\documentclass[journal]{rmaa}


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

\title{Atomic species in the spectrum of the Hg-Mn star HD 53244} 

\author{
N.~L. Maza,\altaffilmark{1,2}
H. Levato,\altaffilmark{1,3}
and Z. L\'opez-Garc\'ia\altaffilmark{1,3}}

\altaffiltext{1}{Instituto de Ciencias Astron\'omicas, de la Tierra y del Espacio, San Juan, Argentina.}
\altaffiltext{2}{Visiting astronomer Complejo Astron\'omico El Leoncito, Argentina.}
\altaffiltext{3}{Consejo Nacional de Investigaciones Cient\'ificas y T\'ecnicas, Argentina.} 


\fulladdresses{
\item Natalia L. Maza: Instituto de Ciencias Astron\'omicas, de la Tierra y del Espacio, Av. Espa\~na 1512 Sur, J5402DSP, San Juan, Argentina 
(nmaza@icate-conicet.gob.ar).
\item Hugo Levato: Consejo Nacional de Investigaciones Cient\'ificas y T\'ecnicas de la Rep\'ublica Argentina (hlevato@icate-conicet.gob.ar). 
\item Zulema L\'opez-Garc\'ia: Visiting Astronomer of Instituto de Ciencias Astron\'omicas, de la Tierra y del Espacio, Av.Espa\~na 1512 Sur, 
J5402DSP, San Juan, Argentina (zlgarcia@icate-conicet.gob.ar).}


\shortauthor{Maza, Levato, \& L\'opez-Garc\'ia}

\shorttitle{Line Identification of the Hg-Mn star HD 53244}


\SetYear{2010}
\SetVolume{46}
\ReceivedDate{2009 December 29} 
\AcceptedDate{2010 July 15} 

\listofauthors{N.~L.~Maza, H.~Levato, \& Z.~L\'opez-Garc\'ia}

\indexauthor{Maza, N.~L.}
\indexauthor{Levato, H.}
\indexauthor{L\'opez-Garc\'ia, Z.}

\abstract{Line identifications are presented for the Hg-Mn Bp star HD 53244 ($\gamma$CMa), in the spectral region $\lambda\lambda3750-6700$~\AA. 
This object is a member of the southern open cluster Cr 121. Comparison of the spectrum of HD 53244 with other field Hg-Mn stars shows that it 
shares many of their spectral anomalies but that also some differences exist.}

\resumen{Presentamos la identificaci\'on de l\'ineas del espectro de la estrella Bp de Hg-Mn HD 53244 ($\gamma$CMa) en el intervalo espectral 
$\lambda\lambda3700-6700$~\AA. Este objeto es miembro del c\'umulo abierto austral Cr 121. La comparaci\'on de su espectro con otros de estrellas 
de Hg-Mn de campo muestra que comparte muchas de las anomal\'ias espectrales pero tambi\'en presenta algunas diferencias.}

\addkeyword{stars: chemically peculiar}
\addkeyword{stars: line identification}
\addkeyword{stars: individual (HD 53244)}


\begin{document}

\maketitle

\section{Introduction}
\label{sec:intro}

The identification of lines in stellar spectra is one of the basic operations in stellar spectroscopy. The main purpose of this task is to 
determine the element responsible for each observed spectral line. Today, complete identification studies in which one attempts to identify 
every absorption feature are rarely done but they are badly needed. This research is part of our current program for producing line identification 
lists and elemental abundances among southern chemically peculiar (CP) stars. For this paper we selected the Hg-Mn star HD 53244. It is a 
member of the open cluster Collinder 121 \citep{feinstein67}. It was observed by Hipparcos (HIP 34045).

This peculiar star was classified as B8 II (Houk \& Cowley 1975) and B8 III in several papers in the literature. In fact, HD 53244 is a Hg-Mn 
peculiar star or CP3 in the classification scheme of \citet{1974ARA&A...12...297}. It was first classified as a manganese star of the $\alpha$And 
class by \citet{morgan33}. Some years later \citep{bidelman62a, bidelman62b} identified the nature of the line $\lambda$ 3984 \AA\ as produced 
by Hg II and HD 53244 became a Hg-Mn star. It is included as such in the catalogues of Renson, Gerbaldi, \& Catalano (1991) and \citet{schneider81}. 
$UBV$ photoelectric fotometry was published by several authors; there are more than a dozen measurements in the literature. Also, $ubvy$ photoelectric 
photometry has been provided by more than half a dozen sources. The most recent values for the $UBV$ photometry are those provided by 
\citet{fernie83}, ($B-V=-0.13$~mag, $U-B=-0.45$~mag). The $ubvy-\beta$ photometry was taken from \citet{hauck98}.

The radial velocity published by \citet{wielen00} is 32~km~s$^{-1}$ and the rotational velocity, 30~km~s$^{-1}$, was derived by Abt, Levato, \& Grosso 
(2002). Very recently \citet{briquet10} found variable line profiles of Hg line and they derived a rotation period of 6.16 days for HD 53244.

\section{Observational Material}
\label{sec:observ}

The spectra of HD 53244 were obtained by NM with the Jorge Sahade 2.15 m telescope at Complejo Astr\'onomico El Leoncito (CASLEO) and the 
EBASIM bench echelle spectrograph with a Roper Scientific $1340 \times 1310$ CCD back illuminated detector with a pixel size of 20$\mu$. Two 
spectra of the star were obtained covering the visual range $\lambda\lambda3700-5500$~\AA\ and another two covering the red portion 
$\lambda\lambda4600-6700$~\AA. The EBASIM spectrograph uses gratings as cross dispersers. We have used one grating with 226~lines~mm$^{-1}$. 
The S/N ratio of the spectra was around 300 and they were taken in March, 2008. The resolving power was 40000 at 5000~\AA. There was no more 
than a 20\% difference among the equivalent width measurements of the same lines in different orders of the echelle spectra. 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, and were normalized order by order with the {\sc continuum} task of the same package. The resolution of the spectra was 
0.04~\AA/px. Extensive description of EBASIM spectrograph has been published by \citet{sim96} and by \citet{pintado03}.


