5943  \\
28  &amp;  4587--4632  &amp; &amp;      &amp;               \\
\bottomrule
\end{tabular}
\vspace{0.3cm}
\end{table}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


The spectra were reduced using IRAF\footnote {IRAF is distributed by the National Optical Astronomical Observatories which is operated by the Association 
of Universities for Research in Astronomy, Inc., under a cooperative agreement with the National Science Foundation.} standard procedures for echelle 
spectra. We applied bias and flat corrections and then normalized order by order with the {\it continuum} task, using 7--9 order Chebyshev polynomials. We 
also corrected the scattered light in the spectrograph ({\it apscatter} task). We fitted the background with a linear function on both sides of the echelle 
apertures, using the task {\it apall}. Extensive description of the characteristics of the reduction technique and some results obtained with the 
observational material, have been previously published \citep[e.g., ][]{saffe3}. The equivalent widths were measured by integrating the profiles across the 
stellar metallic lines using the \emph{splot} task. There are no differences among the equivalent width measurements of the same lines in different spectra. 

We used Gaussian profiles to fit the stellar lines. This is an interactive process in which the IRAF user marks two continuum points in the spectra and then 
the program fits a single line profile (splot task). IRAF uses a fixed linear continuum through the stellar line. The fitting uses an interactive algorithm 
based on the Levenberg-Marquardt method. The successive iterations tend to improve the fit by varying the parameters along the gradient of improvement in 
the $\chi^{2}$ function. The final fit is overplotted on the spectrum of the star and the user decides if the fit is satisfactory or not. The center, continuum 
at the center, core intensity, integrated flux, equivalent width and FWHMs are printed and saved in a log file. All the parameters except the continuum are 
based on the fitted analytic profiles.

\citet{pintado03} compared EBASIM and DAO (Dominion Astrophysical Observatory) equivalent widths corresponding to echelle and coud\'e spectra, respectively. 
The scattered light is usually easier to measure in the latter case. They used Gaussian profiles for the EBASIM spectra and rotational profiles for the DAO 
spectra, due to the lower resolution of the EBASIM data. For 170 unblended lines of the star $\alpha$ Sex in the region 3840--4930~\AA, they obtained nearly 
the same scale for the equivalent widths. Then, they did not apply any additional correction to the equivalent widths of the EBASIM spectra. However, we caution 
that the comparison done in \citet{pintado03} needs to be extended and made more robust. The authors plan to extend it with high S/N ($&gt;500$) spectra of 
sharp-lined stars.

The stellar lines of the HgMn stars were identified using the same procedure of previous papers (Saffe, Levato, \&amp; L\'opez-Garc\'ia 2004, 2005; Saffe \&amp; Levato 
2009). We used the general references of {\it{A Multiplet Table of Astrophysical Interest}} \citep{moo} and {\it{Wavelengths and Transition Probabilities for 
Atoms and Atomic Ions}}, Part 1 (Reader et al. 1980) as well as the more specialized references for \ion{P}{ii} (Svendenius, Magnusson, \&amp; Zetterberg 1983), 
\ion{Mn}{ii} \citep{igl64}, \ion{Fe}{ii} \citep{dworetsky71,joh78,guthrie85} and \ion{Y}{ii} (Nilsson, Johansson, \&amp; Kurucz 1991). The final line list is similar 
to those used in recent papers of HgMn stars \citep{zavala07,adelman10}.


\section{Atmospheric parameters} 

An estimate of the effective temperature and gravity was done by \citet{woolf-lambert99}, who used the Str\"omgren $uvby-\beta$ photometry and the calibration 
of \citet{moon-dworetsky85}. For HR 3273, the authors derived 12350~K and 3.28~dex for $T_{\rm eff}$ and $\log g$, respectively. \citet{gla} used the Shallis-Blackwell 
method and derived two temperatures from the parameters $Q$ and $X$ (reddening free index and multicolor photometry parameter). For HR 8118 they obtained 11900~K 
and 11500~K, while for HR 8937 they obtained 12400 and 12300~K, using the $Q$ and $X$ parameters, respectively. \citet{dolk03} derived a temperature and gravity 
using $uvby$ photometric data but with the calibration of Napiwotzki, Shonberner, \&amp; Wenske (1993). For HR~8567, they obtained 11977~K and 4.06~dex, while for 
HR~8937 they derived 12476~K and 4.13~dex for $T_{\rm eff}$ and $\log g$, respectively.

We compared the observed H$\gamma$ profiles with synthetic spectra of the H$\gamma$ region calculated with SYNTHE \citep{synthe} using Kurucz ATLAS9 (Kurucz 1995, private communication) model atmospheres with [M/H]=0.0, i.e. solar abundance, which seems to be adequate for these stars. However it is difficult to obtain accurate Balmer line profiles in this region from echelle spectra covering several orders. Thus, we estimated $T_{\rm eff}$ and $\log g$ using the $uvby-\beta$ mean colors of \citet{hauck-mermilliod98} with the calibration of \citet{napi}, and then we corrected the $T_{\rm eff}$ values according to \citet{corr}. These values are presented in the first two columns of Table~\ref{tefflogg}. Next we adjusted the surface gravity to get ionization equilibrium from FeI and FeII. A similar strategy was applied by \citet{adelman10} in the derivation of the fundamental parameters. The final adopted values of the fundamental parameters are shown in Table~\ref{tefflogg}.


%%%%%% TABLA 3

\begin{table}
\center
\caption{Temperature and gravity derived for the HgMn stars}
\label{tefflogg}
\footnotesize
\begin{tabular}{ccccc}
\toprule
Star &amp; $uvby-\beta$ &amp; $uvby-\beta$  &amp; Adopted     &amp; Adopted \\
     &amp; $T_{\rm eff}$ &amp; $\log g$     &amp; $T_{\rm eff}$ &amp; $\log g$ \\
\midrule
HR 3273 &amp; 12253 &amp; 3.32 &amp; 12253 &amp;  3.42\\
HR 8118 &amp; 11381 &amp; 4.01 &amp; 11381 &amp;  4.11\\
HR 8567 &amp; 12315 &amp; 3.78 &amp; 12315 &amp;  3.68\\
HR 8937 &amp; 12088 &amp; 4.28 &amp; 12088 &amp;  4.28\\
\bottomrule
\end{tabular}
\end{table}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


We fitted a synthetic spectrum to $\sim$20 Fe lines in order to derive an estimation of the rotational velocities of the HgMn stars. We used the program 
SYNTHE \citep{synthe} and the command {\it{broaden}} to reproduce the instrumental broadening of the EBASIM spectrograph, adopting a resolving power of 
$R \sim 40000$. The value of $R$ is approximate, and thus the derived rotational velocities should be taken with caution. The final $v \sin i$ values are 
obtained using the average and standard deviation of the lines. We derived rotational velocities of $20 \pm 2$~km~s$^{-1}$, $30 \pm1$~km~s$^{-1}$, 
$22\pm 1$~km~s$^{-1}$ and $24 \pm 2$~km~s$^{-1}$ for the stars HR 3273, HR 8118, HR 8567 and HR 8937, respectively. The HgMn stars of our sample are not 
extremely slow rotators.


\section{Abundance analyses} 

To derive the abundances of the chemical species we used the WIDTH9 code (Kurucz 1995, private communication) and equivalent widths measured in the spectra 
of the stars. The program also requires the selection of a model atmosphere and the atomic data for the lines (oscillator strength, excitation potentials, 
damping constants, etc.). The code calculates a theoretical equivalent width for an initial input abundance (taken from the model atmosphere) and compares 
this value with the measured $EW$. WIDTH9 computes basically the line profile and the curve of growth. Then it modifies the abundance iteratively to achieve 
a difference between theoretical and measured equivalent width $&lt; 0.01$~m\AA. The process is repeated for each measured spectral line.


%%%%% TABLA 4

\begin{table*}[!t]
\vspace{0.1cm}
\centering
\label{tab.micro}
\caption{Determination of microturbulent velocity from FeII lines}
\setlength{\tabnotewidth}{0.9\textwidth}
\tablecols{8}
%\setlength{\tabcolsep}{0.7\tabcolsep}
\small
\begin{tabular}{cccccccl}
\toprule
     &amp;         &amp;   &amp; $\xi_{1}$   &amp;               &amp; $\xi_{2}$   &amp;               &amp;  \\
Star &amp; Species &amp; $n$ &amp; km~s$^{-1}$ &amp; $\log N/N_{T}$ &amp; km~s$^{-1}$ &amp; $\log N/N_{T}$ &amp; $gf$-values \\
\midrule
\multirow{2}{*}{HR 3273}   &amp; \multirow{2}{*}{FeII} &amp; 64  &amp; 0.3  &amp; $-4.75\pm0.22$ &amp; 0.0  &amp; $-4.74\pm0.27$ &amp; N4$+$KX$+$MF \\
                           &amp;                       &amp; 37  &amp; 0.9  &amp; $-4.87\pm0.24$ &amp; 0.0  &amp; $-4.80\pm0.28$ &amp; N4$+$MF \\
                           &amp; adopted $\xi$:        &amp; 0.3~km~s$^{-1}$  &amp;     &amp;     &amp;      &amp;                &amp; \\
\multirow{2}{*}{HR 8118}   &amp; \multirow{2}{*}{FeII} &amp; 63  &amp; 1.0  &amp; $-4.36\pm0.21$ &amp; 0.0  &amp; $-4.28\pm0.28$ &amp; N4$+$KX$+$MF \\
                           &amp;                       &amp; 37  &amp; 1.2  &amp; $-4.41\pm0.24$ &amp; 0.0  &amp; $-4.27\pm0.26$ &amp; N4$+$MF \\
                           &amp; adopted $\xi$:        &amp; 0.5~km~s$^{-1}$  &amp;     &amp;     &amp;      &amp;                &amp; \\
\multirow{2}{*}{HR 8567}   &amp; \multirow{2}{*}{FeII} &amp; 56  &amp; 0.0  &amp; $-4.91\pm0.21$ &amp; 0.0  &amp; $-4.91\pm0.28$ &amp; N4$+$KX$+$MF \\
                           &amp;                       &amp; 33  &amp; 0.5  &amp; $-4.99\pm0.24$ &amp; 0.0  &amp; $-4.98\pm0.26$ &amp; N4$+$MF \\
                           &amp; adopted $\xi$:        &amp; 0.1~km~s$^{-1}$  &amp;     &amp;     &amp;      &amp;                &amp; \\
\multirow{2}{*}{HR 8937}   &amp; \multirow{2}{*}{FeII} &amp; 80  &amp; 0.9  &amp; $-4.32\pm0.21$ &amp; 0.0  &amp; $-4.27\pm0.28$ &amp; N4$+$KX$+$MF \\
                           &amp;                       &amp; 39  &amp; 1.1  &amp; $-4.40\pm0.24$ &amp; 0.0  &amp; $-4.29\pm0.26$ &amp; N4$+$MF \\
                           &amp; adopted $\xi$:        &amp; 0.5~km~s$^{-1}$  &amp;     &amp;     &amp;      &amp;                &amp; \\
\bottomrule
\tabnotetext{}{Note: the source of $gf$ values are KX \citep{kb95}, MF (Fuhr, Martin, \&amp; Wiese 1988) and N4 \citep{n4}.}
\end{tabular}
\vspace{0.3cm}
\end{table*}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


\vspace{0.1cm}

The adopted metal line damping constants were the default semi-classical approximations except for those of neutral 
and singly-ionized Ca-Ni lines, whose values are based on the data of \citet{kb95}. For the lines of CII, multiplet 6, 
and MgII, multiplet 4, the adopted values for Stark broadening were based on data of \citet{saha69}, and for SiII
and CaII, the damping constants are those of Lanz, Dimitrijevic, \&amp; Artru (1988), and \citet{cha70} respectively.
We prefer this choice of $gf$ values to the VALD database \citep{pis96} to ensure homogeneity with our previous work.

\vspace{0.1cm}

To determine the abundances we need an initial estimation of the microturbulent velocity ($\xi$). For this estimation 
we have used the standard method. We computed abundances from the FeII lines for a range of possible microturbulent 
velocities ($\xi$). For determining the final values (Table~\ref{tab.micro}), we looked for the conditions that 
the abundances of FeII were not dependent on the equivalent widths ($\xi_{1}$) or that they minimize the rms scatter 
of the abundances ($\xi_{2}$). Values for each species were derived using lines with $gf$ values from 3 different sources: 
KX values \citep{kb95}, MF values \citep{fuhr88} and N4 values \citep{n4}. The sources of $gf$ values shown in the last 
column of Table~\ref{tab.micro} determine the number of lines, $n$. The values derived for the microturbulence using the 
FeII lines are 0.32~km~s$^{-1}$, 0.55~km~s$^{-1}$, 0.13~km~s$^{-1}$ and 0.52 km~s$^{-1}$, for the HgMn stars HR 3273, 
HR 8118, HR 8567 and HR~8937, respectively. Once a $\xi$ value has been fixed the abundances corresponding to all 
chemical species measured are determined using the WIDTH9 code.

\vspace{0.1cm}

In our abundance determination we did not include seriously blended lines. To give an idea of the sensitivity of our results, 
raising the temperature of HR 3273 by $\sim$4\% (500~K) increases the average abundance by $\sim$2\%, and raising the surface 
gravity by $\sim$15\% (0.5~dex) increases the average abundance by $\sim$0.5\%. Table~5 shows the sensivity of the results 
for the abundances to these changes.


%%%%% TABLA 5

\begin{table*}[!t]
\vspace{0.1cm}
\centering
\label{hotter}
\caption{Sensitivity of the derived abundances of HR 3273 to\\ changes in effective temperature and surface gravity}
\setlength{\tabcolsep}{1.5\tabcolsep}
\small
\begin{tabular}{lccc}
\toprule
\multicolumn{1}{c}{HR 3273} &amp; $\log N/H$ for &amp; $\log N/H$ for 500~K &amp; $\log N/H$ for 0.5~dex \\
\multicolumn{1}{c}{Element} &amp; adopted model  &amp; hotter model         &amp;  greater model \\
\midrule
CII    &amp;  $-$3.61 &amp;   $-$3.96 &amp; $-$3.57 \\
OI     &amp;  $-$3.23 &amp;   $-$3.15 &amp; $-$3.27 \\
MgI    &amp;  $-$5.17 &amp;   $-$4.68 &amp; $-$5.26 \\
MgII   &amp;  $-$5.11 &amp;   $-$5.02 &amp; $-$5.08 \\
AlII   &amp;  $-$6.80 &amp;   $-$6.83 &amp; $-$6.70 \\
SiII   &amp;  $-$4.92 &amp;   $-$4.95 &amp; $-$4.89 \\
PII    &amp;  $-$5.97 &amp;   $-$6.13 &amp; $-$5.89 \\
SII    &amp;  $-$4.99 &amp;   $-$5.28 &amp; $-$4.91 \\
CaII   &amp;  $-$5.57 &amp;   $-$5.31 &amp; $-$5.70 \\
ScII   &amp;  $-$8.03 &amp;   $-$7.72 &amp; $-$8.00 \\
TiII   &amp;  $-$6.35 &amp;   $-$6.06 &amp; $-$6.30 \\
CrII   &amp;  $-$5.53 &amp;   $-$5.32 &amp; $-$5.45 \\
MnI    &amp;  $-$4.63 &amp;   $-$4.13 &amp; $-$4.68 \\
MnII   &amp;  $-$4.68 &amp;   $-$4.52 &amp; $-$4.59 \\
FeI    &amp;  $-$4.34 &amp;   $-$3.93 &amp; $-$4.37 \\
FeII   &amp;  $-$4.75 &amp;   $-$4.67 &amp; $-$4.65 \\
FeIII  &amp;  $-$4.56 &amp;   $-$4.81 &amp; $-$4.38 \\
NiII   &amp;  $-$6.74 &amp;   $-$6.66 &amp; $-$6.57 \\
YII    &amp;  $-$7.68 &amp;   $-$7.37 &amp; $-$7.64 \\
ZrII   &amp;  $-$7.79 &amp;   $-$7.46 &amp; $-$7.72 \\
\bottomrule
\end{tabular}
\vspace{0.3cm}
\end{table*}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

We present in the Table~6 the He/H ratios derived comparing the observed HeI line profiles with synthetized spectra. 
We used the program SYNTHE under the LTE condition; the results were convolved with the rotational velocity of the 
star and the instrumental broadening of the spectrograph. The mean derived He/H values are 0.07, 0.09, 0.08 and 0.03, 
for the stars HR 3273, HR 8118, HR 8567 and HR 8937, respectively. 


%%%%% TABLA 6

\begin{table*}[!t]
\vspace{0.1cm}
\centering
\label{helium}
\caption{He/H determination for the sample of HgMn stars}
\begin{tabular}{ccccc}
\toprule
Line &amp; HR 3273 &amp; HR 8118 &amp; HR 8567 &amp; HR 8937 \\
\midrule
3867 &amp; 0.08 &amp; ---  &amp; ---  &amp; ---  \\
4026 &amp; 0.07 &amp; 0.09 &amp; 0.09 &amp; 0.03 \\
4121 &amp; 0.08 &amp; ---  &amp; 0.09 &amp; ---  \\
4471 &amp; 0.06 &amp; 0.09 &amp; 0.07 &amp; 0.03 \\
4713 &amp; 0.06 &amp; 0.09 &amp; 0.08 &amp; 0.03 \\
4921 &amp; ---  &amp; ---  &amp; 0.09 &amp; ---  \\
\midrule
Average &amp; 0.07$\pm$0.01 &amp; 0.09 &amp; 0.08$\pm$0.01 &amp; 0.03 \\
\bottomrule
\end{tabular}
\vspace{0.35cm}
\end{table*}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


Previous works in literature derived the Hg abundance taking into account the isotopic and hyperfine structure, using higher resolution spectra and S/N than 
ours \citep[][]{woolf-lambert99,dolk03}. They determined the isotopic mixture for the line HgII $\lambda\lambda$3984 using similar values of $T_{\rm eff}$ and 
$\log g$. We adopted the Hg abundance derived by these authors for HR 3273 ($-5.25\pm0.32$~dex), HR 8567 ($-5.58\pm0.37$~dex) and HR 8937 ($-4.23\pm0.43$~dex). 
These values are comparable to those derived using the equivalent width of $\lambda\lambda$ 3984, and LTE model atmosphere, i.e. $-$4.83~dex, $-$5.39~dex and 
$-$4.06~dex, for HR 3273, HR 8567 and HR 8937, respectively, with a mean offset of $-$0.23~dex. For HR 8118 we used our estimation based on the equivalent 
width of $\lambda\lambda$ 3984 ($-$5.03~dex) and then we added the mean offset ($-$0.23~dex), obtaining finally $-$5.26~dex for the Hg abundance of this star. 
This is not a perfect solution as some very sharp-lined HgMn stars have $\lambda\lambda$ 3984 lines with a unique distribution of Hg isotopes.