\section{Line Identifications}
\label{sec:ident}

The line identification techniques have been extensively reviewed by \citet{1990PASP...102...1077} and by \citet{1990PASP...102...587}. Also the 
subject was addressed by \citet{1995ASPCS...vol.81}. Cowley \& Adelman (1990) in particular compared the results of the classical technique for 
line identification with the WCS (wavelength coincidence statistics). As HD 53244 is an early type Bp star, we have used the classical technique 
for line identification based on the following precautions: (a) we use the highest resolution spectra on hand (EBASIM, 40000 resolving power), 
(b) we try to identify all the possible lines in the wavelength range, (c) we require that the strongest laboratory lines of each atomic 
species be present. The stellar lines were identified using the general compilation by \citet{moo} as well as the more specialized references: 
for \ion{Si}{ii} Shenstone (1961), for \ion{P}{ii} we used the NIST tables\footnote{\url{http://physics.nist.gov/cgi-bin/AtData/lines.form}.}, 
for \ion{Ti}{ii} Huldt et al. (1982), for \ion{Mn}{ii} Iglesias \& Velasco (1964), for \ion{Fe}{ii} Johansson (1978), Nave et al. (1994) and some 
few lines from Kurucz\footnote{\url{www.kurucz.havarard.edu/atoms/260l/gf2601.lines}.}, while for the rare earths we have used 
the DREAM\footnote{\url{http://www.umh.ac.be/astro/dream.shtml}.} database. We used a $\Delta$\,$\lambda$ interval of 0.15~\AA\ to search for 
the possible contributors to each spectral feature. HD 53244 is not a very low rotator. The $v \sin i$ value derived from our EBASIM spectra is 
around 30~km~s$^{-1}$ and agrees with the \citet{abt02} determination. So we chose the interval $\pm 0.15$~\AA\ because the total width due to rotation 
for lines at 4000~\AA\ is around 0.4~\AA. Empirically, it is demonstrated that on our spectra one may note the presence of a companion line with 
less than half of that value. We have not used the synthetic computation of the spectra for line identification because that technique involves theory 
and several assumptions and simplifications of the real physical situation in Bp-Ap stars. The technique we have applied has been extensively 
justified in \citet{1995ASPCS...vol.81}.