%%%%%% TABLA 7

\begin{table*}[!t]
\vspace{0.1cm}
\centering
\caption{Comparison of derived and solar abundances}
\setlength{\tabcolsep}{1.2\tabcolsep}
\small
\begin{tabular}{lccccccccc}
\toprule
                            &amp; HR 3273       &amp;      &amp; HR 8118        &amp;     &amp; HR 8567        &amp;      &amp; HR 8937        &amp;      &amp; Sun            \\
\multicolumn{1}{c}{Species} &amp; $\log N/N_{H}$ &amp; $n$  &amp; $\log N/N_{H}$ &amp; $n$  &amp; $\log N/N_{H}$ &amp; $n$  &amp; $\log N/N_{H}$  &amp; $n$  &amp; $\log N/N_{H}$  \\
\midrule
HeI  &amp; $-1.12\pm 0.06$  &amp;  ~5 &amp; $-1.01\pm 0.01$  &amp;  ~3 &amp; $-1.04\pm 0.05$  &amp;  ~5 &amp; $-1.47\pm 0.04$  &amp;  ~3 &amp; ~$-$1.01          \\
CII  &amp; $-3.61\pm 0.11$  &amp;  ~2 &amp; $-3.10\pm 0.02$  &amp;  ~2 &amp; $-3.82\pm 0.27$  &amp;  ~3 &amp; $-3.24\pm 0.03$  &amp;  ~2 &amp; ~$-$3.45          \\
OI   &amp; $-$3.23          &amp;  ~1 &amp; $-$3.71          &amp;  ~1 &amp; $-$3.09          &amp;  ~1 &amp;                  &amp;     &amp; ~$-$3.13          \\
MgI  &amp; $-$5.17          &amp;  ~1 &amp; $-4.96\pm 0.02$  &amp;  ~2 &amp; $-$5.14          &amp;  ~1 &amp; $-5.01\pm 0.01$  &amp;  ~2 &amp; ~$-$4.42          \\
MgII &amp; $-5.11\pm 0.03$  &amp;  ~2 &amp; $-4.54\pm 0.10$  &amp;  ~3 &amp; $-4.91\pm 0.03$  &amp;  ~2 &amp; $-4.73\pm 0.15$  &amp;  ~3 &amp; ~$-$4.42          \\
AlII &amp; $-$6.80          &amp;  ~1 &amp; $-$5.47          &amp;  ~1 &amp; $-$6.52          &amp;  ~1 &amp;                  &amp;     &amp; ~$-$5.53          \\
SiII &amp; $-4.92\pm 0.22$  &amp;  ~8 &amp; $-4.61\pm 0.17$  &amp;  ~6 &amp; $-4.78\pm 0.20$  &amp;  ~7 &amp; $-4.52\pm 0.18$  &amp;  ~8 &amp; ~$-$4.45          \\
PII  &amp; $-$5.97          &amp;  ~1 &amp;                  &amp;     &amp;                  &amp;     &amp; $-$5.37          &amp;  ~1 &amp; ~$-$6.55          \\
SII  &amp; $-4.99\pm 0.14$  &amp;  ~7 &amp; $-4.45\pm 0.19$  &amp;  ~5 &amp; $-4.73\pm 0.18$  &amp;  ~7 &amp; $-5.09\pm 0.09$  &amp;  ~3 &amp; ~$-$4.67          \\
CaII &amp; $-$5.57          &amp;  ~1 &amp; $-$6.18          &amp;  ~1 &amp; $-$5.35          &amp;  ~1 &amp; $-$5.93          &amp;  ~1 &amp; ~$-$5.64          \\
ScII &amp; $-$8.03          &amp;  ~1 &amp; $-$7.02          &amp;  ~1 &amp; $-$7.62          &amp;  ~1 &amp;                  &amp;     &amp; ~$-$8.83          \\
TiII &amp; $-6.35\pm 0.24$  &amp;  34 &amp; $-6.11\pm 0.22$  &amp;  34 &amp; $-5.97\pm 0.23$  &amp;  32 &amp; $-6.60\pm 0.23$  &amp;  26 &amp; ~$-$6.98          \\
CrI  &amp;                  &amp;     &amp; $-$5.20          &amp;  ~1 &amp;                  &amp;     &amp;                  &amp;     &amp; ~$-$6.33          \\
CrII &amp; $-5.53\pm 0.23$  &amp;  37 &amp; $-5.19\pm 0.19$  &amp;  23 &amp; $-5.34\pm 0.21$  &amp;  32 &amp; $-5.73\pm 0.25$  &amp;  30 &amp; ~$-$6.33          \\
MnI  &amp; $-4.63\pm 0.22$  &amp;  ~7 &amp; $-5.54\pm 0.18$  &amp;  ~3 &amp; $-4.20\pm 0.26$  &amp;  14 &amp; $-4.67\pm 0.19$  &amp;  11 &amp; ~$-$6.61          \\
MnII &amp; $-4.68\pm 0.21$  &amp;  39 &amp; $-5.26\pm 0.32$  &amp;  12 &amp; $-4.25\pm 0.23$  &amp;  41 &amp; $-4.46\pm 0.21$  &amp;  39 &amp; ~$-$6.61          \\
FeI  &amp; $-4.34\pm 0.02$  &amp;  ~2 &amp; $-4.27\pm 0.35$  &amp;  19 &amp; $-4.78\pm 0.24$  &amp;  ~3 &amp; $-4.30\pm 0.40$  &amp;  18 &amp; ~$-$4.50          \\
FeII &amp; $-4.75\pm 0.21$  &amp;  64 &amp; $-4.31\pm 0.19$  &amp;  63 &amp; $-4.91\pm 0.21$  &amp;  56 &amp; $-4.29\pm 0.20$  &amp;  80 &amp; ~$-$4.50          \\
FeIII&amp; $-$4.56          &amp;  ~1 &amp;                  &amp;     &amp;                  &amp;     &amp; $-$4.35          &amp;  ~1 &amp; ~$-$4.50          \\
NiII &amp; $-6.74\pm 0.30$  &amp;  ~2 &amp; $-6.06\pm 0.21$  &amp;   2 &amp; $-6.79\pm 0.25$  &amp;  ~2 &amp;                  &amp;     &amp; ~$-$5.75          \\
SrII &amp;                  &amp;     &amp; $-$8.43          &amp;  ~1 &amp; $-$8.35          &amp;  ~1 &amp; $-$6.30          &amp;  ~1 &amp; ~$-$9.03          \\
YII  &amp; $-7.68\pm 0.26$  &amp;  ~5 &amp; $-6.32\pm 0.24$  &amp;  ~9 &amp; $-7.40\pm 0.16$  &amp;  ~8 &amp; $-6.37\pm 0.20$  &amp;  11 &amp; ~$-$9.76          \\
ZrII &amp; $-7.79\pm 0.05$  &amp;  ~2 &amp; $-7.06\pm 0.16$  &amp;  13 &amp; $-7.59\pm 0.32$  &amp;  ~2 &amp; $-7.72\pm 0.14$  &amp;  ~6 &amp; ~$-$9.40          \\
BaII &amp;                  &amp;     &amp; $-$9.17          &amp;  ~1 &amp;                  &amp;     &amp;                  &amp;     &amp; ~$-$9.87          \\
HgII &amp; $-$5.25          &amp;  ~1 &amp; $-$5.03          &amp;  ~1 &amp; $-$5.58          &amp;  ~1 &amp; $-$4.23          &amp;  ~1 &amp; $-$10.83         \\
\midrule
$T_{\rm eff}$&amp; 12253      &amp;     &amp; 11381            &amp;      &amp; 12315 &amp;       &amp; 12088   &amp;       &amp;           \\
$\log g$   &amp; ~3.42            &amp;      &amp;  4.11     &amp;      &amp; ~3.68 &amp;         &amp; ~4.28   &amp;       &amp;           \\
\bottomrule
\end{tabular}
\vspace{0.825cm}
\end{table*}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


%%%%% TABLA 8

\setcounter{table}{7} 
\begin{table*}[!t]
\vspace{0.1cm}
\centering
\caption{Line abundances of HR 3273}
\setlength{\tabnotewidth}{0.99\textwidth}
\tablecols{17}
\setlength{\tabcolsep}{0.778\tabcolsep}
\casitiny
\begin{tabular}{clcccccccclcccccc}
\toprule
Code &amp; \multicolumn{1}{c}{Species} &amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) &amp;  &amp; Code &amp; \multicolumn{1}{c}{Species} 
&amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) \\  
\cmidrule{1-8}
\cmidrule{10-17}
~6.01 &amp; C II   &amp;  ~~4 &amp; 3918.97 &amp; $-$0.53 &amp; WF &amp; ~19 &amp; $-$3.72  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~31 &amp; 4261.91 &amp; $-$1.53 &amp; KX &amp; 46 &amp; $-$5.40 \\
~6.01 &amp; C II   &amp;  ~~4 &amp; 3920.68 &amp; $-$0.23 &amp; WF &amp; ~30 &amp; $-$3.49  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~31 &amp; 4275.57 &amp; $-$1.70 &amp; KX &amp; 42 &amp; $-$5.36 \\
~8.00 &amp; O I    &amp;  ~12 &amp; 5330.73 &amp; $-$0.87 &amp; WF &amp; ~22 &amp; $-$3.22  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~44 &amp; 4554.99 &amp; $-$1.38 &amp; MF &amp; 47 &amp; $-$5.42 \\
12.00 &amp; Mg I   &amp;  ~~2 &amp; 5183.60 &amp; $-$0.16 &amp; WS &amp; ~~6 &amp; $-$5.17  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~39 &amp; 4565.74 &amp; $-$2.11 &amp; MF &amp; 25 &amp; $-$5.36 \\
12.01 &amp; Mg II  &amp;  ~10 &amp; 4390.57 &amp; $-$0.53 &amp; WS &amp; ~23 &amp; $-$5.14  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~44 &amp; 4588.20 &amp; $-$0.63 &amp; MF &amp; 79 &amp; $-$5.05 \\
12.01 &amp; Mg II  &amp;  ~~9 &amp; 4427.99 &amp; $-$1.21 &amp; WS &amp; ~~6 &amp; $-$5.07  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~44 &amp; 4592.05 &amp; $-$1.22 &amp; MF &amp; 42 &amp; $-$5.72 \\
13.01 &amp; Al II  &amp;  ~~2 &amp; 4663.05 &amp; $-$0.28 &amp; FW &amp; ~~5 &amp; $-$6.80  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~44 &amp; 4616.63 &amp; $-$1.29 &amp; MF &amp; 43 &amp; $-$5.64 \\
14.01 &amp; Si II  &amp;  ~~1 &amp; 3853.66 &amp; $-$1.44 &amp; LA &amp; ~50 &amp; $-$5.18  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~44 &amp; 4618.80 &amp; $-$1.11 &amp; MF &amp; 60 &amp; $-$5.22 \\
14.01 &amp; Si II  &amp;  ~~1 &amp; 3856.02 &amp; $-$0.49 &amp; LA &amp; ~96 &amp; $-$5.10  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~44 &amp; 4634.07 &amp; $-$1.24 &amp; MF &amp; 55 &amp; $-$5.27 \\
14.01 &amp; Si II  &amp;  ~~1 &amp; 3862.59 &amp; $-$0.74 &amp; LA &amp; ~90 &amp; $-$4.97  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~30 &amp; 4836.23 &amp; $-$2.25 &amp; MF &amp; 24 &amp; $-$5.31 \\
14.01 &amp; Si II  &amp; 3.01 &amp; 4075.45 &amp; $-$1.40 &amp; SG &amp; ~14 &amp; $-$4.85  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~30 &amp; 4848.23 &amp; $-$1.14 &amp; MF &amp; 51 &amp; $-$5.63 \\
14.01 &amp; Si II  &amp; 3.01 &amp; 4076.78 &amp; $-$1.67 &amp; SG &amp; ~13 &amp; $-$4.61  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~30 &amp; 4884.61 &amp; $-$2.08 &amp; MF &amp; 19 &amp; $-$5.63 \\
14.01 &amp; Si II  &amp;  ~~3 &amp; 4128.05 &amp;  ~~0.38 &amp; LA &amp; 120 &amp; $-$4.54  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~190 &amp; 4912.46 &amp; $-$0.95 &amp; KX &amp; 17 &amp; $-$5.53 \\
14.01 &amp; Si II  &amp;  ~~3 &amp; 4130.89 &amp;  ~~0.53 &amp; LA &amp; ~91 &amp; $-$5.06  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5232.50 &amp; $-$2.09 &amp; KX &amp; 15 &amp; $-$5.67 \\
14.01 &amp; Si II  &amp;  ~~5 &amp; 5041.02 &amp;  ~~0.29 &amp; SG &amp; ~60 &amp; $-$5.07  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5237.33 &amp; $-$1.16 &amp; MF &amp; 52 &amp; $-$5.42 \\
15.01 &amp; P II   &amp;  ~15 &amp; 4602.07 &amp;  ~~0.74 &amp; WS &amp; ~~8 &amp; $-$5.97  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~23 &amp; 5246.77 &amp; $-$2.45 &amp; MF &amp; 20 &amp; $-$5.31 \\
16.01 &amp; S II   &amp;  ~44 &amp; 4153.07 &amp;  ~~0.62 &amp; WS &amp; ~11 &amp; $-$4.94  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~23 &amp; 5249.44 &amp; $-$2.43 &amp; KX &amp; 13 &amp; $-$5.54 \\
16.01 &amp; S II   &amp;  ~44 &amp; 4162.66 &amp;  ~~0.78 &amp; WS &amp; ~12 &amp; $-$4.99  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5274.96 &amp; $-$1.29 &amp; KX &amp; 48 &amp; $-$5.43 \\
16.01 &amp; S II   &amp;  ~~9 &amp; 4815.55 &amp;  ~~0.18 &amp; WM &amp; ~~9 &amp; $-$5.26  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5279.88 &amp; $-$2.10 &amp; MF &amp; 34 &amp; $-$5.05 \\
16.01 &amp; S II   &amp;  ~~7 &amp; 4925.34 &amp; $-$0.47 &amp; WS &amp; ~~7 &amp; $-$4.77  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5280.05 &amp; $-$2.01 &amp; KX &amp; 36 &amp; $-$5.08 \\
16.01 &amp; S II   &amp;  ~15 &amp; 5014.04 &amp;  ~~0.03 &amp; KX &amp; ~~8 &amp; $-$4.99  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5308.44 &amp; $-$1.81 &amp; MF &amp; 25 &amp; $-$5.61 \\
16.01 &amp; S II   &amp;  ~39 &amp; 5212.62 &amp;  ~~0.24 &amp; WS &amp; ~~6 &amp; $-$4.91  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5310.70 &amp; $-$2.28 &amp; MF &amp; 17 &amp; $-$5.39 \\
16.01 &amp; S II   &amp;  ~38 &amp; 5320.72 &amp;  ~~0.46 &amp; WS &amp; ~~6 &amp; $-$5.08  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5313.59 &amp; $-$1.65 &amp; MF &amp; 33 &amp; $-$5.54 \\
20.01 &amp; Ca II  &amp;  ~~1 &amp; 3933.66 &amp;  ~~0.13 &amp; WM &amp; 212 &amp; $-$5.57  &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5334.87 &amp; $-$1.56 &amp; KX &amp; 34 &amp; $-$5.59 \\
21.01 &amp; Sc II  &amp;  ~~7 &amp; 4246.82 &amp;  ~~0.24 &amp; LD &amp; ~40 &amp; $-$8.03  &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~~2 &amp; 4030.75 &amp; $-$0.47 &amp; MF &amp; 15 &amp; $-$4.91 \\
22.01 &amp; Ti II  &amp;  ~34 &amp; 3900.54 &amp; $-$0.45 &amp; MF &amp; ~55 &amp; $-$6.38  &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~~2 &amp; 4033.06 &amp; $-$0.62 &amp; MF &amp; 19 &amp; $-$4.62 \\
22.01 &amp; Ti II  &amp;  ~34 &amp; 3913.46 &amp; $-$0.53 &amp; MF &amp; ~50 &amp; $-$6.50  &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~~2 &amp; 4034.48 &amp; $-$0.81 &amp; MF &amp; ~9 &amp; $-$4.84 \\
22.01 &amp; Ti II  &amp;  ~31 &amp; 3932.02 &amp; $-$1.78 &amp; MF &amp; ~10 &amp; $-$6.49  &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~~5 &amp; 4041.35 &amp;  ~~0.29 &amp; MF &amp; 13 &amp; $-$4.69 \\
22.01 &amp; Ti II  &amp;  ~11 &amp; 4012.38 &amp; $-$1.61 &amp; MF &amp; ~35 &amp; $-$6.11  &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~28 &amp; 4462.03 &amp;  ~~0.32 &amp; MF &amp; ~9 &amp; $-$4.47 \\
22.01 &amp; Ti II  &amp;  ~87 &amp; 4028.34 &amp; $-$1.00 &amp; MF &amp; ~14 &amp; $-$6.69  &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~21 &amp; 4762.37 &amp;  ~~0.42 &amp; MF &amp; 21 &amp; $-$4.19 \\
22.01 &amp; Ti II  &amp;  ~87 &amp; 4053.82 &amp; $-$1.21 &amp; MF &amp; ~22 &amp; $-$6.22  &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~16 &amp; 4783.43 &amp;  ~~0.04 &amp; MF &amp; ~7 &amp; $-$4.69 \\
22.01 &amp; Ti II  &amp;  105 &amp; 4163.64 &amp; $-$0.40 &amp; MF &amp; ~35 &amp; $-$6.34  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3859.21 &amp; $-$2.56 &amp; KX &amp; 11 &amp; $-$4.91 \\
22.01 &amp; Ti II  &amp;  ~20 &amp; 4287.87 &amp; $-$2.02 &amp; MF &amp; ~19 &amp; $-$5.91  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3878.99 &amp; $-$1.71 &amp; KX &amp; 40 &amp; $-$4.73 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4294.09 &amp; $-$1.11 &amp; MF &amp; ~37 &amp; $-$6.33  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3917.32 &amp; $-$1.15 &amp; KX &amp; 29 &amp; $-$4.97 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4300.04 &amp; $-$0.77 &amp; MF &amp; ~58 &amp; $-$5.97  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3930.95 &amp; $-$2.15 &amp; KX &amp; 13 &amp; $-$4.68 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4301.92 &amp; $-$1.16 &amp; MF &amp; ~20 &amp; $-$6.70  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3952.42 &amp; $-$1.50 &amp; KX &amp; 12 &amp; $-$4.78 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4312.86 &amp; $-$1.16 &amp; MF &amp; ~27 &amp; $-$6.49  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3986.58 &amp; $-$2.60 &amp; KX &amp; 14 &amp; $-$4.70 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4320.95 &amp; $-$1.87 &amp; MF &amp; ~17 &amp; $-$6.07  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4000.05 &amp; $-$1.21 &amp; KX &amp; 26 &amp; $-$4.58 \\
22.01 &amp; Ti II  &amp;  ~51 &amp; 4394.06 &amp; $-$1.59 &amp; MF &amp; ~~6 &amp; $-$6.86  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4081.44 &amp; $-$2.24 &amp; KX &amp; 28 &amp; $-$4.27 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4395.03 &amp; $-$0.66 &amp; MF &amp; ~49 &amp; $-$6.41  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4087.91 &amp; $-$2.91 &amp; KX &amp; ~7 &amp; $-$4.81 \\
22.01 &amp; Ti II  &amp;  ~61 &amp; 4395.84 &amp; $-$2.17 &amp; MF &amp; ~~8 &amp; $-$6.14  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4136.90 &amp; $-$1.29 &amp; KX &amp; 59 &amp; $-$4.21 \\
22.01 &amp; Ti II  &amp;  ~61 &amp; 4409.24 &amp; $-$2.64 &amp; KX &amp; ~~5 &amp; $-$5.90  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4140.44 &amp; $-$2.46 &amp; KX &amp; 17 &amp; $-$4.67 \\
22.01 &amp; Ti II  &amp;  115 &amp; 4411.07 &amp; $-$1.06 &amp; MF &amp; ~10 &amp; $-$6.25  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~2 &amp; 4174.32 &amp; $-$3.55 &amp; KX &amp; 44 &amp; $-$4.62 \\
22.01 &amp; Ti II  &amp;  ~40 &amp; 4417.71 &amp; $-$1.43 &amp; MF &amp; ~21 &amp; $-$6.39  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4184.45 &amp; $-$1.95 &amp; KX &amp; 22 &amp; $-$4.72 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4443.80 &amp; $-$0.70 &amp; MF &amp; ~45 &amp; $-$6.50  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4200.27 &amp; $-$1.74 &amp; KX &amp; 32 &amp; $-$4.64 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4450.48 &amp; $-$1.45 &amp; MF &amp; ~16 &amp; $-$6.58  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~2 &amp; 4205.38 &amp; $-$3.38 &amp; KX &amp; 51 &amp; $-$4.54 \\
22.01 &amp; Ti II  &amp;  ~31 &amp; 4468.49 &amp; $-$0.60 &amp; MF &amp; ~44 &amp; $-$6.60  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4240.39 &amp; $-$2.07 &amp; KX &amp; 25 &amp; $-$4.51 \\
22.01 &amp; Ti II  &amp;  115 &amp; 4488.32 &amp; $-$0.82 &amp; MF &amp; ~17 &amp; $-$6.18  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~7 &amp; 4244.25 &amp; $-$2.39 &amp; KX &amp; 33 &amp; $-$4.34 \\
22.01 &amp; Ti II  &amp;  ~31 &amp; 4501.27 &amp; $-$0.75 &amp; MF &amp; ~41 &amp; $-$6.56  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4251.73 &amp; $-$1.06 &amp; KX &amp; 52 &amp; $-$4.68 \\
22.01 &amp; Ti II  &amp;  ~50 &amp; 4533.96 &amp; $-$0.77 &amp; MF &amp; ~57 &amp; $-$5.97  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~2 &amp; 4260.46 &amp; $-$4.25 &amp; KX &amp; 15 &amp; $-$4.77 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4563.76 &amp; $-$0.96 &amp; MF &amp; ~35 &amp; $-$6.46  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4377.74 &amp; $-$2.14 &amp; KX &amp; 20 &amp; $-$4.95 \\
22.01 &amp; Ti II  &amp;  ~82 &amp; 4571.97 &amp; $-$0.53 &amp; MF &amp; ~53 &amp; $-$6.19  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4393.38 &amp; $-$2.32 &amp; KX &amp; 15 &amp; $-$4.94 \\
22.01 &amp; Ti II  &amp;  ~59 &amp; 4657.20 &amp; $-$2.15 &amp; MF &amp; ~~7 &amp; $-$6.23  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4403.51 &amp; $-$1.80 &amp; KX &amp; 11 &amp; $-$5.08 \\
22.01 &amp; Ti II  &amp;  ~92 &amp; 4779.98 &amp; $-$1.37 &amp; MF &amp; ~13 &amp; $-$6.28  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4478.64 &amp; $-$0.95 &amp; KX &amp; 40 &amp; $-$4.92 \\
22.01 &amp; Ti II  &amp;  ~82 &amp; 4805.09 &amp; $-$1.10 &amp; MF &amp; ~17 &amp; $-$6.39  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4497.94 &amp; $-$2.59 &amp; KX &amp; ~9 &amp; $-$4.98 \\
22.01 &amp; Ti II  &amp;  ~14 &amp; 4911.20 &amp; $-$0.34 &amp; MF &amp; ~17 &amp; $-$6.65  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4503.20 &amp; $-$2.16 &amp; KX &amp; 15 &amp; $-$4.82 \\
22.01 &amp; Ti II  &amp;  ~86 &amp; 5129.16 &amp; $-$1.39 &amp; MF &amp; ~~9 &amp; $-$6.53  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4689.55 &amp; $-$2.54 &amp; KX &amp; 11 &amp; $-$4.56 \\
22.01 &amp; Ti II  &amp;  ~86 &amp; 5185.90 &amp; $-$1.35 &amp; MF &amp; ~17 &amp; $-$6.24  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4702.73 &amp; $-$2.34 &amp; KX &amp; 10 &amp; $-$4.78 \\
22.01 &amp; Ti II  &amp;  ~~7 &amp; 5188.69 &amp; $-$1.21 &amp; MF &amp; ~17 &amp; $-$6.52  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4717.26 &amp; $-$1.86 &amp; KX &amp; 15 &amp; $-$4.86 \\
24.01 &amp; Cr II  &amp;  167 &amp; 3865.60 &amp; $-$0.78 &amp; KX &amp; ~32 &amp; $-$5.84  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4730.40 &amp; $-$2.15 &amp; KX &amp; 40 &amp; $-$4.33 \\
24.01 &amp; Cr II  &amp;  130 &amp; 3866.52 &amp; $-$2.07 &amp; KX &amp; ~~4 &amp; $-$5.86  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4749.11 &amp; $-$2.00 &amp; KX &amp; 16 &amp; $-$4.85 \\
24.01 &amp; Cr II  &amp;  129 &amp; 3911.32 &amp; $-$2.06 &amp; KX &amp; ~~9 &amp; $-$5.56  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4764.73 &amp; $-$1.35 &amp; KX &amp; 62 &amp; $-$4.37 \\
24.01 &amp; Cr II  &amp;  183 &amp; 3979.50 &amp; $-$0.73 &amp; KX &amp; ~30 &amp; $-$5.79  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4791.78 &amp; $-$1.72 &amp; KX &amp; 29 &amp; $-$4.69 \\
24.01 &amp; Cr II  &amp;  183 &amp; 4012.50 &amp; $-$0.89 &amp; KX &amp; ~37 &amp; $-$5.44  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4806.82 &amp; $-$1.56 &amp; KX &amp; 46 &amp; $-$4.72 \\
24.01 &amp; Cr II  &amp;  ~19 &amp; 4051.93 &amp; $-$2.19 &amp; KX &amp; ~22 &amp; $-$5.80  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4830.06 &amp; $-$1.85 &amp; KX &amp; 25 &amp; $-$4.70 \\
24.01 &amp; Cr II  &amp;  ~19 &amp; 4054.08 &amp; $-$2.48 &amp; KX &amp; ~24 &amp; $-$5.46  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4839.74 &amp; $-$1.86 &amp; KX &amp; 19 &amp; $-$4.87 \\
24.01 &amp; Cr II  &amp;  ~26 &amp; 4072.56 &amp; $-$2.41 &amp; KX &amp; ~10 &amp; $-$5.76  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4842.32 &amp; $-$2.01 &amp; KX &amp; 25 &amp; $-$4.53 \\
24.01 &amp; Cr II  &amp;  165 &amp; 4082.28 &amp; $-$1.23 &amp; KX &amp; ~13 &amp; $-$5.99  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 5102.52 &amp; $-$1.93 &amp; KX &amp; 27 &amp; $-$4.63 \\
24.01 &amp; Cr II  &amp;  ~26 &amp; 4086.13 &amp; $-$2.42 &amp; KX &amp; ~~8 &amp; $-$5.83  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 5177.65 &amp; $-$1.77 &amp; KX &amp; 44 &amp; $-$4.24 \\
24.01 &amp; Cr II  &amp;  ~26 &amp; 4132.42 &amp; $-$2.35 &amp; KX &amp; ~11 &amp; $-$5.73  &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3902.36 &amp; $-$2.72 &amp; KX &amp; 13 &amp; $-$4.57 \\
24.01 &amp; Cr II  &amp;  162 &amp; 4145.78 &amp; $-$1.16 &amp; KX &amp; ~25 &amp; $-$5.66  &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~43 &amp; 4132.06 &amp; $-$0.68 &amp; N4 &amp; ~4 &amp; $-$4.31 \\
24.01 &amp; Cr II  &amp;  ~26 &amp; 4179.42 &amp; $-$1.77 &amp; KX &amp; ~23 &amp; $-$5.84  &amp;  &amp; 26.00 &amp; Fe I   &amp; 1146 &amp; 5383.37 &amp;  ~~0.65 &amp; N4 &amp; ~3 &amp; $-$4.36 \\
\bottomrule
\end{tabular}
\end{table*}