%%%%%% TABLA 1

\setcounter{table}{0}
\begin{table*}[!t]
\vspace{0.1cm}
\centering
\caption{Line Identification}
\label{tab:I}
%\setlength{\tabnotewidth}{0.99\textwidth}
\tablecols{13}
%\setlength{\tabcolsep}{0.7\tabcolsep}
\casitiny
\begin{tabular}{rclrcccrclrcc}
\toprule  
   &  & \multicolumn{4}{c}{Identification}  &   &   &   & \multicolumn{4}{c}{Identification} \\
\cmidrule{3-6}
\cmidrule{10-13}
$\lambda$ [\AA] & $W_\mathrm{eq}$ & Element & Mult. & $\lambda_\mathrm{lab}$ & Intensity &  & $\lambda$ [\AA] & $W_\mathrm{eq}$ & Element & Mult. & $\lambda_\mathrm{lab}$ & Intensity \\
\cmidrule{1-6}
\cmidrule{8-13}
3700.00  &        &	            &	    &	     &      &  &   50.40  & 0.027  & YII             &    6  & 50.35  & 1 \\
  59.22  & 0.081  & TiII            &   13  & 59.30  & 3    &  &   52.40  & 0.065  & MnII            &    I  & 52.42  & 2 \\
         &        & FeII            &  154  & 59.46  &      &  &   60.99  & 0.031  & FeII            &  212  & 60.90  & 2 \\ 
  61.48  & 0.018  & TiII            &   13  & 61.33  & 1    &  &   68.75  &        & CaII            &       &        & 4 \\
         &        & CrII            &   11  & 61.66  &      &  &   70.07  &        & H$\varepsilon$  &       &        & 6 \\
         &        & TiII            &  107  & 61.88  &      &  &   75.69  & 0.034  & MnII            &    I  & 75.74  & 1 \\
         &        & CrII            &   11  & 61.85  &      &  &   79.48  & 0.037  & CrII            &  183  & 79.51  & 1 \\
  63.79  & 0.037  & MnII            &    I  & 63.76  & 2    &  &   83.91  & 0.009  & HgII            &       & 83.94  & 1 \\
  65.63  & 0.014  & CrII            &   20  & 65.56  & 1    &  &   86.22  & 0.031  &                 &       &        & 1 \\  
  67.89  & 0.028  & MnII            &    I  & 67.94  & 1    &  &   87.68  & 0.011  & TiII            &   11  & 87.61  & 1 \\
  68.78  & 0.009  & HeI             &   65  & 68.81  & 1/2  &  &   91.20  & 0.030  & ZrII ?          &   30  & 91.14  & 1 \\
  70.69  &        & H11             &       &        & 7    &  &   95.31  & 0.014  & MnII            &    I  & 95.32  & 1 \\
  78.32  & 0.054  & MnII            &    I  & 78.32  & 2    &  &   99.84  & 0.013  &                 &       &        & 1 \\
  79.62  & 0.019  & FeII            &   23  & 79.58  & 1    &  &          &        &                 &       &        &   \\ 
  83.33  & 0.100  & FeII            &   14  & 83.35  & 3    &  & 4000.00  &        &                 &       &        &   \\
  84.23  & 0.092  & CeIII ?         &       &        & 3    &  &   00.02  & 0.006  & MnII            &    I  & 00.04  & 1/2 \\
  97.90  &        & H10             &       &        & 7    &  &   02.58  & 0.030  & FeII            &  190  & ~2.54  & 1 \\ 
  98.28  & 0.049  & FeII            &   14  & 98.28  & 2    &  &          &        & CrII            &  166  & ~2.48  &   \\
         &        &                 &       &        &      &  &   03.62  & 0.013  &                 &       &        & 1 \\
3800.00  &        &                 &       &        &      &  &   04.69  & 0.021  &                 &       &        & 1 \\
  01.38  & 0.022  & MnII            &    I  & 01.63  & 1    &  &   09.35  & 0.042  & HeI             &       & 09.25  & 1 \\
         &        & CrII            &    -  & 01.21  & 3    &  &   12.45  & 0.019  & TiII            &   11  & 12.40  & 1 \\
  12.36  & 0.013  & MnII            &    I  & 12.24  & 1    &  &          &        & CrII            &  183  & 12.50  &   \\
         &        & MnII            &    I  & 12.52  &      &  &   15.50  & 0.037  & NiII            &   12  & 15.50  & 2 \\ 
  14.19  & 0.025  & FeII            &  153  & 14.12  & 1    &  &   18.24  & 0.018  & ZrII ?          &   54  & 18.38  & 1 \\
  17.30  & 0.024  & MnII            &    I  & 17.26  & 1    &  &   20.95  & 0.041  &                 &       &        & 2 \\
  19.55  & 0.087  & HeI             &       &        & 3    &  &   26.06  &        & HeI             &       &        & 6 \\
  20.43  & 0.042  & FeI             &   20  & 20.43  & 2    &  &   28.41  & 0.012  & TiII            &   87  & 28.36  & 1 \\
  24.84  & 0.059  & FeII            &   29  & 24.91  & 2    &  &   32.95  & 0.021  & FeII            &  126  & 32.95  & 1 \\
         &        & MnII            &    I  & 25.04  &      &  &   34.06  & 0.016  & ZrII ?          &   42  & 34.10  & 1 \\
  27.08  & 0.014  & FeII            &  153  & 27.08  & 1    &  &   37.91  & 0.032  & CrII            &  194  & 37.98  & 1 \\ 
  35.39  &        & H9              &       &        & 8    &  &   40.26  & 0.018  & ZrII            &   54  & 40.24  & 1 \\
  38.80  & 0.024  & MnII            &    I  & 39.05  & 1    &  &   44.44  & 0.061  & PII             &   30  & 44.49  & 2 \\
  41.79  & 0.019  &                 &       &        &      &  &   48.81  & 0.032  & FeII            &  172  & 48.83  & 1 \\
  42.99  & 0.025  & ZrII            &    7  & 43.03  & 1    &  &   50.60  & 0.027  &                 &       &        &   \\
  43.26  & 0.010  & MnII            &    I  & 43.32  & 1    &  &   53.97  & 0.012  & TiII            &   87  & 53.83  & 1 \\
  44.10  & 0.022  & MnII            &    I  & 44.17  & 1    &  &          &        & CrII            &   19  & 54.09  &   \\
  45.17  & 0.072  & FeII            &  127  & 45.18  & 2    &  &   57.46  & 0.051  & FeII            &  212  & 57.46  & 2 \\
  48.24  & 0.059  & MgII            &    5  & 48.24  & 2    &  &   61.76  & 0.020  & FeII            &  189  & 61.79  & 1 \\
  49.51  & 0.035  & NiII            &   11  & 49.58  & 2    &  &   63.85  & 0.029  &                 &       &        &   \\
  50.95  & 0.034  & OII             &   NI  & 51.03  & 1    &  &   64.48  & 0.028  & FeII            &   29  & 64.57  & 1 \\
         &        & SII             &   50  & 50.93  &      &  &          &        & TiII            &  106  & 64.35  &   \\
  53.58  & 0.041  & SiII            &    1  & 53.66  & 2    &  &   65.40  & 0.015  &                 &       &        & 1 \\
  56.00  & 0.078  & SiII            &    1  & 56.02  & 4    &  &   66.94  & 0.054  & NiII            &   11  & 67.05  & 2 \\
  60.92  & 0.014  & FeII            &    0  & 60.92  & 1    &  &   69.96  & 0.014  & FeII            &  188  & 69.88  & 1 \\
  62.55  & 0.084  & SiII            &    1  & 62.60  & 3    &  &   72.48  & 0.027  & CrII            &   26  & 72.56  & 1 \\ 
  63.95  & 0.016  & FeII            &       & 63.95  & 1    &  &   73.76  & 0.031  &                 &       &        & 1 \\
  65.74  & 0.021  & CrII            &  167  & 65.60  & 1    &  &   75.43  & 0.028  & SiII            & 3.01  & 75.45  & 1 \\
         &        & CrII            &  130  & 65.99  &      &  &   78.50  & 0.013  &                 &       &        & 1 \\
  67.56  & 0.022  & HeI             &   20  & 67.48  & 1    &  &   80.94  & 0.080  &                 &       &        & 2 \\
         &        & HeI             &   20  & 67.63  &      &  &   83.63  & 0.100  & MnII            &    I  & 83.66  & 3 \\
  71.82  & 0.035  & HeI             &   60  & 71.82  & 1    &  &          &        &                 &       &        &   \\
  78.90  & 0.037  & MnII            &    I  & 79.00  & 1    &  & 4100.00  &        &                 &       &        &   \\
  88.65  & 0.007  & HeI             &    2  & 88.65  & 1/2  &  &   01.76  &        & H$\delta$       &       &        & 6 \\ 
  89.05  &        & H8              &       &        & 6    &  &   07.90  & 0.022  &                 &       &        & 1 \\
         &        &                 &       &        &      &  &   09.30  & 0.059  & MnII ?          &    I  & 09.20  & 2 \\
3900.00  &        &                 &       &        &      &  &   10.72  & 0.111  & MnII            &    I  & 10.62  & 2 \\  
  00.48  & 0.028  & TiII            &   34  & 00.56  & 1    &  &          &        & CrII            &   18  & 11.01  &   \\
  05.94  & 0.075  & FeII            &  173  & 06.04  & 2    &  &   20.90  & 0.028  & HeI             &       &        & 1 \\   
         &        & CrII            &  167  & 05.64  &      &  &   22.69  & 0.019  & FeII            &   28  & 22.64  & 1 \\
  11.76  & 0.018  &                 &       &        &      &  &   24.75  & 0.013  & FeII            &   22  & 24.79  & 1 \\     
  13.48  & 0.056  & TiII            &   34  & 13.48  & 2    &  &   28.05  & 0.132  & SiII            &    3  & 28.07  & 4 \\
  17.25  & 0.020  & MnII            &    I  & 17.32  & 1    &  &   30.85  & 0.092  & SiII            &    3  & 30.89  & 4 \\
  19.03  & 0.036  & CII             &    4  & 18.98  & 1    &  &   36.90  & 0.020  & MnII            &    I  & 36.90  & 1 \\
  20.66  & 0.048  & CII             &    4  & 20.68  & 2    &  &   40.37  & 0.022  & MnII            &    I  & 40.44  & 1 \\
  26.51  & 0.052  & HeI             &   68  & 26.53  & 2    &  &   43.80  & 0.039  & HeI             &       &        & 1 \\
  32.09  & 0.040  & TiII            &   34  & 32.02  & 1    &  &   45.68  & 0.013  & CrII            &  162  & 45.77  & 1 \\ 
  33.62  & 0.145  & CaII            &       &        & 5    &  &   49.33  & 0.065  & ZrII ?          &   41  & 49.22  & 2 \\
  35.91  & 0.032  & HeI             &   57  & 35.91  & 1    &  &   53.20  & 0.010  & SII             &   44  & 53.10  & 1 \\
  38.92  & 0.037  & FeII            &  190  & 38.97  & 1    &  &   63.62  & 0.019  & TiII            &  105  & 63.63  & 1 \\
  47.38  & 0.043  & OI              &    3  & 47.29  & 1    &  &   67.24  & 0.040  & FeII            &  K88  & 67.30  & 1 \\
\bottomrule
\end{tabular}
\end{table*}

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


%%%%% PAGINA 2 TABLA 1 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

\setcounter{table}{0}
\begin{table*}[!t]
\vspace{0.1cm}
\centering
\centerline{TABLE~1 (CONTINUED)\smallskip}
%\setlength{\tabnotewidth}{0.99\textwidth}
\tablecols{6}
%\setlength{\tabcolsep}{0.7\tabcolsep}
\casitiny
\begin{tabular}{rclrcccrclrcc}
\toprule  
   &  & \multicolumn{4}{c}{Identification}  &   &   &   & \multicolumn{4}{c}{Identification} \\
\cmidrule{3-6}
\cmidrule{10-13}
$\lambda$ [\AA] & $W_\mathrm{eq}$ & Element & Mult. & $\lambda_\mathrm{lab}$ & Intensity &  & $\lambda$ [\AA] & $W_\mathrm{eq}$ & Element & Mult. & $\lambda_\mathrm{lab}$ & Intensity \\
\cmidrule{1-6}
\cmidrule{8-13}
         &        & FeIII           &  118  & 66.86     &      &  &   65.22  & 0.030  & MnII            &     I &65.22     &1\\
  71.54  & 0.039  & MnII            &    I  & 71.51     & 2    &  &   67.69  & 0.011  & TiII            &   105 &67.65     & 1\\
  73.59  & 0.090  & FeII            &   27  & 73.45     & 2    &  &   69.36  & 0.006  & FeII            &    28 &69.40     &  1/2\\
         &        & TiII            &   21  & 73.53     &      &  &   73.03  & 0.018  &                 &       &          &1\\
  78.67  & 0.058  & FeII            &   28  & 78.86     & 2    &  &   74.59  & 0.016  & TiII            &    93 &74.84     & 1\\
         &        & PII             &    S  & 78.46     &      &  &          &        & ScII            &    14 &74.46     & \\
  81.75  & 0.016  & CrII            &  181  & 81.50     & 1    &  &          &        & YII             &   13&74.94     & \\
  84.54  & 0.013  & MnII            &    I  & 84.45     & 1    &  &   79.64  & 0.014  & MnII            &     I &79.67     & 1\\
  91.32  & 0.030  &                 &       &           & 1    &  &   84.56  & 0.026  & MgII            &    10 &84.64     &  1\\
         &        &                 &       &           &      &  &   85.34  & 0.034  & FeII            &    27 &85.39     &  1\\     
4200.00  &        &                 &       &           &      &  &          &        & PII             &   NI &85.31     &\\
  00.28  & 0.029  & MnII            &    I  & 00.27     & 1    &  &   87.88  & 0.098  & HeI             &       &87.93    &3\\
  03.08  & 0.016  & FeII            &  K88  & 02.99     & 1    &  &   90.57  & 0.013  & MgII            &    10 &90.58     & 1\\
  05.37  & 0.034  & MnII            &    I  & 05.38     & 1    &  &   93.33  & 0.032  & MnII            &     I &93.38     & 1\\ 
  06.31  & 0.056  & MnII            &    I  & 06.37     & 2    &  &   94.96  & 0.043  & TiII            &    19 &95.00     & 2\\
  22.26  & 0.012  & CrII            &  180  & 22.00     & 1    &  &   95.77  & 0.008  & FeIII           &    4 &95.78     & 1 \\
  24.62  & 0.032  & CrII            &   31  & 24.08     & 1    &  &   99.80  & 0.026  & TiII            &    51 &99.79     & 1      \\
         &        & CrII            &  162  & 24.89     &      &  &          &        &                 &       &          &  \\   
  33.14  & 0.057  & FeII            &   27  & 33.17     & 2    &  & 4400.00  &        &                 &       &          &\\
         &        & CrII            &   31  & 33.27     &      &  &   00.74  & 0.020  &                 &       &          &   1\\
  35.16  & 0.012  &                 &       &           & 1    &  &   07.74  & 0.004  & TiII            &    51 &07.68     &  1 \\
  35.62  & 0.027  & YII             &    5  & 35.73     & 1    &  &   09.49  & 0.007  & TiII            &    61 &09.51     &  1\\
         &        & FeII            &  K88  & 35.39     &      &  &   11.10  & 0.009  & TiII            &   115 &11.10    & 1\\
  37.95  & 0.014  & MnII            &    I  & 37.87     & 1    &  &   11.99  & 0.003  & TiII            &   61&11.92     & 1\\
  38.80  & 0.022  & MnII            &    I  & 38.79     & 1    &  &   15.20  & 0.003  & FeI             &   41 &15.12      &  1   \\ 
  42.36  & 0.056  & MnII            &    I  & 42.33     & 1    &  &   16.80  & 0.035  & FeII            &    27 &16.83     &  1\\
         &        & CrII            &   31  & 42.38     &      &  &   17.76  & 0.002  & TiII            &    40 &17.72     & 1\\
  44.23  & 0.023  & MnII            &    I  & 44.25     & 1    &  &   19.41  & 0.007  & {FeIII}         &     4 &19.59     & 1\\
  46.55  & 0.073  & ScII ?          &    7  & 46.83     & 2    &  &   20.73  & 0.019  & PII             &   NI &20.71     &1\\
         &        & CrII            &   31  & 46.41     &      &  &   27.92  & 0.017  & MgII            &     9 &28.00     &  1  \\
  50.44  & 0.013  & FeII            &    K  & 50.44     & 1    &  &   30.93  & 0.012  & FeIII           &     4 &30.95     &  1  \\
  51.73  & 0.043  & MnII            &    I  & 51.74     & 2    &  &   34.03  & 0.019  & MgII            &     9 &33.99     &  1\\
  52.97  & 0.045  & MnII            &    I  & 52.96     & 2    &  &          &        & MnII            &     I &34.06     &  \\
  54.47  & 0.004  & CrII            &    D  & 54.52     & 1    &  &   37.51  & 0.017  & HeI             &       &          & 1 \\