%%%%% CONTINUA TABLA 8

\setcounter{table}{7} 
\begin{table*}[!t]
\vspace{0.1cm}
\centering
\centerline{TABLE~8 (CONTINUED)\smallskip}
\setlength{\tabnotewidth}{0.99\textwidth}
\tablecols{17}
\setlength{\tabcolsep}{0.778\tabcolsep}
\casitiny
\begin{tabular}{clcccccccclcccccc}
\toprule
Code &amp; \multicolumn{1}{c}{Species} &amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) &amp;  &amp; Code &amp; \multicolumn{1}{c}{Species} 
&amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) \\  
\cmidrule{1-8}
\cmidrule{10-17}
26.01 &amp; Fe II  &amp;  ~38 &amp; 3935.96 &amp; $-$1.86 &amp; N4 &amp; 18 &amp; $-$4.78 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5018.44 &amp; $-$1.22 &amp; MF &amp; 88 &amp; $-$4.44 \\
26.01 &amp; Fe II  &amp;  ~~3 &amp; 3938.29 &amp; $-$4.07 &amp; N4 &amp; 11 &amp; $-$4.72 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5021.59 &amp; $-$0.30 &amp; KX &amp; 11 &amp; $-$4.37 \\
26.01 &amp; Fe II  &amp;  190 &amp; 3938.97 &amp; $-$1.85 &amp; N4 &amp; 16 &amp; $-$4.71 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5022.79 &amp; $-$0.02 &amp; KX &amp; 12 &amp; $-$4.60 \\
26.01 &amp; Fe II  &amp;  127 &amp; 4024.55 &amp; $-$2.44 &amp; N4 &amp; 11 &amp; $-$4.99 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5035.71 &amp;  ~~0.61 &amp; KX &amp; 27 &amp; $-$4.63 \\
26.01 &amp; Fe II  &amp;  172 &amp; 4048.83 &amp; $-$2.14 &amp; N4 &amp; 23 &amp; $-$4.34 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5061.72 &amp;  ~~0.22 &amp; KX &amp; 11 &amp; $-$4.88 \\
26.01 &amp; Fe II  &amp;  ~28 &amp; 4122.67 &amp; $-$3.38 &amp; N4 &amp; 15 &amp; $-$4.82 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5070.90 &amp;  ~~0.24 &amp; KX &amp; 11 &amp; $-$4.88 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4233.17 &amp; $-$1.81 &amp; N4 &amp; 77 &amp; $-$4.36 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5075.76 &amp;  ~~0.28 &amp; KX &amp; 12 &amp; $-$4.78 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4273.33 &amp; $-$3.34 &amp; N4 &amp; 11 &amp; $-$4.95 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5093.58 &amp;  ~~0.11 &amp; KX &amp; 12 &amp; $-$4.65 \\
26.01 &amp; Fe II  &amp;  ~28 &amp; 4296.57 &amp; $-$3.01 &amp; N4 &amp; 24 &amp; $-$4.81 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5097.27 &amp;  ~~0.31 &amp; KX &amp; 25 &amp; $-$4.37 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4303.18 &amp; $-$2.61 &amp; N4 &amp; 51 &amp; $-$4.38 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5106.11 &amp; $-$0.28 &amp; KX &amp; 10 &amp; $-$4.38 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4351.77 &amp; $-$2.08 &amp; N4 &amp; 44 &amp; $-$5.16 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5145.77 &amp; $-$0.40 &amp; KX &amp; ~8 &amp; $-$4.33 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4357.58 &amp; $-$2.10 &amp; KX &amp; 11 &amp; $-$4.59 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5150.49 &amp; $-$0.12 &amp; KX &amp; 11 &amp; $-$4.46 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4385.39 &amp; $-$2.57 &amp; N4 &amp; 34 &amp; $-$4.92 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5169.03 &amp; $-$0.87 &amp; MF &amp; 90 &amp; $-$4.72 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4416.83 &amp; $-$2.60 &amp; N4 &amp; 33 &amp; $-$4.92 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5199.12 &amp;  ~~0.10 &amp; KX &amp; ~7 &amp; $-$4.92 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4489.18 &amp; $-$2.97 &amp; N4 &amp; 23 &amp; $-$4.83 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5216.85 &amp;  ~~0.81 &amp; KX &amp; 19 &amp; $-$5.01 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4491.40 &amp; $-$2.70 &amp; N4 &amp; 24 &amp; $-$5.04 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5228.90 &amp; $-$0.30 &amp; KX &amp; ~7 &amp; $-$4.49 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4508.29 &amp; $-$2.21 &amp; N4 &amp; 42 &amp; $-$4.99 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5232.79 &amp; $-$0.06 &amp; KX &amp; 14 &amp; $-$4.37 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4515.34 &amp; $-$2.48 &amp; N4 &amp; 34 &amp; $-$4.99 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5234.62 &amp; $-$2.05 &amp; MF &amp; 45 &amp; $-$4.84 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4520.22 &amp; $-$2.60 &amp; N4 &amp; 33 &amp; $-$4.91 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5247.95 &amp;  ~~0.55 &amp; N4 &amp; 18 &amp; $-$4.74 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4522.63 &amp; $-$2.03 &amp; N4 &amp; 47 &amp; $-$5.03 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5254.93 &amp; $-$3.23 &amp; KX &amp; 11 &amp; $-$4.79 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4541.52 &amp; $-$3.05 &amp; N4 &amp; 17 &amp; $-$4.92 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5257.12 &amp;  ~~0.03 &amp; KX &amp; ~9 &amp; $-$4.66 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4555.89 &amp; $-$2.29 &amp; N4 &amp; 42 &amp; $-$4.94 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5260.25 &amp;  ~~1.07 &amp; KX &amp; 33 &amp; $-$4.82 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4576.34 &amp; $-$3.04 &amp; N4 &amp; 17 &amp; $-$4.93 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5272.40 &amp; $-$2.03 &amp; MF &amp; 16 &amp; $-$4.44 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4582.84 &amp; $-$3.10 &amp; N4 &amp; 15 &amp; $-$4.94 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5276.00 &amp; $-$1.94 &amp; MF &amp; 45 &amp; $-$4.96 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4583.84 &amp; $-$2.02 &amp; N4 &amp; 60 &amp; $-$4.62 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5291.67 &amp;  ~~0.58 &amp; KX &amp; 17 &amp; $-$4.86 \\
26.01 &amp; Fe II  &amp;  ~~D &amp; 4596.02 &amp; $-$1.84 &amp; N4 &amp; 12 &amp; $-$4.69 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5339.59 &amp;  ~~0.54 &amp; KX &amp; 17 &amp; $-$4.80 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4620.52 &amp; $-$3.28 &amp; N4 &amp; 15 &amp; $-$4.76 &amp;  &amp; 26.02 &amp; Fe III &amp;  ~~4 &amp; 4419.60 &amp; $-$2.22 &amp; KX &amp; ~7 &amp; $-$4.56 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4629.34 &amp; $-$2.37 &amp; N4 &amp; 38 &amp; $-$4.98 &amp;  &amp; 28.01 &amp; Ni II  &amp;  ~12 &amp; 4015.47 &amp; $-$2.42 &amp; KX &amp; ~4 &amp; $-$6.44 \\
26.01 &amp; Fe II  &amp;  186 &amp; 4635.32 &amp; $-$1.65 &amp; N4 &amp; 22 &amp; $-$4.65 &amp;  &amp; 28.01 &amp; Ni II  &amp;  ~11 &amp; 4067.03 &amp; $-$1.29 &amp; KX &amp; 12 &amp; $-$7.03 \\
26.01 &amp; Fe II  &amp;  ~28 &amp; 4666.76 &amp; $-$3.33 &amp; N4 &amp; 11 &amp; $-$4.90 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~~6 &amp; 3950.35 &amp; $-$0.49 &amp; HL &amp; 12 &amp; $-$7.90 \\
26.01 &amp; Fe II  &amp;  ~43 &amp; 4731.45 &amp; $-$3.13 &amp; N4 &amp; 17 &amp; $-$4.82 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~~6 &amp; 3982.59 &amp; $-$0.49 &amp; HL &amp; 11 &amp; $-$7.96 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4913.29 &amp;  ~~0.01 &amp; KX &amp; 11 &amp; $-$4.69 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~14 &amp; 4124.90 &amp; $-$1.50 &amp; HL &amp; ~4 &amp; $-$7.25 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4951.58 &amp;  ~~0.18 &amp; KX &amp; 14 &amp; $-$4.69 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~22 &amp; 4900.12 &amp; $-$0.09 &amp; HL &amp; 14 &amp; $-$7.74 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4977.04 &amp;  ~~0.04 &amp; KX &amp; 11 &amp; $-$4.65 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~20 &amp; 5205.72 &amp; $-$0.34 &amp; HL &amp; 12 &amp; $-$7.57 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4990.51 &amp;  ~~0.18 &amp; KX &amp; 13 &amp; $-$4.72 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~16 &amp; 3998.95 &amp; $-$0.67 &amp; GB &amp; ~6 &amp; $-$7.84 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4993.36 &amp; $-$3.65 &amp; MF &amp; ~6 &amp; $-$4.88 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~30 &amp; 4045.64 &amp; $-$0.60 &amp; KX &amp; ~8 &amp; $-$7.74 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5001.96 &amp;  ~~0.90 &amp; KX &amp; 30 &amp; $-$4.86 &amp;  &amp; 80.01 &amp; Hg II  &amp;  $-$ &amp; 3983.94 &amp; $-$1.73 &amp; DW &amp; 83 &amp; $-$4.83 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5004.20 &amp;  ~~0.50 &amp; KX &amp; 18 &amp; $-$4.85 &amp;  &amp;       &amp;        &amp;      &amp;         &amp;         &amp;    &amp;    &amp;         \\
\bottomrule
\end{tabular}
\vspace{0.7cm}
\end{table*}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