  59.07  & 0.029  & MnII            &    I  & 59.20     & 1    &  &   41.84  & 0.007  & TiII            &    40 &41.73     & 1\\
  61.99  & 0.022  & CrII            &   31  & 61.92     & 1    &  &   43.76  & 0.039  & TiII            &    19 &43.78     & 1    \\ 
  63.89  & 0.012  & FeII            &    J  & 63.90     & 1    &  &   50.43  & 0.015  & TiII            &    19 &50.50     & 1\\
  67.19  & 0.061  & CII             &    6  & 67.02,.27 & 2    &  &   51.53  & 0.008  & FeII            &       &51.55     &  1\\
  70.84  & 0.014  &                 &       &           & 1    &  &   55.26  & 0.009  & FeII            &     J &55.27     &  1\\
  73.31  & 0.019  & FeII            &   27  & 73.32     & 1    &  &   61.93  & 0.015  &                 &       &          &  1\\
  75.59  & 0.029  & CrII            &   31  & 75.57     & 1    &  &   63.07  & 0.017  &                 &       &          &   1\\
  78.38  & 0.008  & SII             &   40  & 78.50     & 1/2  &  &   68.49  & 0.043  & TiII            &    31 &68.52     & 1  \\
  82.45  & 0.044  & MnII            &    I  & 82.47     & 2    &  &   71.51  & 0.182  & HeI             &       &          &5\\
  83.94  & 0.039  & CrII            &   31  & 84.21     & 1    &  &   75.24  & 0.013  & PII             &   NI &75.26     &1\\
         &        & MnII            &    I  & 83.77     &      &  &   78.64  & 0.026  & MnII            &     I &78.64     &1\\
  86.24  & 0.004  & FeII            &    J  & 86.31     & 1/2  &  &   81.17  & 0.187  & MgII            &     4 &81.13     & 6\\
  87.95  & 0.022  & TiII            &   20  & 87.88     & 1    &  &          &        & MgII            &     4 &81.33     & \\
         &        & MnII            &    I  & 88.07     &      &  &   89.14  & 0.028  & FeII            &    37 &89.18     &1\\
  90.19  & 0.042  & TiII            &   41  & 90.22     & 2    &  &          &        & CrII            &     J &89.11     &  \\
  92.24  & 0.036  & MnII            &    I  & 92.24     & 2    &  &   91.38  & 0.029  & FeII            &    37 &91.40     &  1\\
  94.24  & 0.024  & TiII            &   20  & 94.09     & 1    &  &   93.68  & 0.011  & TiII            &    18 &93.53     &  1\\
         &        & SII             &   49  & 94.43     &      &  &          &        & FeII            &   222 &93.58     &  \\
  96.57  & 0.026  & FeII            &   28  & 96.57     & 1    &  &   99.31  & 0.029  & PII             &   NI &99.24     &1\\
         &        &                 &       &           &      &  &          &        &                 &        &        &  \\ 
4300.00  &        &                 &       &           &      &  & 4500.00  &        &                 &      &          &\\
  00.08  & 0.037  & TiII            &   41  & 00.06     & 2    &  &   01.31  & 0.037  & TiII            &   31& 01.27    &  1\\
  03.10  & 0.044  & FeII            &   27  & 00.17     & 2    &  &   08.24  & 0.038  & FeII            &   38& 08.28    &   2\\
  07.96  & 0.047  & MnII            &    I  & 08.16     & 2    &  &   15.29  & 0.039  & FeII            &   37& 15.34    &   2\\
         &        & TiII            &   41  & 07.87     &      &  &   18.99  & 0.012  & MnII            &    I& 18.96    & 1\\
  09.52  & 0.003  & YII             &    5  & 09.62     & 1    &  &   20.20  & 0.030  & FeII            &   37& 20.22    &  1\\ 
  12.91  & 0.013  & TiII            &   41  & 12.87     & 1    &  &   22.57  & 0.046  & FeII            &   38& 22.63    &   2\\
  14.46  & 0.013  & MnII            &    I  & 14.38     & 1    &  &   24.83  & 0.018  & SII             &  45 &24.95     & 1\\
  15.10  & 0.006  & TiII            &   41  & 14.97     & 1    &  &   29.55  & 0.003  & TiI             &   82& 29.48    &  1\\
  20.69  & 0.008  & ScII            &   15  & 20.74     & 1    &  &   33.98  & 0.030  & TiII            &   50& 33.97    &   1\\
  25.06  & 0.007  & MnII            &    I  & 25.04     & 1    &  &   39.54  & 0.009  & CrII            &   39& 39.62    &   1\\
  26.63  & 0.045  & MnII            &    I  & 26.64     & 3    &  &   41.51  & 0.022  & FeII            &   38& 41.53    &   1\\
  30.13  & 0.011  & TiII            &   94  & 30.23     & 1    &  &   46.66  & 0.014  & CrII            &   J& 46.62    &  1\\
  40.47  &        & H$\gamma$       &       &           & 6    &  &   49.42  & 0.100  & FeII            &  186& 49.21    &   4\\
  43.92  & 0.054  & MnII            &    I  & 43.98     & 2    &  &          &        & FeII            &   38& 49.47    &  \\
  48.42  & 0.030  & MnII            &    I  & 48.40     & 1    &  &          &        & TiII            &   82& 49.62    &  \\
  51.79  & 0.053  & FeII            &   27  & 51.77     & 2    &  &   52.42  & 0.010  & SiIII           &    2& 52.62    &  1 \\ 
  56.62  & 0.018  & MnII            &    I  & 56.62     & 1    &  &          &        & SII             &  48 &52.38     &  \\
  63.22  & 0.019  & MnII            &    I  & 63.26     & 1    &  &   55.07  & 0.015  & CrII            &   44& 55.02    &  1 \\
\bottomrule
\end{tabular}
\end{table*}

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


%%%%% PAGINA 3 TABLA 1 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

\setcounter{table}{0}
\begin{table*}[!t]
\vspace{0.1cm}
\centering
\centerline{TABLE~1 (CONTINUED)\smallskip}
%\setlength{\tabnotewidth}{0.99\textwidth}
\tablecols{6}
%\setlength{\tabcolsep}{0.7\tabcolsep}
\casitiny
\begin{tabular}{rclrcccrclrcc}
\toprule  
   &  & \multicolumn{4}{c}{Identification}  &   &   &   & \multicolumn{4}{c}{Identification} \\
\cmidrule{3-6}
\cmidrule{10-13}
$\lambda$ [\AA] & $W_\mathrm{eq}$ & Element & Mult. & $\lambda_\mathrm{lab}$ & Intensity &  & $\lambda$ [\AA] & $W_\mathrm{eq}$ & Element & Mult. & $\lambda_\mathrm{lab}$ & Intensity \\
\cmidrule{1-6}
\cmidrule{8-13}
  55.92  & 0.013  & FeII            &   37  & 55.89  & 2    &  & 4900.00  &        &                 &        &      &\\
  58.56  & 0.048  & CrII            &   44  & 58.66  & 2    &  &   01.60  & 0.013  & CrII            &  190 &01.65  &     1\\
  63.77  & 0.024  & TiII            &   50  & 63.72  & 1    &  &   11.13  & 0.015  & TiII            &    114& 11.18&      1 \\
  65.74  & 0.010  & CrII            &   30  & 65.77  & 1    &  &   13.29  & 0.020  & FeII            &      J& 13.29&       1\\ 
  67.87  & 0.008  & SiIII           &    2  & 67.83  & 1/2  &  &   21.77  & 0.133  & HeI             &       &      &3\\
  71.89  & 0.034  & TiII            &   82  & 71.96  & 1    &  &   23.87  & 0.063  & FeII            &    42 &23.93 &     2\\
  74.86  & 0.005  & SiIII           &    2  & 74.76  & 1/2  &  &   31.30  & 0.018  &                 &       &      &1\\
  76.39  & 0.029  & FeII            &   38  & 76.33  & 1    &  &   43.51  & 0.021  & PII             &   NI &43.53  & 1\\
  79.58  & 0.007  & FeII            &    J  & 79.52  & 1    &  &   48.80  & 0.010  & FeII            &     J &48.80 &  1\\
  82.87  & 0.020  & FeII            &   37  & 82.84  & 1    &  &   51.52  & 0.014  & FeII            &     J &51.59 &     1\\
  83.80  & 0.074  & FeII            &   38  & 83.83  & 2    &  &   54.18  & 0.011  & FeII            &     J &53.98 & 1\\
  88.13  & 0.027  & PII             &   NI  & 88.04  & 3    &  &   69.63  & 0.039  & PII             &   NI &69.71  &   1\\
         &        & CrII            &   44  & 88.22  &      &  &   76.95  & 0.019  & FeII            &     J &77.04 &     1\\
  89.83  & 0.031  & CrII            &   44  & 89.89  & 1    &  &   77.50  & 0.038  & FeII            &     J &77.03 & 1\\
         &        & PII             &   NI  & 89.86  &      &  &          &        & FeII            &     J &77.93 & \\
  92.03  & 0.023  & CrII            &   44  & 92.07  & 1    &  &   80.14  & 0.006  &                 &       &      &      1\\
  96.02  & 0.021  & FeII            &    D  & 96.02  & 1    &  &   84.49  & 0.010  & FeII            &     J &84.49 &     1\\
  98.39  & 0.013  & FeII            &  219  & 98.53  & 1    &  &   90.59  & 0.012  & FeII            &     J &90.51 &     1\\
         &        &                 &       &        &      &  &   91.66  & 0.010  &                 &       &      & 1\\ 
4600.00  &        &                 &       &        &      &  &   93.36  & 0.003  & FeII            &     J &93.35 &      1\\
  02.04  & 0.034  & P II            &   NI  & 02.08  & 1    &  &          &        &                 &        &     & \\   
  00.44  & 0.029  &                 &       &        & 1    &  & 5000.00  &        &                 &       &      &\\
  16.60  & 0.022  & CrII            &   44  & 16.64  & 1    &  &   01.90  & 0.034  & FeII            &   J &01.92  &   2\\
  18.78  & 0.023  & CrII            &   44  & 18.82  & 1    &  &   04.22  & 0.025  & FeII            &    J &04.20 &    1\\  
  20.56  & 0.017  & FeII            &   38  & 20.52  & 1    &  &   07.40  & 0.030  & FeII            &    J &07.45 &    1 \\
  21.65  & 0.023  & SiII            & 7.05  & 21.42  & 1    &  &   09.54  & 0.012  & SII             &  \textbf{7} &09.54  &    1\\
         &        &                 &       & 21.72  &      &  &   15.73  & 0.056  & FeII            &    J &15.75 &    2\\
  25.86  & 0.002  & FeII            &  186  & 25.91  & 1    &  &   18.41  & 0.080  & FeII            &    J &18.45 &    3\\  
  29.26  & 0.037  & FeII            &   37  & 29.34  & 1    &  &   21.60  & 0.010  & FeII            &    J &21.59 &    1\\
  31.99  & 0.003  & FeII            &  219  & 31.90  & 1    &  &   22.77  & 0.018  & FeII            &    J &22.79 &    1 \\
  34.12  & 0.020  & CrII            &   44  & 34.16  & 1    &  &   26.90  & 0.013  & FeII            &    J &26.80 &     1\\
  35.27  & 0.022  & FeII            &  186  & 35.32  & 1    &  &   30.67  & 0.030  & FeII            &   J &30.63 &    1\\
  40.91  & 0.004  & FeII            &    J  & 40.84  & 1    &  &   32.40  & 0.017  & SII             & \textbf{7} &32.41  &    1\\