%%%%% TABLA 9

\setcounter{table}{8} 
\begin{table*}[!t]
\vspace{0.1cm}
\centering
\caption{Line abundances of HR 8118}
\setlength{\tabnotewidth}{0.99\textwidth}
\tablecols{17}
\setlength{\tabcolsep}{0.778\tabcolsep}
\casitiny
\begin{tabular}{clcccccccclcccccc}
\toprule
Code &amp; \multicolumn{1}{c}{Species} &amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) &amp;  &amp; Code &amp; \multicolumn{1}{c}{Species} 
&amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) \\  
\cmidrule{1-8}
\cmidrule{10-17}
~6.01 &amp; C II   &amp; ~~~4 &amp; 3918.97 &amp; $-$0.53 &amp; WF &amp; ~16 &amp; $-$3.12 &amp;  &amp; 24.01 &amp; Cr II  &amp;   30 &amp; 4884.61 &amp; $-$2.08 &amp; MF &amp; 35 &amp; $-$5.20 \\
~6.01 &amp; C II   &amp;  ~~4 &amp; 3920.68 &amp; $-$0.23 &amp; WF &amp; ~23 &amp; $-$3.09 &amp;  &amp; 24.01 &amp; Cr II  &amp; ~190 &amp; 4901.62 &amp; $-$0.83 &amp; KX &amp; 28 &amp; $-$5.28 \\
12.00 &amp; Mg I   &amp;  ~~2 &amp; 5172.68 &amp; $-$0.38 &amp; WS &amp; ~28 &amp; $-$4.98 &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5232.50 &amp; $-$2.09 &amp; KX &amp; 34 &amp; $-$5.08 \\
12.00 &amp; Mg I   &amp;  ~~2 &amp; 5183.60 &amp; $-$0.16 &amp; WS &amp; ~41 &amp; $-$4.93 &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~23 &amp; 5246.77 &amp; $-$2.45 &amp; MF &amp; 25 &amp; $-$5.14 \\
12.01 &amp; Mg II  &amp;  ~~5 &amp; 3848.21 &amp; $-$1.59 &amp; WS &amp; ~31 &amp; $-$4.42 &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~23 &amp; 5249.44 &amp; $-$2.43 &amp; KX &amp; 25 &amp; $-$5.16 \\
12.01 &amp; Mg II  &amp;  ~10 &amp; 4390.57 &amp; $-$0.53 &amp; WS &amp; ~50 &amp; $-$4.65 &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5308.44 &amp; $-$1.81 &amp; MF &amp; 46 &amp; $-$5.02 \\
12.01 &amp; Mg II  &amp;  ~~9 &amp; 4427.99 &amp; $-$1.21 &amp; WS &amp; ~18 &amp; $-$4.55 &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5310.70 &amp; $-$2.28 &amp; MF &amp; 29 &amp; $-$5.03 \\
13.01 &amp; Al II  &amp;  ~~2 &amp; 4663.05 &amp; $-$0.28 &amp; FW &amp; ~25 &amp; $-$5.47 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~~2 &amp; 4033.06 &amp; $-$0.62 &amp; MF &amp; 24 &amp; $-$5.29 \\
14.01 &amp; Si II  &amp;  ~~1 &amp; 3853.66 &amp; $-$1.44 &amp; LA &amp; ~64 &amp; $-$4.66 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~~2 &amp; 4034.48 &amp; $-$0.81 &amp; MF &amp; ~9 &amp; $-$5.63 \\
14.01 &amp; Si II  &amp;  ~~1 &amp; 3856.02 &amp; $-$0.49 &amp; LA &amp; 120 &amp; $-$4.78 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~16 &amp; 4754.04 &amp; $-$0.09 &amp; MF &amp; ~3 &amp; $-$5.69 \\
14.01 &amp; Si II  &amp;  ~~1 &amp; 3862.59 &amp; $-$0.74 &amp; LA &amp; ~95 &amp; $-$4.85 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4136.90 &amp; $-$1.29 &amp; KX &amp; 17 &amp; $-$5.49 \\
14.01 &amp; Si II  &amp; 3.01 &amp; 4075.45 &amp; $-$1.40 &amp; SG &amp; ~19 &amp; $-$4.38 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4184.45 &amp; $-$1.95 &amp; KX &amp; 12 &amp; $-$5.01 \\
14.01 &amp; Si II  &amp;  ~~3 &amp; 4130.89 &amp;  ~~0.53 &amp; LA &amp; 123 &amp; $-$4.54 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~7 &amp; 4244.25 &amp; $-$2.39 &amp; KX &amp; ~9 &amp; $-$5.11 \\
14.01 &amp; Si II  &amp;  ~~5 &amp; 5041.02 &amp;  ~~0.29 &amp; SG &amp; ~81 &amp; $-$4.47 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4251.73 &amp; $-$1.06 &amp; KX &amp; 17 &amp; $-$5.69 \\
16.01 &amp; S II   &amp;  ~44 &amp; 4145.06 &amp;  ~~0.23 &amp; KX &amp; ~~6 &amp; $-$4.33 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~2 &amp; 4260.46 &amp; $-$4.25 &amp; KX &amp; 11 &amp; $-$4.94 \\
16.01 &amp; S II   &amp;  ~44 &amp; 4153.07 &amp;  ~~0.62 &amp; WS &amp; ~~8 &amp; $-$4.51 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4478.64 &amp; $-$0.95 &amp; KX &amp; 14 &amp; $-$5.69 \\
16.01 &amp; S II   &amp;  ~44 &amp; 4162.66 &amp;  ~~0.78 &amp; WS &amp; ~13 &amp; $-$4.31 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4702.73 &amp; $-$2.34 &amp; KX &amp; ~9 &amp; $-$4.72 \\
16.01 &amp; S II   &amp;  ~~9 &amp; 4815.55 &amp;  ~~0.18 &amp; WM &amp; ~~6 &amp; $-$4.78 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4730.40 &amp; $-$2.15 &amp; KX &amp; 13 &amp; $-$5.13 \\
16.01 &amp; S II   &amp;  ~~7 &amp; 5032.43 &amp;  ~~0.18 &amp; WS &amp; ~12 &amp; $-$4.30 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4755.72 &amp; $-$1.24 &amp; KX &amp; 37 &amp; $-$5.27 \\
20.01 &amp; Ca II  &amp;  ~~1 &amp; 3933.66 &amp;  ~~0.13 &amp; WM &amp; 249 &amp; $-$6.18 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4806.82 &amp; $-$1.56 &amp; KX &amp; 13 &amp; $-$5.69 \\
21.01 &amp; Sc II  &amp;  ~~7 &amp; 4246.82 &amp;  ~~0.24 &amp; LD &amp; ~89 &amp; $-$7.03 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 5177.65 &amp; $-$1.77 &amp; KX &amp; 18 &amp; $-$4.97 \\
22.01 &amp; Ti II  &amp;  ~34 &amp; 3900.54 &amp; $-$0.45 &amp; MF &amp; ~75 &amp; $-$6.13 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4238.79 &amp; $-$3.63 &amp; KX &amp; 14 &amp; $-$5.43 \\
22.01 &amp; Ti II  &amp;  ~34 &amp; 3913.46 &amp; $-$0.53 &amp; MF &amp; ~75 &amp; $-$6.07 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~45 &amp; 3815.84 &amp;  ~~0.23 &amp; N4 &amp; 31 &amp; $-$4.79 \\
22.01 &amp; Ti II  &amp;  ~31 &amp; 3932.02 &amp; $-$1.78 &amp; MF &amp; ~33 &amp; $-$6.08 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~~4 &amp; 3859.91 &amp; $-$0.71 &amp; N4 &amp; 27 &amp; $-$4.73 \\
22.01 &amp; Ti II  &amp;  ~87 &amp; 4028.34 &amp; $-$1.00 &amp; MF &amp; ~42 &amp; $-$6.25 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~43 &amp; 4132.06 &amp; $-$0.68 &amp; N4 &amp; 26 &amp; $-$3.96 \\
22.01 &amp; Ti II  &amp;  105 &amp; 4163.64 &amp; $-$0.40 &amp; MF &amp; ~57 &amp; $-$6.05 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~152 &amp; 4187.04 &amp; $-$0.55 &amp; N4 &amp; 19 &amp; $-$3.87 \\
22.01 &amp; Ti II  &amp;  ~33 &amp; 4227.33 &amp; $-$2.36 &amp; KX &amp; ~11 &amp; $-$6.20 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~152 &amp; 4187.80 &amp; $-$0.55 &amp; N4 &amp; 12 &amp; $-$4.13 \\
22.01 &amp; Ti II  &amp;  ~20 &amp; 4287.87 &amp; $-$2.02 &amp; MF &amp; ~26 &amp; $-$6.05 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~152 &amp; 4198.30 &amp; $-$0.72 &amp; N4 &amp; ~7 &amp; $-$4.21 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4290.22 &amp; $-$1.12 &amp; MF &amp; ~72 &amp; $-$5.62 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~522 &amp; 4199.10 &amp;  ~~0.16 &amp; N4 &amp; 29 &amp; $-$3.97 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4294.09 &amp; $-$1.11 &amp; MF &amp; ~66 &amp; $-$5.85 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~152 &amp; 4222.21 &amp; $-$0.97 &amp; N4 &amp; ~9 &amp; $-$3.85 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4300.04 &amp; $-$0.77 &amp; MF &amp; ~78 &amp; $-$5.77 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~693 &amp; 4227.43 &amp;  ~~0.27 &amp; N4 &amp; 12 &amp; $-$4.50 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4301.92 &amp; $-$1.16 &amp; MF &amp; ~51 &amp; $-$6.24 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~152 &amp; 4250.12 &amp; $-$0.41 &amp; N4 &amp; 17 &amp; $-$4.07 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4307.87 &amp; $-$1.29 &amp; MF &amp; ~57 &amp; $-$5.92 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~42 &amp; 4250.79 &amp; $-$0.71 &amp; N4 &amp; 15 &amp; $-$4.28 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4312.86 &amp; $-$1.16 &amp; MF &amp; ~50 &amp; $-$6.25 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~42 &amp; 4271.76 &amp; $-$0.16 &amp; N4 &amp; 17 &amp; $-$4.80 \\
22.01 &amp; Ti II  &amp;  104 &amp; 4386.85 &amp; $-$1.26 &amp; MF &amp; ~28 &amp; $-$5.95 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~41 &amp; 4383.54 &amp;  ~~0.20 &amp; N4 &amp; 30 &amp; $-$4.79 \\
22.01 &amp; Ti II  &amp;  ~51 &amp; 4394.06 &amp; $-$1.59 &amp; MF &amp; ~20 &amp; $-$6.58 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~41 &amp; 4404.75 &amp; $-$0.14 &amp; N4 &amp; 22 &amp; $-$4.64 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4395.03 &amp; $-$0.66 &amp; MF &amp; ~73 &amp; $-$6.07 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~554 &amp; 4736.77 &amp; $-$0.75 &amp; N4 &amp; ~6 &amp; $-$3.84 \\
22.01 &amp; Ti II  &amp;  ~61 &amp; 4395.84 &amp; $-$2.17 &amp; MF &amp; ~14 &amp; $-$6.19 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~318 &amp; 4920.50 &amp;  ~~0.07 &amp; N4 &amp; 13 &amp; $-$4.47 \\
22.01 &amp; Ti II  &amp;  ~61 &amp; 4409.52 &amp; $-$2.57 &amp; KX &amp; ~12 &amp; $-$5.89 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~383 &amp; 5232.94 &amp; $-$0.06 &amp; N4 &amp; 24 &amp; $-$3.93 \\
22.01 &amp; Ti II  &amp;  115 &amp; 4411.07 &amp; $-$1.06 &amp; MF &amp; ~20 &amp; $-$6.11 &amp;  &amp; 26.00 &amp; Fe I   &amp; 1146 &amp; 5383.37 &amp;  ~~0.65 &amp; N4 &amp; 11 &amp; $-$4.39 \\
22.01 &amp; Ti II  &amp;  ~40 &amp; 4417.71 &amp; $-$1.43 &amp; MF &amp; ~46 &amp; $-$6.10 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~686 &amp; 5586.76 &amp; $-$0.14 &amp; N4 &amp; 15 &amp; $-$3.89 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4450.48 &amp; $-$1.45 &amp; MF &amp; ~32 &amp; $-$6.46 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~127 &amp; 3845.18 &amp; $-$2.29 &amp; KX &amp; 17 &amp; $-$4.73 \\
22.01 &amp; Ti II  &amp;  ~31 &amp; 4468.49 &amp; $-$0.60 &amp; MF &amp; ~68 &amp; $-$6.28 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~29 &amp; 3872.77 &amp; $-$3.32 &amp; KX &amp; 31 &amp; $-$4.18 \\
22.01 &amp; Ti II  &amp;  ~31 &amp; 4501.27 &amp; $-$0.75 &amp; MF &amp; ~65 &amp; $-$6.25 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~173 &amp; 3906.04 &amp; $-$1.83 &amp; N4 &amp; 32 &amp; $-$4.22 \\
22.01 &amp; Ti II  &amp;  ~50 &amp; 4533.96 &amp; $-$0.77 &amp; MF &amp; ~80 &amp; $-$5.63 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~38 &amp; 3935.96 &amp; $-$1.86 &amp; N4 &amp; 36 &amp; $-$4.05 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4563.76 &amp; $-$0.96 &amp; MF &amp; ~64 &amp; $-$6.02 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~~3 &amp; 3938.29 &amp; $-$4.07 &amp; N4 &amp; 21 &amp; $-$4.24 \\
22.01 &amp; Ti II  &amp;  ~82 &amp; 4571.97 &amp; $-$0.53 &amp; MF &amp; ~73 &amp; $-$5.95 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~190 &amp; 3938.97 &amp; $-$1.85 &amp; N4 &amp; 24 &amp; $-$4.26 \\
22.01 &amp; Ti II  &amp;  ~59 &amp; 4657.20 &amp; $-$2.15 &amp; MF &amp; ~18 &amp; $-$6.07 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~28 &amp; 4122.67 &amp; $-$3.38 &amp; N4 &amp; 25 &amp; $-$4.36 \\
22.01 &amp; Ti II  &amp;  ~92 &amp; 4779.98 &amp; $-$1.37 &amp; MF &amp; ~26 &amp; $-$6.20 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~27 &amp; 4233.17 &amp; $-$1.81 &amp; N4 &amp; 87 &amp; $-$4.05 \\
22.01 &amp; Ti II  &amp;  ~82 &amp; 4805.09 &amp; $-$1.10 &amp; MF &amp; ~40 &amp; $-$6.11 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~27 &amp; 4273.33 &amp; $-$3.34 &amp; N4 &amp; 37 &amp; $-$3.98 \\
22.01 &amp; Ti II  &amp;  114 &amp; 4874.01 &amp; $-$0.79 &amp; MF &amp; ~18 &amp; $-$6.45 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~28 &amp; 4296.57 &amp; $-$3.01 &amp; N4 &amp; 46 &amp; $-$4.06 \\
22.01 &amp; Ti II  &amp;  114 &amp; 4911.20 &amp; $-$0.34 &amp; MF &amp; ~29 &amp; $-$6.57 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~27 &amp; 4303.18 &amp; $-$2.61 &amp; N4 &amp; 53 &amp; $-$4.27 \\
22.01 &amp; Ti II  &amp;  ~86 &amp; 5129.16 &amp; $-$1.39 &amp; MF &amp; ~26 &amp; $-$6.25 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~27 &amp; 4351.77 &amp; $-$2.08 &amp; N4 &amp; 58 &amp; $-$4.64 \\
22.01 &amp; Ti II  &amp;  ~86 &amp; 5185.90 &amp; $-$1.35 &amp; MF &amp; ~36 &amp; $-$6.04 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~~J &amp; 4357.58 &amp; $-$2.10 &amp; KX &amp; ~8 &amp; $-$4.52 \\
22.01 &amp; Ti II  &amp;  ~~7 &amp; 5188.69 &amp; $-$1.21 &amp; MF &amp; ~43 &amp; $-$6.16 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~27 &amp; 4385.39 &amp; $-$2.57 &amp; N4 &amp; 52 &amp; $-$4.28 \\
24.00 &amp; Cr I   &amp;  ~~7 &amp; 5208.43 &amp;  ~~0.16 &amp; MF &amp; ~21 &amp; $-$5.20 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~27 &amp; 4416.83 &amp; $-$2.60 &amp; N4 &amp; 43 &amp; $-$4.52 \\
24.01 &amp; Cr II  &amp;  129 &amp; 3911.32 &amp; $-$2.06 &amp; KX &amp; ~17 &amp; $-$5.18 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~37 &amp; 4489.18 &amp; $-$2.97 &amp; N4 &amp; 40 &amp; $-$4.20 \\
24.01 &amp; Cr II  &amp;  183 &amp; 3979.50 &amp; $-$0.73 &amp; KX &amp; ~44 &amp; $-$5.40 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~37 &amp; 4491.40 &amp; $-$2.70 &amp; N4 &amp; 39 &amp; $-$4.49 \\
24.01 &amp; Cr II  &amp;  ~19 &amp; 4051.93 &amp; $-$2.19 &amp; KX &amp; ~41 &amp; $-$5.34 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~38 &amp; 4508.29 &amp; $-$2.21 &amp; N4 &amp; 52 &amp; $-$4.60 \\
24.01 &amp; Cr II  &amp;  ~26 &amp; 4072.56 &amp; $-$2.41 &amp; KX &amp; ~36 &amp; $-$4.94 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~37 &amp; 4515.34 &amp; $-$2.48 &amp; N4 &amp; 55 &amp; $-$4.23 \\
24.01 &amp; Cr II  &amp;  165 &amp; 4082.28 &amp; $-$1.23 &amp; KX &amp; ~25 &amp; $-$5.60 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~37 &amp; 4520.22 &amp; $-$2.60 &amp; N4 &amp; 41 &amp; $-$4.55 \\
24.01 &amp; Cr II  &amp;  ~26 &amp; 4132.42 &amp; $-$2.35 &amp; KX &amp; ~13 &amp; $-$5.64 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~38 &amp; 4522.63 &amp; $-$2.03 &amp; N4 &amp; 58 &amp; $-$4.60 \\
24.01 &amp; Cr II  &amp;  162 &amp; 4145.78 &amp; $-$1.16 &amp; KX &amp; ~45 &amp; $-$5.09 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~38 &amp; 4541.52 &amp; $-$3.05 &amp; N4 &amp; 29 &amp; $-$4.41 \\
24.01 &amp; Cr II  &amp;  ~26 &amp; 4179.42 &amp; $-$1.77 &amp; KX &amp; ~39 &amp; $-$5.44 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~37 &amp; 4555.89 &amp; $-$2.29 &amp; N4 &amp; 52 &amp; $-$4.52 \\
24.01 &amp; Cr II  &amp;  ~31 &amp; 4275.57 &amp; $-$1.70 &amp; KX &amp; ~56 &amp; $-$4.98 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~38 &amp; 4576.34 &amp; $-$3.04 &amp; N4 &amp; 30 &amp; $-$4.41 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4554.99 &amp; $-$1.38 &amp; MF &amp; ~62 &amp; $-$5.01 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~37 &amp; 4582.84 &amp; $-$3.10 &amp; N4 &amp; 22 &amp; $-$4.56 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4588.20 &amp; $-$0.63 &amp; MF &amp; ~87 &amp; $-$4.97 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~38 &amp; 4583.84 &amp; $-$2.02 &amp; N4 &amp; 75 &amp; $-$4.11 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4592.05 &amp; $-$1.22 &amp; MF &amp; ~63 &amp; $-$5.14 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~~D &amp; 4596.02 &amp; $-$1.84 &amp; N4 &amp; 18 &amp; $-$4.25 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4616.63 &amp; $-$1.29 &amp; MF &amp; ~63 &amp; $-$5.08 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~38 &amp; 4620.52 &amp; $-$3.28 &amp; N4 &amp; 22 &amp; $-$4.38 \\
24.01 &amp; Cr II  &amp;  178 &amp; 4697.60 &amp; $-$1.88 &amp; MF &amp; ~15 &amp; $-$5.07 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~37 &amp; 4629.34 &amp; $-$2.37 &amp; N4 &amp; 66 &amp; $-$4.01 \\
24.01 &amp; Cr II  &amp;  ~30 &amp; 4812.34 &amp; $-$1.80 &amp; MF &amp; ~42 &amp; $-$5.29 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~186 &amp; 4635.32 &amp; $-$1.65 &amp; N4 &amp; 32 &amp; $-$4.12 \\
24.01 &amp; Cr II  &amp;  ~30 &amp; 4848.23 &amp; $-$1.14 &amp; MF &amp; ~65 &amp; $-$5.26 &amp;  &amp; 26.01 &amp; Fe II  &amp; ~~28 &amp; 4666.76 &amp; $-$3.33 &amp; N4 &amp; 18 &amp; $-$4.47 \\
\bottomrule
\end{tabular}
\end{table*}