  56.99  & 0.007  & FeII            &   43  & 56.98  & 1/2  &  &   35.68  & 0.027  & FeII            &   J &35.71 &    1\\
  58.36  & 0.011  & PII             &   NI  & 58.31  & 1    &  &   40.96  & 0.086  & SiII            &   5 &41.02&3\\
  66.70  & 0.008  & FeII            &   37  & 66.75  & 1/2  &  &   47.66  & 0.029  & FeII            &   J &47.64 &     1 \\
  70.13  & 0.010  & FeII            &   25  & 70.18  & 1/2  &  &          &        & HeI             &     &       &   \\
  73.16  & 0.017  & SiII            & 7.15  & 73.27  & 1    &  &   56.16  & 0.122  & SiII            &   5 &55.98&4\\
         &        &                 &       &        &      &  &          &        & SiII            &   5 &56.32 &     \\
4700.00  &        &                 &       &        &      &  &   61.64  & 0.018  & FeII            &   J &61.72 &1\\ 
  08.72  & 0.043  & NeI             &   11  & 08.85  & 2    &  &   67.79  & 0.018  & FeII            &   J &67.89 & 1\\
  13.18  & 0.045  & HeI             &       &        & 2    &  &   75.74  & 0.024  & FeII            &   J &75.76 &    1\\
  16.16  & 0.008  & SII             &    9  & 16.27  & 1/2  &  &   82.22  & 0.013  & FeII            &   J &82.23 &     1\\
  17.30  & 0.016  & MnII            &    I  & 17.26  & 1    &  &   89.17  & 0.012  & FeII            &   J &89.21 &     1\\
  27.77  & 0.036  & MnII            &    I  & 27.84  & 1    &  &   93.54  & 0.023  & FeII            &   J &93.56 &     1\\
  30.36  & 0.022  & MnII            &    I  & 30.40  & 1    &  &   97.24  & 0.018  & FeII            &   J &97.27 &    1 \\
  31.52  & 0.011  & FeII            &   43  & 31.45  & 1    &  &          &        &                 &     &      & \\
  38.20  & 0.045  & MnII            &    I  & 38.29  & 2    &  & 5100.00  &        &                 &     &      &\\
         &        & MnII            &    I  & 38.29  &      &  &   00.72  & 0.056  & FeII            &   J &00.74 &     2\\
  55.71  & 0.054  & MnII            &    I  & 55.73  & 3    &  &   02.47  & 0.029  & MnII            &   I &02.52 &      1\\
  64.74  & 0.054  & MnII            &    I  & 64.73  & 2    &  &   03.30  & 0.004  & SII             &  7  &3.30  &     1/2\\ 
  70.15  & 0.033  &                 &       &        & 1    &  &   06.16  & 0.021  & FeII            &   J &06.11 &      1\\
  76.47  & 0.025  &                 &       &        & 1    &  &   23.19  & 0.020  & FeII            &   J &23.19 &      1\\
  79.89  & 0.020  & TiII            &   92  & 79.98  & 1    &  &   27.50  & 0.018  & FeII            &   J &27.85 & 1\\
  84.56  & 0.025  &                 &       &        & 1    &  &   44.16  & 0.012  & FeII            &   J &43.88 &      1\\
  91.76  & 0.011  & MnII            &    I  & 91.81  & 1    &  &          &        & FeII            &   J &44.36 &     \\
         &        &                 &       &        &      &  &   45.71  & 0.010  & FeII            &   J &45.78  &    1\\
4800.00  &        &                 &       &        &      &  &   49.24  & 0.036  & FeII            &   J &48.94  &     2\\
  04.90  & 0.013  & TiII            &   92  & 05.09  & 1    &  &          &        & FeII            &   J &49.46  &    \\
         &        & FeII            &    J  & 04.73  &      &  &   57.58  & 0.024  & FeII            &   J &57.51  &    1\\
  06.86  & 0.026  & MnII            &    I  & 06.82  & 1    &  &   60.87  & 0.016  & FeII            &   J &60.85  &     1\\
  11.91  & 0.023  & MnII            &    I  & 11.62  & 1    &  &   63.22  & 0.013  & FeII            &   J &63.00  &     1\\
         &        & CrII            &   30  & 12.36  &      &  &          &        & FeII            &   J &63.58  &     \\
  15.61  & 0.012  & SII             &    9  & 15.55  & 1    &  &   66.47  & 0.020  & FeII            &   J &66.56  &     1\\
  24.08  & 0.032  & CrII            &   30  & 24.13  & 2    &  &   69.00  & 0.080  & FeII            &   J &69.03  &    3 \\
  26.63  & 0.017  & FeII            &    J  & 26.68  & 1    &  &   77.46  & 0.042  & FeII            &   J &77.39  &     2\\
  30.17  & 0.011  & MnII            &    I  & 30.06  & 1    &  &          &        & MnII            &   I &77.65  &     \\
  36.13  & 0.008  & CrII            &   30  & 36.22  & 1    &  &   83.51  & 0.014  & MgI             &   2 &83.60  &   1\\
  47.67  & 0.019  & MnII            &    I  & 47.61  & 1    &  &   85.86  & 0.018  & TiII            &  86 &85.90  &    1 \\ 
  48.28  & 0.017  & CrII            &   30  & 48.24  & 1    &  &   91.48  & 0.023  & PII             & NI &91.41   &  1  \\
  61.33  &        & H$\beta$        &       &        & 6    &  &   97.56  & 0.036  & FeII            &     &97.58  &   2\\
  76.41  & 0.029  & CrII            &   30  & 76.41  & 1    &  &   99.16  & 0.009  & FeII            &   J &99.12  &    1\\
  83.25  & 0.011  & FeII            &    J  & 83.28  & 1    &  &          &        &                 &     &       &  \\
\bottomrule
\end{tabular}
\end{table*}