%%%%% CONTINUA TABLA 9

\setcounter{table}{8} 
\begin{table*}[!t]
\vspace{0.1cm}
\centering
\centerline{TABLE~9 (CONTINUED)\smallskip}
\setlength{\tabnotewidth}{0.99\textwidth}
\tablecols{17}
\setlength{\tabcolsep}{0.778\tabcolsep}
\casitiny
\begin{tabular}{clcccccccclcccccc}
\toprule
Code &amp; \multicolumn{1}{c}{Species} &amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) &amp;  &amp; Code &amp; \multicolumn{1}{c}{Species} 
&amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) \\  
\cmidrule{1-8}
\cmidrule{10-17}
26.01 &amp; Fe II  &amp; 43 &amp; 4731.45 &amp; $-$3.13 &amp; N4 &amp; ~27 &amp; $-$4.37 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5291.67 &amp;  ~~0.58 &amp; KX &amp; 22 &amp; $-$4.37 \\
26.01 &amp; Fe II  &amp; ~J &amp; 4826.68 &amp; $-$0.44 &amp; KX &amp; ~~5 &amp; $-$4.40 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~~J &amp; 5339.59 &amp;  ~~0.54 &amp; KX &amp; 25 &amp; $-$4.22 \\
26.01 &amp; Fe II  &amp; ~J &amp; 4951.58 &amp;  ~~0.18 &amp; KX &amp; ~14 &amp; $-$4.44 &amp;  &amp; 28.01 &amp; Ni II  &amp;  ~11 &amp; 3849.55 &amp; $-$1.88 &amp; KX &amp; 21 &amp; $-$5.85 \\
26.01 &amp; Fe II  &amp; ~J &amp; 4984.47 &amp;  ~~0.01 &amp; KX &amp; ~12 &amp; $-$4.32 &amp;  &amp; 28.01 &amp; Ni II  &amp;  ~11 &amp; 4067.03 &amp; $-$1.29 &amp; KX &amp; 26 &amp; $-$6.27 \\
26.01 &amp; Fe II  &amp; ~J &amp; 4990.51 &amp;  ~~0.18 &amp; KX &amp; ~15 &amp; $-$4.35 &amp;  &amp; 38.01 &amp; Sr II  &amp;  ~~1 &amp; 4215.52 &amp; $-$0.17 &amp; WM &amp; 35 &amp; $-$8.43 \\
26.01 &amp; Fe II  &amp; ~J &amp; 4993.36 &amp; $-$3.65 &amp; MF &amp; ~10 &amp; $-$4.49 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~~6 &amp; 3950.35 &amp; $-$0.49 &amp; HL &amp; 65 &amp; $-$6.35 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5001.96 &amp;  ~~0.90 &amp; KX &amp; ~39 &amp; $-$4.34 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~~6 &amp; 3982.59 &amp; $-$0.49 &amp; HL &amp; 62 &amp; $-$6.47 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5004.20 &amp;  ~~0.50 &amp; KX &amp; ~22 &amp; $-$4.43 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~14 &amp; 4124.90 &amp; $-$1.50 &amp; HL &amp; 42 &amp; $-$6.20 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5018.44 &amp; $-$1.22 &amp; MF &amp; 106 &amp; $-$4.04 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~~5 &amp; 4422.58 &amp; $-$1.27 &amp; HL &amp; 53 &amp; $-$6.13 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5035.71 &amp;  ~~0.61 &amp; KX &amp; ~28 &amp; $-$4.34 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~22 &amp; 4854.86 &amp; $-$0.38 &amp; HL &amp; 48 &amp; $-$6.80 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5045.11 &amp; $-$0.13 &amp; KX &amp; ~~8 &amp; $-$4.40 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~22 &amp; 4900.12 &amp; $-$0.09 &amp; HL &amp; 74 &amp; $-$5.99 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5061.72 &amp;  ~~0.22 &amp; KX &amp; ~12 &amp; $-$4.52 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~20 &amp; 4982.13 &amp; $-$1.29 &amp; HL &amp; 30 &amp; $-$6.51 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5070.90 &amp;  ~~0.24 &amp; KX &amp; ~13 &amp; $-$4.50 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~20 &amp; 5200.41 &amp; $-$0.57 &amp; HL &amp; 59 &amp; $-$6.10 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5075.76 &amp;  ~~0.28 &amp; KX &amp; ~17 &amp; $-$4.29 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~20 &amp; 5289.82 &amp; $-$1.85 &amp; HL &amp; 20 &amp; $-$6.30 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5082.23 &amp; $-$0.10 &amp; KX &amp; ~~9 &amp; $-$4.33 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~17 &amp; 3915.96 &amp; $-$0.82 &amp; KX &amp; 28 &amp; $-$7.22 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5093.58 &amp;  ~~0.11 &amp; KX &amp; ~21 &amp; $-$4.00 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~16 &amp; 3958.23 &amp; $-$0.31 &amp; KX &amp; 44 &amp; $-$7.14 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5097.27 &amp;  ~~0.31 &amp; KX &amp; ~32 &amp; $-$3.85 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~30 &amp; 3991.15 &amp; $-$0.25 &amp; KX &amp; 45 &amp; $-$7.07 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5145.77 &amp; $-$0.40 &amp; KX &amp; ~10 &amp; $-$3.93 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~16 &amp; 3998.95 &amp; $-$0.67 &amp; GB &amp; 41 &amp; $-$6.90 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5149.46 &amp;  ~~0.40 &amp; KX &amp; ~25 &amp; $-$4.12 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~54 &amp; 4018.37 &amp; $-$0.99 &amp; KX &amp; 12 &amp; $-$7.41 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5160.84 &amp; $-$2.64 &amp; KX &amp; ~10 &amp; $-$4.05 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~42 &amp; 4034.10 &amp; $-$1.55 &amp; BG &amp; ~8 &amp; $-$7.17 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5169.03 &amp; $-$0.87 &amp; MF &amp; 111 &amp; $-$4.31 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~29 &amp; 4090.53 &amp; $-$1.10 &amp; GB &amp; 18 &amp; $-$7.15 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5216.85 &amp;  ~~0.81 &amp; KX &amp; ~22 &amp; $-$4.57 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~41 &amp; 4149.22 &amp; $-$0.03 &amp; BG &amp; 52 &amp; $-$6.94 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5234.62 &amp; $-$2.05 &amp; MF &amp; ~58 &amp; $-$4.34 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~29 &amp; 4156.28 &amp; $-$0.71 &amp; GB &amp; 32 &amp; $-$7.13 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5247.95 &amp;  ~~0.55 &amp; N4 &amp; ~18 &amp; $-$4.44 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~97 &amp; 4186.67 &amp; $-$0.58 &amp; KX &amp; 20 &amp; $-$7.10 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5251.23 &amp;  ~~0.42 &amp; N4 &amp; ~21 &amp; $-$4.22 &amp;  &amp; 40.01 &amp; Zr II  &amp;  ~99 &amp; 4231.67 &amp; $-$1.02 &amp; KX &amp; 13 &amp; $-$6.91 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5254.93 &amp; $-$3.23 &amp; KX &amp; ~19 &amp; $-$4.28 &amp;  &amp; 40.01 &amp; Zr II  &amp;  130 &amp; 4494.42 &amp; $-$0.48 &amp; KX &amp; 20 &amp; $-$6.85 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5257.12 &amp;  ~~0.03 &amp; KX &amp; ~12 &amp; $-$4.20 &amp;  &amp; 40.01 &amp; Zr II  &amp;  129 &amp; 4661.78 &amp; $-$0.80 &amp; KX &amp; 12 &amp; $-$6.83 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5260.25 &amp;  ~~1.07 &amp; KX &amp; ~39 &amp; $-$4.38 &amp;  &amp; 56.01 &amp; Ba II  &amp;  ~~1 &amp; 4934.07 &amp;  ~~0.00 &amp; WM &amp; 10 &amp; $-$9.17 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5272.40 &amp; $-$2.03 &amp; MF &amp; ~14 &amp; $-$4.27 &amp;  &amp; 80.01 &amp; Hg II  &amp;  $-$ &amp; 3983.94 &amp; $-$1.73 &amp; DW &amp; 59 &amp; $-$5.03 \\
26.01 &amp; Fe II  &amp; ~J &amp; 5276.00 &amp; $-$1.94 &amp; MF &amp; ~58 &amp; $-$4.45 &amp;  &amp;       &amp;        &amp;      &amp;         &amp;         &amp;    &amp;    &amp;         \\
\bottomrule
\end{tabular}
\vspace{0.5cm}
\end{table*}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%



%%%%% TABLA 10

\setcounter{table}{9} 
\begin{table*}[!t]
\vspace{0.1cm}
\centering
\caption{Line abundances of HR 8567}
\setlength{\tabnotewidth}{0.99\textwidth}
\tablecols{17}
\setlength{\tabcolsep}{0.778\tabcolsep}
\casitiny
\begin{tabular}{clcccccccclcccccc}
\toprule
Code &amp; \multicolumn{1}{c}{Species} &amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) &amp;  &amp; Code &amp; \multicolumn{1}{c}{Species} 
&amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) \\  
\cmidrule{1-8}
\cmidrule{10-17}
~6.01 &amp; C II   &amp;  ~~4 &amp; 3918.97 &amp; $-$0.53 &amp; WF &amp; ~15 &amp; $-$3.76 &amp;  &amp; 24.01 &amp; Cr II  &amp;   44 &amp; 4616.63 &amp; $-$1.29 &amp; MF &amp; 50 &amp; $-$5.34 \\
~6.01 &amp; C II   &amp;  ~~4 &amp; 3920.68 &amp; $-$0.23 &amp; WF &amp; ~26 &amp; $-$3.53 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~44 &amp; 4634.07 &amp; $-$1.24 &amp; MF &amp; 62 &amp; $-$4.96 \\
~6.01 &amp; C II   &amp;  ~~6 &amp; 4267.26 &amp;  ~~0.72 &amp; WF &amp; ~15 &amp; $-$4.19 &amp;  &amp; 24.01 &amp; Cr II  &amp;  178 &amp; 4697.60 &amp; $-$1.88 &amp; MF &amp; ~9 &amp; $-$5.31 \\
~8.00 &amp; O I    &amp;  ~12 &amp; 5330.73 &amp; $-$0.87 &amp; WF &amp; ~28 &amp; $-$3.09 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~30 &amp; 4812.34 &amp; $-$1.80 &amp; MF &amp; 30 &amp; $-$5.53 \\
12.00 &amp; Mg I   &amp;  ~~2 &amp; 5183.60 &amp; $-$0.16 &amp; WS &amp; ~~8 &amp; $-$5.14 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~30 &amp; 4836.23 &amp; $-$2.25 &amp; MF &amp; 31 &amp; $-$5.06 \\
12.01 &amp; Mg II  &amp;  ~10 &amp; 4390.57 &amp; $-$0.53 &amp; WS &amp; ~31 &amp; $-$4.95 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~30 &amp; 4848.23 &amp; $-$1.14 &amp; MF &amp; 54 &amp; $-$5.46 \\
12.01 &amp; Mg II  &amp;  ~~9 &amp; 4427.99 &amp; $-$1.21 &amp; WS &amp; ~10 &amp; $-$4.88 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~30 &amp; 4884.61 &amp; $-$2.08 &amp; MF &amp; 24 &amp; $-$5.43 \\
13.01 &amp; Al II  &amp;  ~~2 &amp; 4663.05 &amp; $-$0.28 &amp; FW &amp; ~~8 &amp; $-$6.52 &amp;  &amp; 24.01 &amp; Cr II  &amp;  190 &amp; 4912.46 &amp; $-$0.95 &amp; KX &amp; 19 &amp; $-$5.43 \\
14.01 &amp; Si II  &amp;  ~~1 &amp; 3853.66 &amp; $-$1.44 &amp; LA &amp; ~56 &amp; $-$4.99 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~43 &amp; 5232.50 &amp; $-$2.09 &amp; KX &amp; 21 &amp; $-$5.42 \\
14.01 &amp; Si II  &amp;  ~~1 &amp; 3856.02 &amp; $-$0.49 &amp; LA &amp; 107 &amp; $-$4.89 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~43 &amp; 5237.33 &amp; $-$1.16 &amp; MF &amp; 59 &amp; $-$5.11 \\
14.01 &amp; Si II  &amp;  ~~1 &amp; 3862.59 &amp; $-$0.74 &amp; LA &amp; ~88 &amp; $-$4.98 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~23 &amp; 5249.44 &amp; $-$2.43 &amp; KX &amp; 16 &amp; $-$5.40 \\
14.01 &amp; Si II  &amp; 3.01 &amp; 4075.45 &amp; $-$1.40 &amp; SG &amp; ~16 &amp; $-$4.72 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~43 &amp; 5274.96 &amp; $-$1.29 &amp; KX &amp; 49 &amp; $-$5.35 \\
14.01 &amp; Si II  &amp; 3.01 &amp; 4076.78 &amp; $-$1.67 &amp; SG &amp; ~19 &amp; $-$4.35 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~43 &amp; 5308.44 &amp; $-$1.81 &amp; MF &amp; 37 &amp; $-$5.19 \\
14.01 &amp; Si II  &amp;  ~~3 &amp; 4130.89 &amp;  ~~0.53 &amp; LA &amp; 114 &amp; $-$4.73 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~43 &amp; 5310.70 &amp; $-$2.28 &amp; MF &amp; 20 &amp; $-$5.25 \\
14.01 &amp; Si II  &amp;  ~~5 &amp; 5041.02 &amp;  ~~0.29 &amp; SG &amp; ~73 &amp; $-$4.77 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~43 &amp; 5313.59 &amp; $-$1.65 &amp; MF &amp; 43 &amp; $-$5.18 \\
16.01 &amp; S II   &amp;  ~44 &amp; 4153.07 &amp;  ~~0.62 &amp; WS &amp; ~12 &amp; $-$4.79 &amp;  &amp; 24.01 &amp; Cr II  &amp;  ~43 &amp; 5334.87 &amp; $-$1.56 &amp; KX &amp; 40 &amp; $-$5.37 \\
16.01 &amp; S II   &amp;  ~44 &amp; 4162.66 &amp;  ~~0.78 &amp; WS &amp; ~14 &amp; $-$4.82 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~~2 &amp; 4030.75 &amp; $-$0.47 &amp; MF &amp; 31 &amp; $-$4.50 \\
16.01 &amp; S II   &amp;  ~~9 &amp; 4815.55 &amp;  ~~0.18 &amp; WM &amp; ~13 &amp; $-$4.93 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~~2 &amp; 4033.06 &amp; $-$0.62 &amp; MF &amp; 49 &amp; $-$3.76 \\
16.01 &amp; S II   &amp;  ~~1 &amp; 4991.97 &amp; $-$0.65 &amp; WS &amp; ~~7 &amp; $-$4.45 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~~2 &amp; 4034.48 &amp; $-$0.81 &amp; MF &amp; 16 &amp; $-$4.63 \\
16.01 &amp; S II   &amp;  ~15 &amp; 5014.04 &amp;  ~~0.03 &amp; KX &amp; ~14 &amp; $-$4.47 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~~5 &amp; 4035.72 &amp; $-$0.19 &amp; KX &amp; 12 &amp; $-$4.33 \\
16.01 &amp; S II   &amp;  ~~7 &amp; 5032.43 &amp;  ~~0.18 &amp; WS &amp; ~15 &amp; $-$4.71 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~~5 &amp; 4041.35 &amp;  ~~0.29 &amp; MF &amp; 30 &amp; $-$4.25 \\
16.01 &amp; S II   &amp;  ~39 &amp; 5212.62 &amp;  ~~0.24 &amp; WS &amp; ~~4 &amp; $-$4.93 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~~5 &amp; 4058.93 &amp; $-$0.45 &amp; MF &amp; ~8 &amp; $-$4.25 \\
20.01 &amp; Ca II  &amp;  ~~1 &amp; 3933.66 &amp;  ~~0.13 &amp; WM &amp; 280 &amp; $-$5.35 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~23 &amp; 4235.14 &amp; $-$0.26 &amp; KX &amp; 14 &amp; $-$3.81 \\
21.01 &amp; Sc II  &amp;  ~~7 &amp; 4246.82 &amp;  ~~0.24 &amp; LD &amp; ~54 &amp; $-$7.61 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~28 &amp; 4455.01 &amp; $-$0.39 &amp; KX &amp; 11 &amp; $-$3.76 \\
22.01 &amp; Ti II  &amp;  ~34 &amp; 3900.54 &amp; $-$0.45 &amp; MF &amp; ~66 &amp; $-$5.97 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~28 &amp; 4462.03 &amp;  ~~0.32 &amp; MF &amp; 11 &amp; $-$4.46 \\
22.01 &amp; Ti II  &amp;  ~34 &amp; 3913.46 &amp; $-$0.53 &amp; MF &amp; ~70 &amp; $-$5.78 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~22 &amp; 4470.14 &amp; $-$0.44 &amp; MF &amp; ~5 &amp; $-$4.16 \\
22.01 &amp; Ti II  &amp;  ~31 &amp; 3932.02 &amp; $-$1.78 &amp; MF &amp; ~23 &amp; $-$5.99 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~21 &amp; 4709.71 &amp; $-$0.34 &amp; MF &amp; ~6 &amp; $-$4.14 \\
22.01 &amp; Ti II  &amp;  ~87 &amp; 4028.34 &amp; $-$1.00 &amp; MF &amp; ~31 &amp; $-$6.19 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~16 &amp; 4754.04 &amp; $-$0.09 &amp; MF &amp; 14 &amp; $-$4.32 \\
22.01 &amp; Ti II  &amp;  105 &amp; 4163.64 &amp; $-$0.40 &amp; MF &amp; ~48 &amp; $-$5.96 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~21 &amp; 4761.51 &amp; $-$0.14 &amp; MF &amp; ~8 &amp; $-$4.20 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4290.22 &amp; $-$1.12 &amp; MF &amp; ~54 &amp; $-$5.74 &amp;  &amp; 25.00 &amp; Mn I   &amp;  ~16 &amp; 4783.43 &amp;  ~~0.04 &amp; MF &amp; 17 &amp; $-$4.30 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4294.09 &amp; $-$1.11 &amp; MF &amp; ~61 &amp; $-$5.55 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 3878.99 &amp; $-$1.71 &amp; KX &amp; 55 &amp; $-$4.16 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4301.92 &amp; $-$1.16 &amp; MF &amp; ~35 &amp; $-$6.28 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 3917.32 &amp; $-$1.15 &amp; KX &amp; 43 &amp; $-$4.47 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4312.86 &amp; $-$1.16 &amp; MF &amp; ~43 &amp; $-$6.04 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 3930.95 &amp; $-$2.15 &amp; KX &amp; 23 &amp; $-$4.29 \\
22.01 &amp; Ti II  &amp;  ~94 &amp; 4316.79 &amp; $-$1.42 &amp; MF &amp; ~11 &amp; $-$6.31 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 3952.42 &amp; $-$1.50 &amp; KX &amp; 23 &amp; $-$4.35 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4320.95 &amp; $-$1.87 &amp; MF &amp; ~38 &amp; $-$5.49 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 3986.58 &amp; $-$2.60 &amp; KX &amp; 28 &amp; $-$4.20 \\
22.01 &amp; Ti II  &amp;  104 &amp; 4386.85 &amp; $-$1.26 &amp; MF &amp; ~29 &amp; $-$5.62 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 3995.31 &amp; $-$2.44 &amp; KX &amp; 24 &amp; $-$4.52 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4395.03 &amp; $-$0.66 &amp; MF &amp; ~65 &amp; $-$5.83 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4000.05 &amp; $-$1.21 &amp; KX &amp; 40 &amp; $-$4.11 \\
22.01 &amp; Ti II  &amp;  ~61 &amp; 4395.84 &amp; $-$2.17 &amp; MF &amp; ~14 &amp; $-$5.86 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4081.44 &amp; $-$2.24 &amp; KX &amp; 41 &amp; $-$3.83 \\
22.01 &amp; Ti II  &amp;  115 &amp; 4411.07 &amp; $-$1.06 &amp; MF &amp; ~20 &amp; $-$5.84 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4087.91 &amp; $-$2.91 &amp; KX &amp; 12 &amp; $-$4.47 \\
22.01 &amp; Ti II  &amp;  ~40 &amp; 4417.71 &amp; $-$1.43 &amp; MF &amp; ~40 &amp; $-$5.88 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4140.44 &amp; $-$2.46 &amp; KX &amp; 26 &amp; $-$4.35 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4443.80 &amp; $-$0.70 &amp; MF &amp; ~58 &amp; $-$6.06 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~2 &amp; 4174.32 &amp; $-$3.55 &amp; KX &amp; 58 &amp; $-$4.08 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4450.48 &amp; $-$1.45 &amp; MF &amp; ~25 &amp; $-$6.29 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4180.06 &amp; $-$2.83 &amp; KX &amp; 13 &amp; $-$4.46 \\
22.01 &amp; Ti II  &amp;  ~31 &amp; 4468.49 &amp; $-$0.60 &amp; MF &amp; ~61 &amp; $-$6.04 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4184.45 &amp; $-$1.95 &amp; KX &amp; 38 &amp; $-$4.18 \\
22.01 &amp; Ti II  &amp;  115 &amp; 4488.32 &amp; $-$0.82 &amp; MF &amp; ~24 &amp; $-$5.94 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4200.27 &amp; $-$1.74 &amp; KX &amp; 48 &amp; $-$4.06 \\
22.01 &amp; Ti II  &amp;  ~50 &amp; 4533.96 &amp; $-$0.77 &amp; MF &amp; ~65 &amp; $-$5.67 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~2 &amp; 4205.38 &amp; $-$3.38 &amp; KX &amp; 66 &amp; $-$3.92 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4563.76 &amp; $-$0.96 &amp; MF &amp; ~54 &amp; $-$5.86 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4240.39 &amp; $-$2.07 &amp; KX &amp; 40 &amp; $-$4.01 \\
22.01 &amp; Ti II  &amp;  ~59 &amp; 4657.20 &amp; $-$2.15 &amp; MF &amp; ~11 &amp; $-$5.98 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~7 &amp; 4244.25 &amp; $-$2.39 &amp; KX &amp; 44 &amp; $-$3.95 \\
22.01 &amp; Ti II  &amp;  ~92 &amp; 4779.98 &amp; $-$1.37 &amp; MF &amp; ~27 &amp; $-$5.84 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4251.73 &amp; $-$1.06 &amp; KX &amp; 61 &amp; $-$4.29 \\
22.01 &amp; Ti II  &amp;  ~82 &amp; 4805.09 &amp; $-$1.10 &amp; MF &amp; ~32 &amp; $-$5.97 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~2 &amp; 4260.46 &amp; $-$4.25 &amp; KX &amp; 25 &amp; $-$4.41 \\
22.01 &amp; Ti II  &amp;  114 &amp; 4874.01 &amp; $-$0.79 &amp; MF &amp; ~12 &amp; $-$6.38 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4377.74 &amp; $-$2.14 &amp; KX &amp; 29 &amp; $-$4.64 \\
22.01 &amp; Ti II  &amp;  114 &amp; 4911.20 &amp; $-$0.34 &amp; MF &amp; ~27 &amp; $-$6.32 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4391.96 &amp; $-$2.89 &amp; KX &amp; 12 &amp; $-$4.45 \\
22.01 &amp; Ti II  &amp;  113 &amp; 5072.29 &amp; $-$0.75 &amp; MF &amp; ~11 &amp; $-$6.44 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4393.38 &amp; $-$2.32 &amp; KX &amp; 31 &amp; $-$4.36 \\
22.01 &amp; Ti II  &amp;  ~86 &amp; 5129.16 &amp; $-$1.39 &amp; MF &amp; ~21 &amp; $-$6.06 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4403.51 &amp; $-$1.80 &amp; KX &amp; 23 &amp; $-$4.59 \\
22.01 &amp; Ti II  &amp;  ~86 &amp; 5185.90 &amp; $-$1.35 &amp; MF &amp; ~30 &amp; $-$5.84 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4478.64 &amp; $-$0.95 &amp; KX &amp; 56 &amp; $-$4.34 \\
22.01 &amp; Ti II  &amp;  ~~7 &amp; 5188.69 &amp; $-$1.21 &amp; MF &amp; ~35 &amp; $-$5.99 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4497.94 &amp; $-$2.59 &amp; KX &amp; 16 &amp; $-$4.59 \\
22.01 &amp; Ti II  &amp;  ~70 &amp; 5226.54 &amp; $-$1.30 &amp; MF &amp; ~26 &amp; $-$6.15 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4503.20 &amp; $-$2.16 &amp; KX &amp; 26 &amp; $-$4.43 \\
24.01 &amp; Cr II  &amp;  167 &amp; 3865.60 &amp; $-$0.78 &amp; KX &amp; ~50 &amp; $-$5.26 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4509.22 &amp; $-$3.60 &amp; KX &amp; ~8 &amp; $-$3.97 \\
24.01 &amp; Cr II  &amp;  129 &amp; 3911.32 &amp; $-$2.06 &amp; KX &amp; ~13 &amp; $-$5.32 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~17 &amp; 4510.21 &amp; $-$0.72 &amp; KX &amp; 17 &amp; $-$3.98 \\
24.01 &amp; Cr II  &amp;  183 &amp; 3979.50 &amp; $-$0.73 &amp; KX &amp; ~36 &amp; $-$5.58 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4689.55 &amp; $-$2.54 &amp; KX &amp; 24 &amp; $-$4.02 \\
24.01 &amp; Cr II  &amp;  ~19 &amp; 4051.93 &amp; $-$2.19 &amp; KX &amp; ~30 &amp; $-$5.55 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4702.73 &amp; $-$2.34 &amp; KX &amp; 15 &amp; $-$4.50 \\
24.01 &amp; Cr II  &amp;  ~26 &amp; 4072.56 &amp; $-$2.41 &amp; KX &amp; ~25 &amp; $-$5.16 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4717.26 &amp; $-$1.86 &amp; KX &amp; 27 &amp; $-$4.43 \\
24.01 &amp; Cr II  &amp;  165 &amp; 4082.28 &amp; $-$1.23 &amp; KX &amp; ~16 &amp; $-$5.83 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4730.40 &amp; $-$2.15 &amp; KX &amp; 52 &amp; $-$3.90 \\
24.01 &amp; Cr II  &amp;  ~26 &amp; 4086.13 &amp; $-$2.42 &amp; KX &amp; ~15 &amp; $-$5.48 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4749.11 &amp; $-$2.00 &amp; KX &amp; 23 &amp; $-$4.57 \\
24.01 &amp; Cr II  &amp;  181 &amp; 4127.06 &amp; $-$1.77 &amp; KX &amp; ~10 &amp; $-$5.40 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4791.78 &amp; $-$1.72 &amp; KX &amp; 41 &amp; $-$4.28 \\
24.01 &amp; Cr II  &amp;  ~26 &amp; 4132.42 &amp; $-$2.35 &amp; KX &amp; ~15 &amp; $-$5.54 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4806.82 &amp; $-$1.56 &amp; KX &amp; 66 &amp; $-$3.93 \\
24.01 &amp; Cr II  &amp;  ~26 &amp; 4179.42 &amp; $-$1.77 &amp; KX &amp; ~29 &amp; $-$5.63 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4830.06 &amp; $-$1.85 &amp; KX &amp; 39 &amp; $-$4.23 \\
24.01 &amp; Cr II  &amp;  ~31 &amp; 4275.57 &amp; $-$1.70 &amp; KX &amp; ~51 &amp; $-$5.02 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4839.74 &amp; $-$1.86 &amp; KX &amp; 32 &amp; $-$4.43 \\
24.01 &amp; Cr II  &amp;  191 &amp; 4465.73 &amp; $-$1.18 &amp; KX &amp; ~~9 &amp; $-$5.65 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 4842.32 &amp; $-$2.01 &amp; KX &amp; 39 &amp; $-$4.05 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4554.99 &amp; $-$1.38 &amp; MF &amp; ~50 &amp; $-$5.25 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 5102.52 &amp; $-$1.93 &amp; KX &amp; 48 &amp; $-$3.91 \\
24.01 &amp; Cr II  &amp;  ~39 &amp; 4565.74 &amp; $-$2.11 &amp; MF &amp; ~33 &amp; $-$5.08 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 5307.35 &amp; $-$2.07 &amp; KX &amp; 17 &amp; $-$4.25 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4588.20 &amp; $-$0.63 &amp; MF &amp; ~80 &amp; $-$4.96 &amp;  &amp; 25.01 &amp; Mn II  &amp;  ~~I &amp; 3902.36 &amp; $-$2.72 &amp; KX &amp; 13 &amp; $-$4.53 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4592.05 &amp; $-$1.22 &amp; MF &amp; ~54 &amp; $-$5.28 &amp;  &amp; 26.00 &amp; Fe I   &amp;  ~~4 &amp; 3859.91 &amp; $-$0.71 &amp; N4 &amp; 10 &amp; $-$4.68 \\
\bottomrule
\end{tabular}
\end{table*}


%%%%% CONTINUA TABLA 10

\setcounter{table}{9} 
\begin{table*}[!t]
\vspace{0.1cm}
\centering
\centerline{TABLE~10 (CONTINUED)\smallskip}
\setlength{\tabnotewidth}{0.99\textwidth}
\tablecols{17}
\setlength{\tabcolsep}{0.778\tabcolsep}
\casitiny
\begin{tabular}{clcccccccclcccccc}
\toprule
Code &amp; \multicolumn{1}{c}{Species} &amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) &amp;  &amp; Code &amp; \multicolumn{1}{c}{Species} 
&amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) \\  
\cmidrule{1-8}
\cmidrule{10-17}
26.00 &amp; Fe I   &amp;  ~20 &amp; 3872.50 &amp; $-$0.93 &amp; N4 &amp; ~3 &amp; $-$4.54 &amp;  &amp; 26.01 &amp; Fe II  &amp;   J &amp; 5018.44 &amp; $-$1.22 &amp; MF &amp; 77 &amp; $-$4.68 \\
26.00 &amp; Fe I   &amp;  ~41 &amp; 4383.54 &amp;  ~~0.20 &amp; N4 &amp; ~6 &amp; $-$5.10 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5022.79 &amp; $-$0.02 &amp; KX &amp; ~8 &amp; $-$4.78 \\
26.01 &amp; Fe II  &amp;  127 &amp; 3845.18 &amp; $-$2.29 &amp; KX &amp; ~8 &amp; $-$5.24 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5032.71 &amp;  ~~0.11 &amp; KX &amp; 14 &amp; $-$4.52 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 3935.96 &amp; $-$1.86 &amp; N4 &amp; 12 &amp; $-$4.96 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5035.71 &amp;  ~~0.61 &amp; KX &amp; 21 &amp; $-$4.79 \\
26.01 &amp; Fe II  &amp;  190 &amp; 3938.97 &amp; $-$1.85 &amp; N4 &amp; 11 &amp; $-$4.88 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5061.72 &amp;  ~~0.22 &amp; KX &amp; ~7 &amp; $-$5.06 \\
26.01 &amp; Fe II  &amp;  ~28 &amp; 4122.67 &amp; $-$3.38 &amp; N4 &amp; ~9 &amp; $-$4.99 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5070.90 &amp;  ~~0.24 &amp; KX &amp; ~6 &amp; $-$5.16 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4273.33 &amp; $-$3.34 &amp; N4 &amp; ~8 &amp; $-$5.02 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5075.76 &amp;  ~~0.28 &amp; KX &amp; ~8 &amp; $-$4.95 \\
26.01 &amp; Fe II  &amp;  ~28 &amp; 4296.57 &amp; $-$3.01 &amp; N4 &amp; 15 &amp; $-$5.03 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5082.23 &amp; $-$0.10 &amp; KX &amp; ~5 &amp; $-$4.80 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4303.18 &amp; $-$2.61 &amp; N4 &amp; 46 &amp; $-$4.47 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5093.58 &amp;  ~~0.11 &amp; KX &amp; 11 &amp; $-$4.64 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4351.77 &amp; $-$2.08 &amp; N4 &amp; 35 &amp; $-$5.35 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5145.77 &amp; $-$0.40 &amp; KX &amp; ~5 &amp; $-$4.49 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4385.39 &amp; $-$2.57 &amp; N4 &amp; 28 &amp; $-$5.03 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5149.46 &amp;  ~~0.40 &amp; KX &amp; 14 &amp; $-$4.76 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4416.83 &amp; $-$2.60 &amp; N4 &amp; 26 &amp; $-$5.05 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5150.49 &amp; $-$0.12 &amp; KX &amp; ~9 &amp; $-$4.50 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4489.18 &amp; $-$2.97 &amp; N4 &amp; 18 &amp; $-$4.89 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5169.03 &amp; $-$0.87 &amp; MF &amp; 81 &amp; $-$4.89 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4491.40 &amp; $-$2.70 &amp; N4 &amp; 18 &amp; $-$5.16 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5199.12 &amp;  ~~0.10 &amp; KX &amp; ~5 &amp; $-$5.08 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4508.29 &amp; $-$2.21 &amp; N4 &amp; 32 &amp; $-$5.23 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5203.64 &amp; $-$0.05 &amp; KX &amp; ~6 &amp; $-$4.81 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4515.34 &amp; $-$2.48 &amp; N4 &amp; 26 &amp; $-$5.14 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5216.85 &amp;  ~~0.81 &amp; KX &amp; 17 &amp; $-$5.00 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4520.22 &amp; $-$2.60 &amp; N4 &amp; 22 &amp; $-$5.15 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5234.62 &amp; $-$2.05 &amp; MF &amp; 37 &amp; $-$5.02 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4522.63 &amp; $-$2.03 &amp; N4 &amp; 40 &amp; $-$5.17 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5247.95 &amp;  ~~0.55 &amp; N4 &amp; 22 &amp; $-$4.55 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4541.52 &amp; $-$3.05 &amp; N4 &amp; 13 &amp; $-$4.98 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5260.25 &amp;  ~~1.07 &amp; KX &amp; 30 &amp; $-$4.84 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4555.89 &amp; $-$2.29 &amp; N4 &amp; 34 &amp; $-$5.10 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5272.40 &amp; $-$2.03 &amp; MF &amp; 14 &amp; $-$4.46 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4576.34 &amp; $-$3.04 &amp; N4 &amp; 13 &amp; $-$5.00 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5276.00 &amp; $-$1.94 &amp; MF &amp; 34 &amp; $-$5.21 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4582.84 &amp; $-$3.10 &amp; N4 &amp; 11 &amp; $-$5.07 &amp;  &amp; 26.01 &amp; Fe II  &amp;  ~J &amp; 5291.67 &amp;  ~~0.58 &amp; KX &amp; 13 &amp; $-$4.94 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4583.84 &amp; $-$2.02 &amp; N4 &amp; 51 &amp; $-$4.83 &amp;  &amp; 28.01 &amp; Ni II  &amp;  11 &amp; 3849.55 &amp; $-$1.88 &amp; KX &amp; ~9 &amp; $-$6.54 \\
26.01 &amp; Fe II  &amp;  ~~D &amp; 4596.02 &amp; $-$1.84 &amp; N4 &amp; ~8 &amp; $-$4.84 &amp;  &amp; 28.01 &amp; Ni II  &amp;  11 &amp; 4067.03 &amp; $-$1.29 &amp; KX &amp; 11 &amp; $-$7.03 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4620.52 &amp; $-$3.28 &amp; N4 &amp; ~8 &amp; $-$5.03 &amp;  &amp; 38.01 &amp; Sr II  &amp;  ~1 &amp; 4215.52 &amp; $-$0.17 &amp; WM &amp; 21 &amp; $-$8.35 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4629.34 &amp; $-$2.37 &amp; N4 &amp; 31 &amp; $-$5.10 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~6 &amp; 3950.35 &amp; $-$0.49 &amp; HL &amp; 21 &amp; $-$7.55 \\
26.01 &amp; Fe II  &amp;  186 &amp; 4635.32 &amp; $-$1.65 &amp; N4 &amp; 17 &amp; $-$4.77 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~6 &amp; 3982.59 &amp; $-$0.49 &amp; HL &amp; 19 &amp; $-$7.62 \\
26.01 &amp; Fe II  &amp;  ~28 &amp; 4666.76 &amp; $-$3.33 &amp; N4 &amp; 10 &amp; $-$4.90 &amp;  &amp; 39.01 &amp; Y II   &amp;  ~5 &amp; 4422.58 &amp; $-$1.27 &amp; HL &amp; ~7 &amp; $-$7.43 \\
26.01 &amp; Fe II  &amp;  ~43 &amp; 4731.45 &amp; $-$3.13 &amp; N4 &amp; 10 &amp; $-$5.05 &amp;  &amp; 39.01 &amp; Y II   &amp;  22 &amp; 4854.86 &amp; $-$0.38 &amp; HL &amp; 12 &amp; $-$7.59 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4908.15 &amp; $-$0.30 &amp; KX &amp; ~8 &amp; $-$4.50 &amp;  &amp; 39.01 &amp; Y II   &amp;  22 &amp; 4900.12 &amp; $-$0.09 &amp; HL &amp; 24 &amp; $-$7.38 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4951.58 &amp;  ~~0.18 &amp; KX &amp; 12 &amp; $-$4.76 &amp;  &amp; 39.01 &amp; Y II   &amp;  20 &amp; 5119.11 &amp; $-$1.36 &amp; HL &amp; ~4 &amp; $-$7.14 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4984.47 &amp;  ~~0.01 &amp; KX &amp; ~6 &amp; $-$4.92 &amp;  &amp; 39.01 &amp; Y II   &amp;  20 &amp; 5200.41 &amp; $-$0.57 &amp; HL &amp; 14 &amp; $-$7.28 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4990.51 &amp;  ~~0.18 &amp; KX &amp; ~8 &amp; $-$4.94 &amp;  &amp; 39.01 &amp; Y II   &amp;  20 &amp; 5205.72 &amp; $-$0.34 &amp; HL &amp; 20 &amp; $-$7.24 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4993.36 &amp; $-$3.65 &amp; MF &amp; ~4 &amp; $-$4.95 &amp;  &amp; 40.01 &amp; Zr II  &amp;  16 &amp; 3998.95 &amp; $-$0.67 &amp; GB &amp; ~5 &amp; $-$7.91 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5001.96 &amp;  ~~0.90 &amp; KX &amp; 28 &amp; $-$4.85 &amp;  &amp; 40.01 &amp; Zr II  &amp;  42 &amp; 4161.21 &amp; $-$0.72 &amp; BG &amp; 15 &amp; $-$7.26 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5004.20 &amp;  ~~0.50 &amp; KX &amp; 14 &amp; $-$4.96 &amp;  &amp; 80.01 &amp; Hg II  &amp; $-$ &amp; 3983.94 &amp; $-$1.73 &amp; DW &amp; 50 &amp; $-$5.39 \\
\bottomrule
\end{tabular}
\vspace{0.65cm}
\end{table*}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%



%%%%% TABLA 11

\setcounter{table}{10} 
\begin{table*}[!t]
%\vspace{0.1cm}
\centering
\caption{Line abundances of HR 8937}
\setlength{\tabnotewidth}{0.99\textwidth}
\tablecols{17}
\setlength{\tabcolsep}{0.778\tabcolsep}
\casitiny
\begin{tabular}{clcccccccclcccccc}
\toprule
Code &amp; \multicolumn{1}{c}{Species} &amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) &amp;  &amp; Code &amp; \multicolumn{1}{c}{Species} 
&amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) \\  
\cmidrule{1-8}
\cmidrule{10-17}
~6.01 &amp; C II   &amp;  ~~4 &amp; 3918.97 &amp; $-$0.53 &amp; WF &amp; ~19 &amp; $-$3.21 &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5308.44 &amp; $-$1.81 &amp; MF &amp; 20 &amp; $-$5.61 \\
~6.01 &amp; C II   &amp;  ~~4 &amp; 3920.68 &amp; $-$0.23 &amp; WF &amp; ~24 &amp; $-$3.27 &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5310.70 &amp; $-$2.28 &amp; MF &amp; ~8 &amp; $-$5.63 \\
12.00 &amp; Mg I   &amp;  ~~2 &amp; 5172.68 &amp; $-$0.38 &amp; WS &amp; ~15 &amp; $-$5.01 &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5313.59 &amp; $-$1.65 &amp; MF &amp; 19 &amp; $-$5.82 \\
12.00 &amp; Mg I   &amp;  ~~2 &amp; 5183.60 &amp; $-$0.16 &amp; WS &amp; ~22 &amp; $-$5.02 &amp;  &amp; 24.01 &amp; Cr II  &amp; ~~43 &amp; 5334.87 &amp; $-$1.56 &amp; KX &amp; 19 &amp; $-$5.90 \\
12.01 &amp; Mg II  &amp;  ~~5 &amp; 3848.21 &amp; $-$1.59 &amp; WS &amp; ~25 &amp; $-$4.51 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~~2 &amp; 4030.75 &amp; $-$0.47 &amp; MF &amp; 27 &amp; $-$4.98 \\
12.01 &amp; Mg II  &amp;  ~10 &amp; 4390.57 &amp; $-$0.53 &amp; WS &amp; ~35 &amp; $-$4.88 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~~2 &amp; 4033.06 &amp; $-$0.62 &amp; MF &amp; 47 &amp; $-$4.26 \\
12.01 &amp; Mg II  &amp;  ~~9 &amp; 4427.99 &amp; $-$1.21 &amp; WS &amp; ~11 &amp; $-$4.80 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~~2 &amp; 4034.48 &amp; $-$0.81 &amp; MF &amp; 19 &amp; $-$4.86 \\
14.01 &amp; Si II  &amp;  ~~1 &amp; 3853.66 &amp; $-$1.44 &amp; LA &amp; ~69 &amp; $-$4.59 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~~5 &amp; 4035.72 &amp; $-$0.19 &amp; KX &amp; 10 &amp; $-$4.80 \\
14.01 &amp; Si II  &amp;  ~~1 &amp; 3856.02 &amp; $-$0.49 &amp; LA &amp; 122 &amp; $-$4.76 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~~5 &amp; 4041.35 &amp;  ~~0.29 &amp; MF &amp; 26 &amp; $-$4.71 \\
14.01 &amp; Si II  &amp;  ~~1 &amp; 3862.59 &amp; $-$0.74 &amp; LA &amp; 103 &amp; $-$4.76 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~22 &amp; 4414.89 &amp; $-$0.29 &amp; MF &amp; ~7 &amp; $-$4.51 \\
14.01 &amp; Si II  &amp; 3.01 &amp; 4075.45 &amp; $-$1.40 &amp; SG &amp; ~17 &amp; $-$4.52 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~16 &amp; 4754.04 &amp; $-$0.09 &amp; MF &amp; 12 &amp; $-$4.72 \\
14.01 &amp; Si II  &amp; 3.01 &amp; 4076.78 &amp; $-$1.67 &amp; SG &amp; ~17 &amp; $-$4.23 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~21 &amp; 4761.51 &amp; $-$0.14 &amp; MF &amp; ~5 &amp; $-$4.74 \\
14.01 &amp; Si II  &amp;  ~~3 &amp; 4128.05 &amp;  ~~0.38 &amp; LA &amp; 145 &amp; $-$4.27 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~21 &amp; 4765.85 &amp; $-$0.08 &amp; MF &amp; 11 &amp; $-$4.45 \\
14.01 &amp; Si II  &amp;  ~~3 &amp; 4130.89 &amp;  ~~0.53 &amp; LA &amp; 128 &amp; $-$4.56 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~21 &amp; 4766.42 &amp;  ~~0.10 &amp; MF &amp; 11 &amp; $-$4.62 \\
14.01 &amp; Si II  &amp;  ~~5 &amp; 5041.02 &amp;  ~~0.29 &amp; SG &amp; ~90 &amp; $-$4.44 &amp;  &amp; 25.00 &amp; Mn I   &amp; ~~16 &amp; 4783.43 &amp;  ~~0.04 &amp; MF &amp; 15 &amp; $-$4.72 \\
15.01 &amp; P II   &amp;  ~15 &amp; 4602.07 &amp;  ~~0.74 &amp; WS &amp; ~11 &amp; $-$5.37 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3859.21 &amp; $-$2.56 &amp; KX &amp; 10 &amp; $-$4.80 \\
16.01 &amp; S II   &amp;  ~44 &amp; 4153.07 &amp;  ~~0.62 &amp; WS &amp; ~~4 &amp; $-$5.13 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3878.99 &amp; $-$1.71 &amp; KX &amp; 40 &amp; $-$4.61 \\
16.01 &amp; S II   &amp;  ~44 &amp; 4162.66 &amp;  ~~0.78 &amp; WS &amp; ~~7 &amp; $-$4.96 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3917.32 &amp; $-$1.15 &amp; KX &amp; 35 &amp; $-$4.65 \\
16.01 &amp; S II   &amp;  ~~9 &amp; 4815.55 &amp;  ~~0.18 &amp; WM &amp; ~~5 &amp; $-$5.17 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3952.42 &amp; $-$1.50 &amp; KX &amp; 15 &amp; $-$4.53 \\
20.01 &amp; Ca II  &amp;  ~~1 &amp; 3933.66 &amp;  ~~0.13 &amp; WM &amp; 232 &amp; $-$5.93 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3986.58 &amp; $-$2.60 &amp; KX &amp; 18 &amp; $-$4.41 \\
22.01 &amp; Ti II  &amp;  ~34 &amp; 3900.54 &amp; $-$0.45 &amp; MF &amp; ~47 &amp; $-$6.76 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3995.31 &amp; $-$2.44 &amp; KX &amp; 17 &amp; $-$4.65 \\
22.01 &amp; Ti II  &amp;  ~34 &amp; 3913.46 &amp; $-$0.53 &amp; MF &amp; ~49 &amp; $-$6.65 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4000.05 &amp; $-$1.21 &amp; KX &amp; 31 &amp; $-$4.31 \\
22.01 &amp; Ti II  &amp;  ~87 &amp; 4028.34 &amp; $-$1.00 &amp; MF &amp; ~16 &amp; $-$6.70 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4081.44 &amp; $-$2.24 &amp; KX &amp; 32 &amp; $-$4.02 \\
22.01 &amp; Ti II  &amp;  105 &amp; 4163.64 &amp; $-$0.40 &amp; MF &amp; ~30 &amp; $-$6.55 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4087.91 &amp; $-$2.91 &amp; KX &amp; ~9 &amp; $-$4.51 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4294.09 &amp; $-$1.11 &amp; MF &amp; ~36 &amp; $-$6.44 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4110.62 &amp; $-$1.51 &amp; KX &amp; 34 &amp; $-$4.68 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4300.04 &amp; $-$0.77 &amp; MF &amp; ~54 &amp; $-$6.22 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4140.44 &amp; $-$2.46 &amp; KX &amp; 18 &amp; $-$4.50 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4301.92 &amp; $-$1.16 &amp; MF &amp; ~16 &amp; $-$6.90 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4184.45 &amp; $-$1.95 &amp; KX &amp; 28 &amp; $-$4.38 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4312.86 &amp; $-$1.16 &amp; MF &amp; ~26 &amp; $-$6.58 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4200.27 &amp; $-$1.74 &amp; KX &amp; 39 &amp; $-$4.28 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4395.03 &amp; $-$0.66 &amp; MF &amp; ~47 &amp; $-$6.58 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~2 &amp; 4205.38 &amp; $-$3.38 &amp; KX &amp; 57 &amp; $-$4.25 \\
22.01 &amp; Ti II  &amp;  ~61 &amp; 4395.84 &amp; $-$2.17 &amp; MF &amp; ~~6 &amp; $-$6.34 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4240.39 &amp; $-$2.07 &amp; KX &amp; 29 &amp; $-$4.25 \\
22.01 &amp; Ti II  &amp;  ~51 &amp; 4399.77 &amp; $-$1.27 &amp; MF &amp; ~16 &amp; $-$6.75 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~7 &amp; 4244.25 &amp; $-$2.39 &amp; KX &amp; 37 &amp; $-$4.10 \\
22.01 &amp; Ti II  &amp;  ~40 &amp; 4417.71 &amp; $-$1.43 &amp; MF &amp; ~16 &amp; $-$6.62 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~2 &amp; 4260.46 &amp; $-$4.25 &amp; KX &amp; 19 &amp; $-$4.49 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4443.80 &amp; $-$0.70 &amp; MF &amp; ~37 &amp; $-$6.81 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4377.74 &amp; $-$2.14 &amp; KX &amp; 22 &amp; $-$4.73 \\
22.01 &amp; Ti II  &amp;  ~19 &amp; 4450.48 &amp; $-$1.45 &amp; MF &amp; ~13 &amp; $-$6.76 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4391.96 &amp; $-$2.89 &amp; KX &amp; ~7 &amp; $-$4.58 \\
22.01 &amp; Ti II  &amp;  ~31 &amp; 4468.49 &amp; $-$0.60 &amp; MF &amp; ~37 &amp; $-$6.89 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4393.38 &amp; $-$2.32 &amp; KX &amp; 20 &amp; $-$4.61 \\
22.01 &amp; Ti II  &amp;  115 &amp; 4488.32 &amp; $-$0.82 &amp; MF &amp; ~11 &amp; $-$6.48 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4403.51 &amp; $-$1.80 &amp; KX &amp; 20 &amp; $-$4.58 \\
22.01 &amp; Ti II  &amp;  ~31 &amp; 4501.27 &amp; $-$0.75 &amp; MF &amp; ~33 &amp; $-$6.85 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4478.64 &amp; $-$0.95 &amp; KX &amp; 49 &amp; $-$4.51 \\
22.01 &amp; Ti II  &amp;  ~50 &amp; 4533.96 &amp; $-$0.77 &amp; MF &amp; ~51 &amp; $-$6.28 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4497.94 &amp; $-$2.59 &amp; KX &amp; 10 &amp; $-$4.74 \\
22.01 &amp; Ti II  &amp;  ~41 &amp; 4563.76 &amp; $-$0.96 &amp; MF &amp; ~31 &amp; $-$6.63 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4500.54 &amp; $-$2.07 &amp; KX &amp; 15 &amp; $-$4.77 \\
22.01 &amp; Ti II  &amp;  ~82 &amp; 4571.97 &amp; $-$0.53 &amp; MF &amp; ~47 &amp; $-$6.47 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4503.20 &amp; $-$2.16 &amp; KX &amp; 19 &amp; $-$4.55 \\
22.01 &amp; Ti II  &amp;  ~59 &amp; 4657.20 &amp; $-$2.15 &amp; MF &amp; ~~9 &amp; $-$6.17 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4689.55 &amp; $-$2.54 &amp; KX &amp; 15 &amp; $-$4.22 \\
22.01 &amp; Ti II  &amp;  ~92 &amp; 4779.98 &amp; $-$1.37 &amp; MF &amp; ~~9 &amp; $-$6.53 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4702.73 &amp; $-$2.34 &amp; KX &amp; 13 &amp; $-$4.49 \\
22.01 &amp; Ti II  &amp;  ~82 &amp; 4805.09 &amp; $-$1.10 &amp; MF &amp; ~13 &amp; $-$6.61 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4717.26 &amp; $-$1.86 &amp; KX &amp; 19 &amp; $-$4.56 \\
22.01 &amp; Ti II  &amp;  114 &amp; 4911.20 &amp; $-$0.34 &amp; MF &amp; ~~9 &amp; $-$7.05 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4730.40 &amp; $-$2.15 &amp; KX &amp; 46 &amp; $-$4.03 \\
22.01 &amp; Ti II  &amp;  ~86 &amp; 5185.90 &amp; $-$1.35 &amp; MF &amp; ~22 &amp; $-$6.14 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4749.11 &amp; $-$2.00 &amp; KX &amp; 17 &amp; $-$4.64 \\
22.01 &amp; Ti II  &amp;  ~~7 &amp; 5188.69 &amp; $-$1.21 &amp; MF &amp; ~14 &amp; $-$6.72 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4791.78 &amp; $-$1.72 &amp; KX &amp; 29 &amp; $-$4.56 \\
24.01 &amp; Cr II  &amp;  167 &amp; 3865.60 &amp; $-$0.78 &amp; KX &amp; ~25 &amp; $-$5.92 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4806.82 &amp; $-$1.56 &amp; KX &amp; 55 &amp; $-$4.30 \\
24.01 &amp; Cr II  &amp;  167 &amp; 3905.64 &amp; $-$0.90 &amp; KX &amp; ~43 &amp; $-$5.30 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4830.06 &amp; $-$1.85 &amp; KX &amp; 30 &amp; $-$4.41 \\
24.01 &amp; Cr II  &amp;  129 &amp; 3911.32 &amp; $-$2.06 &amp; KX &amp; ~~9 &amp; $-$5.43 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4839.74 &amp; $-$1.86 &amp; KX &amp; 21 &amp; $-$4.65 \\
24.01 &amp; Cr II  &amp;  183 &amp; 3979.50 &amp; $-$0.73 &amp; KX &amp; ~15 &amp; $-$6.15 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 4842.32 &amp; $-$2.01 &amp; KX &amp; 25 &amp; $-$4.38 \\
24.01 &amp; Cr II  &amp;  ~19 &amp; 4051.93 &amp; $-$2.19 &amp; KX &amp; ~~9 &amp; $-$6.16 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 5102.52 &amp; $-$1.93 &amp; KX &amp; 40 &amp; $-$4.08 \\
24.01 &amp; Cr II  &amp;  ~26 &amp; 4072.56 &amp; $-$2.41 &amp; KX &amp; ~11 &amp; $-$5.57 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 5307.35 &amp; $-$2.07 &amp; KX &amp; 11 &amp; $-$4.39 \\
24.01 &amp; Cr II  &amp;  162 &amp; 4145.78 &amp; $-$1.16 &amp; KX &amp; ~16 &amp; $-$5.85 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3902.36 &amp; $-$2.72 &amp; KX &amp; 10 &amp; $-$4.59 \\
24.01 &amp; Cr II  &amp;  ~31 &amp; 4261.91 &amp; $-$1.53 &amp; KX &amp; ~46 &amp; $-$5.31 &amp;  &amp; 25.01 &amp; Mn II  &amp; ~~~I &amp; 3926.11 &amp; $-$2.42 &amp; KX &amp; 26 &amp; $-$4.08 \\
24.01 &amp; Cr II  &amp;  ~31 &amp; 4275.57 &amp; $-$1.70 &amp; KX &amp; ~28 &amp; $-$5.64 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~45 &amp; 3815.84 &amp;  ~~0.23 &amp; N4 &amp; 19 &amp; $-$4.80 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4554.99 &amp; $-$1.38 &amp; MF &amp; ~31 &amp; $-$5.76 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~20 &amp; 3825.88 &amp; $-$0.04 &amp; N4 &amp; 20 &amp; $-$4.80 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4558.65 &amp; $-$0.66 &amp; MF &amp; ~64 &amp; $-$5.51 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~~4 &amp; 3859.91 &amp; $-$0.71 &amp; N4 &amp; 14 &amp; $-$4.79 \\
24.01 &amp; Cr II  &amp;  ~39 &amp; 4565.74 &amp; $-$2.11 &amp; MF &amp; ~13 &amp; $-$5.63 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~20 &amp; 3865.52 &amp; $-$0.98 &amp; N4 &amp; 18 &amp; $-$3.88 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4588.20 &amp; $-$0.63 &amp; MF &amp; ~65 &amp; $-$5.50 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~20 &amp; 3872.50 &amp; $-$0.93 &amp; N4 &amp; 12 &amp; $-$4.17 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4592.05 &amp; $-$1.22 &amp; MF &amp; ~30 &amp; $-$5.94 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~43 &amp; 4071.74 &amp; $-$0.02 &amp; N4 &amp; 12 &amp; $-$4.78 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4616.63 &amp; $-$1.29 &amp; MF &amp; ~24 &amp; $-$6.06 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~152 &amp; 4198.30 &amp; $-$0.72 &amp; N4 &amp; ~8 &amp; $-$3.89 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4618.80 &amp; $-$1.11 &amp; MF &amp; ~45 &amp; $-$5.65 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~522 &amp; 4199.10 &amp;  ~~0.16 &amp; N4 &amp; 18 &amp; $-$4.01 \\
24.01 &amp; Cr II  &amp;  ~44 &amp; 4634.07 &amp; $-$1.24 &amp; MF &amp; ~39 &amp; $-$5.68 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~42 &amp; 4271.76 &amp; $-$0.16 &amp; N4 &amp; 11 &amp; $-$4.74 \\
24.01 &amp; Cr II  &amp;  ~30 &amp; 4812.34 &amp; $-$1.80 &amp; MF &amp; ~11 &amp; $-$6.11 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~41 &amp; 4383.54 &amp;  ~~0.20 &amp; N4 &amp; 19 &amp; $-$4.79 \\
24.01 &amp; Cr II  &amp;  ~30 &amp; 4824.13 &amp; $-$1.22 &amp; MF &amp; ~48 &amp; $-$5.55 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~~41 &amp; 4404.75 &amp; $-$0.14 &amp; N4 &amp; 16 &amp; $-$4.51 \\
24.01 &amp; Cr II  &amp;  ~30 &amp; 4836.23 &amp; $-$2.25 &amp; MF &amp; ~12 &amp; $-$5.61 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~318 &amp; 4920.50 &amp;  ~~0.07 &amp; N4 &amp; 22 &amp; $-$3.90 \\
24.01 &amp; Cr II  &amp;  ~30 &amp; 4848.23 &amp; $-$1.14 &amp; MF &amp; ~31 &amp; $-$6.11 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~289 &amp; 4957.30 &amp; $-$0.41 &amp; N4 &amp; ~9 &amp; $-$3.90 \\
24.01 &amp; Cr II  &amp;  105 &amp; 4876.40 &amp; $-$1.46 &amp; KX &amp; ~35 &amp; $-$5.68 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~318 &amp; 4957.60 &amp;  ~~0.23 &amp; N4 &amp; ~9 &amp; $-$4.58 \\
24.01 &amp; Cr II  &amp;  ~30 &amp; 4884.61 &amp; $-$2.08 &amp; MF &amp; ~~8 &amp; $-$5.94 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~325 &amp; 5192.34 &amp; $-$0.42 &amp; N4 &amp; ~8 &amp; $-$3.86 \\
24.01 &amp; Cr II  &amp;  ~43 &amp; 5232.50 &amp; $-$2.09 &amp; KX &amp; ~15 &amp; $-$5.50 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~383 &amp; 5232.94 &amp; $-$0.06 &amp; N4 &amp; 17 &amp; $-$3.86 \\
24.01 &amp; Cr II  &amp;  ~23 &amp; 5246.77 &amp; $-$2.45 &amp; MF &amp; ~16 &amp; $-$5.29 &amp;  &amp; 26.00 &amp; Fe I   &amp; 1146 &amp; 5383.37 &amp;  ~~0.65 &amp; N4 &amp; 12 &amp; $-$4.10 \\
24.01 &amp; Cr II  &amp;  ~43 &amp; 5274.96 &amp; $-$1.29 &amp; KX &amp; ~24 &amp; $-$6.01 &amp;  &amp; 26.00 &amp; Fe I   &amp; ~686 &amp; 5586.76 &amp; $-$0.14 &amp; N4 &amp; ~8 &amp; $-$3.96 \\
\bottomrule
\end{tabular}
\end{table*}


%%%%% CONTINUA TABLA 11

\setcounter{table}{10} 
\begin{table*}[!t]
\vspace{0.1cm}
\centering
\centerline{TABLE~11 (CONTINUED)\smallskip}
\setlength{\tabnotewidth}{0.99\textwidth}
\tablecols{17}
\setlength{\tabcolsep}{0.778\tabcolsep}
\casitiny
\begin{tabular}{clcccccccclcccccc}
\toprule
Code &amp; \multicolumn{1}{c}{Species} &amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) &amp;  &amp; Code &amp; \multicolumn{1}{c}{Species} 
&amp; Mult. &amp; $\lambda$(\AA) &amp; $\log gf$ &amp; Ref. &amp;  $W_\mathrm{eq}$ &amp; $\log(N/N_{T}$) \\  
\cmidrule{1-8}
\cmidrule{10-17}
26.01 &amp; Fe II  &amp;  127 &amp; 3845.18 &amp; $-$2.29 &amp; KX &amp; ~13 &amp; $-$4.82 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5070.90 &amp;  ~~0.24 &amp; KX &amp; ~18 &amp; $-$4.36 \\
26.01 &amp; Fe II  &amp;  173 &amp; 3906.04 &amp; $-$1.83 &amp; N4 &amp; ~28 &amp; $-$4.29 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5075.76 &amp;  ~~0.28 &amp; KX &amp; ~15 &amp; $-$4.44 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 3935.96 &amp; $-$1.86 &amp; N4 &amp; ~24 &amp; $-$4.37 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5082.23 &amp; $-$0.10 &amp; KX &amp; ~~9 &amp; $-$4.39 \\
26.01 &amp; Fe II  &amp;  ~~3 &amp; 3938.29 &amp; $-$4.07 &amp; N4 &amp; ~13 &amp; $-$4.39 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5093.58 &amp;  ~~0.11 &amp; KX &amp; ~22 &amp; $-$4.01 \\
26.01 &amp; Fe II  &amp;  ~90 &amp; 3938.97 &amp; $-$1.85 &amp; N4 &amp; ~20 &amp; $-$4.34 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5097.27 &amp;  ~~0.31 &amp; KX &amp; ~31 &amp; $-$3.95 \\
26.01 &amp; Fe II  &amp;  ~28 &amp; 4122.67 &amp; $-$3.38 &amp; N4 &amp; ~20 &amp; $-$4.41 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5106.11 &amp; $-$0.28 &amp; KX &amp; ~13 &amp; $-$4.02 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4233.17 &amp; $-$1.81 &amp; N4 &amp; ~83 &amp; $-$4.02 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5117.03 &amp; $-$0.13 &amp; KX &amp; ~~8 &amp; $-$4.41 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4273.33 &amp; $-$3.34 &amp; N4 &amp; ~20 &amp; $-$4.36 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5145.77 &amp; $-$0.40 &amp; KX &amp; ~12 &amp; $-$3.92 \\
26.01 &amp; Fe II  &amp;  ~28 &amp; 4296.57 &amp; $-$3.01 &amp; N4 &amp; ~33 &amp; $-$4.32 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5149.46 &amp;  ~~0.40 &amp; KX &amp; ~28 &amp; $-$4.09 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4303.18 &amp; $-$2.61 &amp; N4 &amp; ~57 &amp; $-$4.01 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5150.49 &amp; $-$0.12 &amp; KX &amp; ~12 &amp; $-$4.18 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4351.77 &amp; $-$2.08 &amp; N4 &amp; ~50 &amp; $-$4.74 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5160.84 &amp; $-$2.64 &amp; KX &amp; ~10 &amp; $-$4.03 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4357.58 &amp; $-$2.10 &amp; KX &amp; ~~9 &amp; $-$4.45 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5169.03 &amp; $-$0.87 &amp; MF &amp; 106 &amp; $-$4.26 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4385.39 &amp; $-$2.57 &amp; N4 &amp; ~45 &amp; $-$4.37 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5180.31 &amp;  ~~0.04 &amp; KX &amp; ~~5 &amp; $-$4.77 \\
26.01 &amp; Fe II  &amp;  ~27 &amp; 4416.83 &amp; $-$2.60 &amp; N4 &amp; ~40 &amp; $-$4.49 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5199.12 &amp;  ~~0.10 &amp; KX &amp; ~21 &amp; $-$4.03 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4472.93 &amp; $-$3.53 &amp; N4 &amp; ~13 &amp; $-$4.38 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5203.64 &amp; $-$0.05 &amp; KX &amp; ~16 &amp; $-$4.07 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4489.18 &amp; $-$2.97 &amp; N4 &amp; ~31 &amp; $-$4.34 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5216.85 &amp;    0.81 &amp; KX &amp; ~28 &amp; $-$4.45 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4491.40 &amp; $-$2.70 &amp; N4 &amp; ~36 &amp; $-$4.46 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5223.26 &amp; $-$0.41 &amp; KX &amp; ~~7 &amp; $-$4.17 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4508.29 &amp; $-$2.21 &amp; N4 &amp; ~50 &amp; $-$4.53 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5228.90 &amp; $-$0.30 &amp; KX &amp; ~12 &amp; $-$3.99 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4515.34 &amp; $-$2.48 &amp; N4 &amp; ~42 &amp; $-$4.51 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5232.79 &amp; $-$0.06 &amp; KX &amp; ~16 &amp; $-$4.07 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4520.22 &amp; $-$2.60 &amp; N4 &amp; ~38 &amp; $-$4.54 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5234.62 &amp; $-$2.05 &amp; MF &amp; ~57 &amp; $-$4.22 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4522.63 &amp; $-$2.03 &amp; N4 &amp; ~56 &amp; $-$4.55 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5247.95 &amp;  ~~0.55 &amp; N4 &amp; ~31 &amp; $-$4.08 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4541.52 &amp; $-$3.05 &amp; N4 &amp; ~28 &amp; $-$4.35 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5251.23 &amp;  ~~0.42 &amp; N4 &amp; ~30 &amp; $-$3.98 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4555.89 &amp; $-$2.29 &amp; N4 &amp; ~51 &amp; $-$4.44 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5254.93 &amp; $-$3.23 &amp; KX &amp; ~13 &amp; $-$4.44 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4576.34 &amp; $-$3.04 &amp; N4 &amp; ~26 &amp; $-$4.40 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5257.12 &amp;  ~~0.03 &amp; KX &amp; ~12 &amp; $-$4.30 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4582.84 &amp; $-$3.10 &amp; N4 &amp; ~22 &amp; $-$4.48 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5260.25 &amp;  ~~1.07 &amp; KX &amp; ~46 &amp; $-$4.25 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4583.84 &amp; $-$2.02 &amp; N4 &amp; ~69 &amp; $-$4.15 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5272.40 &amp; $-$2.03 &amp; MF &amp; ~18 &amp; $-$4.09 \\
26.01 &amp; Fe II  &amp;  ~~D &amp; 4596.02 &amp; $-$1.84 &amp; N4 &amp; ~18 &amp; $-$4.24 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5276.00 &amp; $-$1.94 &amp; MF &amp; ~52 &amp; $-$4.51 \\
26.01 &amp; Fe II  &amp;  ~38 &amp; 4620.52 &amp; $-$3.28 &amp; N4 &amp; ~20 &amp; $-$4.35 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5291.67 &amp;  ~~0.58 &amp; KX &amp; ~37 &amp; $-$3.95 \\
26.01 &amp; Fe II  &amp;  ~37 &amp; 4629.34 &amp; $-$2.37 &amp; N4 &amp; ~50 &amp; $-$4.39 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5306.18 &amp;  ~~0.09 &amp; N4 &amp; ~23 &amp; $-$3.87 \\
26.01 &amp; Fe II  &amp;  186 &amp; 4635.32 &amp; $-$1.65 &amp; N4 &amp; ~29 &amp; $-$4.20 &amp;  &amp; 26.01 &amp; Fe II  &amp;   ~J &amp; 5339.59 &amp;  ~~0.54 &amp; KX &amp; ~30 &amp; $-$4.11 \\
26.01 &amp; Fe II  &amp;  ~28 &amp; 4666.76 &amp; $-$3.33 &amp; N4 &amp; ~18 &amp; $-$4.37 &amp;  &amp; 26.02 &amp; Fe III &amp;   ~4 &amp; 4419.60 &amp; $-$2.22 &amp; KX &amp; ~~3 &amp; $-$4.35 \\
26.01 &amp; Fe II  &amp;  ~43 &amp; 4731.45 &amp; $-$3.13 &amp; N4 &amp; ~22 &amp; $-$4.41 &amp;  &amp; 38.01 &amp; Sr II  &amp;   ~1 &amp; 4215.52 &amp; $-$0.17 &amp; WM &amp; ~81 &amp; $-$6.30 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4908.15 &amp; $-$0.30 &amp; KX &amp; ~10 &amp; $-$4.17 &amp;  &amp; 39.01 &amp; Y II   &amp;   ~6 &amp; 3950.35 &amp; $-$0.49 &amp; HL &amp; ~52 &amp; $-$6.51 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4913.29 &amp;  ~~0.01 &amp; KX &amp; ~14 &amp; $-$4.32 &amp;  &amp; 39.01 &amp; Y II   &amp;   ~6 &amp; 3982.59 &amp; $-$0.49 &amp; HL &amp; ~54 &amp; $-$6.45 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4951.58 &amp;  ~~0.18 &amp; KX &amp; ~18 &amp; $-$4.32 &amp;  &amp; 39.01 &amp; Y II   &amp;   14 &amp; 4124.90 &amp; $-$1.50 &amp; HL &amp; ~29 &amp; $-$6.29 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4977.04 &amp;  ~~0.04 &amp; KX &amp; ~17 &amp; $-$4.16 &amp;  &amp; 39.01 &amp; Y II   &amp;   ~5 &amp; 4235.73 &amp; $-$1.50 &amp; HL &amp; ~34 &amp; $-$6.26 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4984.47 &amp;  ~~0.01 &amp; KX &amp; ~12 &amp; $-$4.33 &amp;  &amp; 39.01 &amp; Y II   &amp;   ~5 &amp; 4422.58 &amp; $-$1.27 &amp; HL &amp; ~35 &amp; $-$6.49 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4990.51 &amp;  ~~0.18 &amp; KX &amp; ~15 &amp; $-$4.41 &amp;  &amp; 39.01 &amp; Y II   &amp;   22 &amp; 4854.86 &amp; $-$0.38 &amp; HL &amp; ~37 &amp; $-$6.81 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 4993.36 &amp; $-$3.65 &amp; MF &amp; ~~7 &amp; $-$4.55 &amp;  &amp; 39.01 &amp; Y II   &amp;   22 &amp; 4900.12 &amp; $-$0.09 &amp; HL &amp; ~59 &amp; $-$6.18 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5001.96 &amp;  ~~0.90 &amp; KX &amp; ~44 &amp; $-$4.25 &amp;  &amp; 39.01 &amp; Y II   &amp;   20 &amp; 4982.13 &amp; $-$1.29 &amp; HL &amp; ~19 &amp; $-$6.53 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5004.20 &amp;  ~~0.50 &amp; KX &amp; ~24 &amp; $-$4.43 &amp;  &amp; 39.01 &amp; Y II   &amp;   20 &amp; 5200.41 &amp; $-$0.57 &amp; HL &amp; ~48 &amp; $-$6.15 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5015.75 &amp; $-$0.05 &amp; KX &amp; ~24 &amp; $-$3.86 &amp;  &amp; 39.01 &amp; Y II   &amp;   20 &amp; 5205.72 &amp; $-$0.34 &amp; HL &amp; ~54 &amp; $-$6.10 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5018.44 &amp; $-$1.22 &amp; MF &amp; 102 &amp; $-$3.99 &amp;  &amp; 39.01 &amp; Y II   &amp;   20 &amp; 5289.82 &amp; $-$1.85 &amp; HL &amp; ~10 &amp; $-$6.35 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5021.59 &amp; $-$0.30 &amp; KX &amp; ~~6 &amp; $-$4.44 &amp;  &amp; 40.01 &amp; Zr II  &amp;   17 &amp; 3915.96 &amp; $-$0.82 &amp; KX &amp; ~~6 &amp; $-$7.86 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5022.79 &amp; $-$0.02 &amp; KX &amp; ~19 &amp; $-$4.17 &amp;  &amp; 40.01 &amp; Zr II  &amp;   16 &amp; 3958.23 &amp; $-$0.31 &amp; KX &amp; ~15 &amp; $-$7.85 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5030.63 &amp;  ~~0.40 &amp; KX &amp; ~21 &amp; $-$4.44 &amp;  &amp; 40.01 &amp; Zr II  &amp;   30 &amp; 3991.15 &amp; $-$0.25 &amp; KX &amp; ~16 &amp; $-$7.77 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5035.71 &amp;  ~~0.61 &amp; KX &amp; ~31 &amp; $-$4.32 &amp;  &amp; 40.01 &amp; Zr II  &amp;   16 &amp; 3998.95 &amp; $-$0.67 &amp; GB &amp; ~16 &amp; $-$7.45 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5045.11 &amp; $-$0.13 &amp; KX &amp; ~~9 &amp; $-$4.38 &amp;  &amp; 40.01 &amp; Zr II  &amp;   41 &amp; 4149.22 &amp; $-$0.03 &amp; BG &amp; ~24 &amp; $-$7.69 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5061.72 &amp;  ~~0.22 &amp; KX &amp; ~16 &amp; $-$4.41 &amp;  &amp; 40.01 &amp; Zr II  &amp;   41 &amp; 4208.98 &amp; $-$0.46 &amp; BG &amp; ~13 &amp; $-$7.70 \\
26.01 &amp; Fe II  &amp;  ~~J &amp; 5067.89 &amp; $-$0.20 &amp; KX &amp; ~~8 &amp; $-$4.35 &amp;  &amp; 80.01 &amp; Hg II  &amp;  $-$ &amp; 3983.94 &amp; $-$1.73 &amp; DW &amp; 128 &amp; $-$4.06 \\
\bottomrule
\end{tabular}
\vspace{0.6cm}
\end{table*}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


\section{Discussion}

HR 3273, HR 8118, HR 8567 and HR 8937 are main sequence stars with anomalous abundances, i.e. different from solar values. The comparison of derived 
and solar abundances for the HgMn stars is presented in the Table~7. We included the rms of the average abundance for each species and the number of 
lines $n$ involved in the average. Solar abundances have been taken from Grevesse, Noels, \&amp; Sauval (1996). We also present in Tables 8--11 the line 
by line abundance values derived for the sample of HgMn stars. The columns shown are the code of the species, the name of the element, multiplet number, 
wavelength of the line, $\log gf$ value, reference for the $\log gf$ value, equivalent width and abundance of the line. In Figure~\ref{abunds} we 
show the abundance anomalies relative to solar as a function of the atomic number. The HgMn stars are presented as crosses (HR 3273), empty triangles 
(HR 8118), empty circles (HR 8567) and empty squares (HR 8937). For comparison purposes we show the abundances of four other HgMn stars, depicted as 
filled circles (HR 4817), filled triangles ($\pi$ Boo), filled hexagons ($\mu$ Lep) and filled squares (28 Her). These data are taken from 
\citet{adelman-pintado97}. From the values presented in Table~7 and Figure~\ref{abunds}, our sample of HgMn stars shows an abundance pattern similar to 
other HgMn stars. However there are some differences in particular cases.


%%%%% FIGURA 1

\begin{figure*}[!t]
\centering
\includegraphics[width=10cm]{csaffefig1.eps}
\caption{Abundance anomalies relative to solar as a function of the atomic number. The 
HgMn stars are presented as crosses (HR 3273), empty triangles (HR 8118), empty circles 
(HR 8567) and empty squares (HR 8937). For comparison purposes we show the abundances of 
four other HgMn stars, depicted as filled circles (HR 4817), filled triangles ($\pi$ Boo), 
filled hexagons ($\mu$ Lep) and filled squares (28 Her). Data taken from \citet{adelman-pintado97}.}
\label{abunds}
%\vspace{0.3cm}
\end{figure*}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%


The star HR 3273 shows a relatively low abundance of SiII (8 lines) compared to other HgMn stars. In the star HR 8567, the abundance of CrII (32 lines) 
is relatively high compared to other HgMn stars. The CrII lines $\lambda\lambda$4588, 4634 and 5237, for instance, are intense in the spectra. The Mn 
and Hg abundances are similar to other HgMn stars. The abundance of CII in HR 8118 and HR 8937 is also relatively high. However, this value is based on 
few lines, and assumes the LTE approximation. For star HR 8937, the abundance of SrII is high compared to other HgMn stars. However, this value is derived 
from one line and should be taken with caution. For HR 8937 we adopted the Hg abundance derived by \citet{dolk03}. They found an abundance of 
$-4.23\pm0.43$~dex, i.e., a relatively high value. We compared this value with an estimation using the equivalent width of $\lambda\lambda$3984 and derived 
$-$4.06~dex, i.e. also a high abundance for HgII in this star.

For star HR 8118, the abundances of CII, AlII and ScII seem to be relatively high compared to other HgMn stars. However, these values are based on the 
measurement of few lines (2, 1 and 1, respectively) and should be taken with caution. On the other hand, the abundances of CrII, YII and ZrII are also 
relatively high, from a greater number of lines (23, 9 and 13, respectively). We caution that this star has the highest $v \sin i$ in our sample 
($30\pm1$~km~s$^{-1}$) which suggest that high abundance values in different species might be due to blends with another lines. However this effect is 
not clearly seen in the FeII abundances (63 lines), and thus the CrII abundance could be real. A comparison of higher resolution spectra with synthetic 
spectra is needed to verify the abundance of Cr, Y and Zr in this star.

HeI was slightly underabundant for the sample of HgMn stars and underabundantin HR 8937. O was slightly underabundant in the stars HR 3273 and HR~8567. 
MgII was underabundant, except for HR 8118 (which is close to the solar value). SiII was close to solar in HR~8118 and HR 8937, and underabundant in 
HR 3273 and HR 8567. Fe was slightly underabundant in HR 3273 and HR 8567, and slightly overabundant in HR 8118 and HR 8937. The species Sc, Ti, Cr, Mn, 
Sr, Y and Zr were overabundant while Ni was underabundant.

As we said in the Introduction, our purpose is to discuss the possible trend of the abundances of the critical elements in HgMn stars with stellar parameters. 
Papers in the literature show that the abundances of some elements seem to correlate with the effective temperature 
\citep[e.g., ][]{smith-dworetsky93,smith97,woolf-lambert99,jomaron99,dolk03}. However, it is not clear (for instance) how the abundances are correlated 
with stellar rotation. If difussion is operating in the atmospheres, probably one should expect that abundance anomalies should decrease with increasing 
rotational velocity. In fact, CP stars are rarely found having rotational velocities larger than $\sim$120~km~s$^{-1}$. Finding a trend or its absence will 
be important in the context of the diffusion theory, which is the best explanation today for the spectroscopic characteristics of CP stars.

\vspace{0.2cm}
 
\acknowledgements

The authors acknowledge the use of the CCD and data reduction acquisition system supported by US NSF Grant AST 90-15827 
to R. M. Rich.  The authors thank Drs. R.L. Kurucz and I. Hubeny for making their codes available to them. This work was 
partially supported by a grant PICT 20269 from Agencia Nacional de Promoci\'on Cient\'ifica y Tecnol\'ogica.

\vspace{0.1cm}

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