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


%%%%% PAGINA 4 TABLA 1 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

\setcounter{table}{0}
\begin{table*}[!t]
\vspace{0.1cm}
\centering
\centerline{TABLE~1 (CONTINUED)\smallskip}
%\setlength{\tabnotewidth}{0.99\textwidth}
\tablecols{13}
%\setlength{\tabcolsep}{0.7\tabcolsep}
\casitiny
\begin{tabular}{rclrcccrclrcc}
\toprule  
   &  & \multicolumn{4}{c}{Identification}  &   &   &   & \multicolumn{4}{c}{Identification} \\
\cmidrule{3-6}
\cmidrule{10-13}
$\lambda$ [\AA] & $W_\mathrm{eq}$ & Element & Mult. & $\lambda_\mathrm{lab}$ & Intensity &  & $\lambda$ [\AA] & $W_\mathrm{eq}$ & Element & Mult. & $\lambda_\mathrm{lab}$ & Intensity \\
\cmidrule{1-6}
\cmidrule{8-13}
5200.00  &        &                 &       &        &      &  &          &        & FeII            &   J& 93.59 &    \\
  01.00  & 0.012  & FeII            &    J  & 00.81  & 1    &  &   95.92  & 0.019  & FeII            &   J& 95.86 &     1\\
  02.40  & 0.010  & SiII            &   23  & 02.41  & 1    &  &          &        &                 &   &        & \\
         &        & SiII            &   23  & 02.41  &      &  & 5400.00  &        &                 &    &       &\\
  03.69  & 0.018  & FeII            &    J  & 03.64  & 1    &  &   02.00  & 0.033  & FeII            &   J& 02.06 & 1\\
  12.70  & 0.001  & SII             &   39  & 12.61  & 1    &  &   05.19  & 0.012  & FeII            &   J& 05.10 &      1 \\
  13.87  & 0.015  & FeII            &    J  & 13.99  & 1    &  &   08.76  & 0.024  & FeII            &   J&  8.81 &      1\\
  15.54  & 0.028  & FeII            &    J  & 15.34  & 1    &  &   09.70  & 0.031  & PII             & NI &09.72  &   1\\
         &        & FeII            &    J  & 15.82  &      &  &   14.53  & 0.028  & FeII            &   J& 14.05 &    1\\
  16.77  & 0.028  & FeII            &    J  & 16.85  & 2    &  &          &        & FeII            &   J& 14.84 &      \\
  18.88  & 0.008  & FeII            &       & 18.84  & 1    &  &   19.19  & 0.017  & XeII            &  NI& 19.15 & 1    \\
  25.56  & 0.032  & FeII            &    J  & 25.25  & 1    &  &   21.92  & 0.015  & MnII            &   I& 21.92&1\\
         &        & FeII            &    J  & 25.36  &      &  &   25.82  & 0.067  & FeII            &   J& 25.82 &    2\\
         &        & FeII            &    J  & 25.98  &      &  &          &        & PII             & NI &25.88  &   \\
  27.43  & 0.037  & FeII            &    J  & 27.48  & 2    &  &   27.70  & 0.008  & FeII            &   J& 27.82 &   1\\
  32.90  & 0.020  & FeII            &    J  & 32.78  & 1    &  &   29.90  & 0.014  & FeII            &   J& 29.99 &     1\\
  34.53  & 0.049  & FeII            &    J  & 34.29  & 2    &  &   32.85  & 0.019  & SII             &   6& 32.82 &     1 \\
         &        & FeII            &    J  & 34.62  &      &  &   42.35  & 0.005  & FeII            &    & 42.35 &      1/2\\
  37.62  & 0.023  & CrII            &   43  & 37.34  & 1    &  &   44.43  & 0.012  & FeII            &   J &44.39 &      1\\
         &        & FeII            &    J  & 37.95  &      &  &   45.87  & 0.013  & FeII            &  J &45.81 &      1\\
  39.71  & 0.013  & FeII            &    J  & 39.81  & 1    &  &   50.68  & 0.019  & PII             & NI &50.74  &   1\\
  41.14  & 0.015  & FeII            &    J  & 41.08  & 1    &  &   53.86  & 0.015  & SII             &  6 &53.83 &    1\\
  43.03  & 0.006  & FeIII           &  113  & 43.3   & 1    &  &   66.40  & 0.050  & SiII            & 7.03 &66.43 &   2   \\
  45.12  & 0.015  & FeII            &    J  & 45.08  & 1    &  &   72.84  & 0.014  & FeII            & J &72.86 &    1\\
  46.75  & 0.003  & CrII            &   23  & 46.75  & 1/2  &  &   75.79  & 0.009  & FeII            & J &75.83 &     1\\
  47.94  & 0.021  & FeII            &    J  & 47.95  & 1    &  &   82.30  & 0.019  & FeII            & J &82.31 &     1\\
  49.40  & 0.017  & CrII            &   23  & 49.40  & 1    &  &   87.66  & 0.023  & FeII            & J &87.62 &     1\\
  51.32  & 0.027  & FeII            &    J  & 51.23  & 1    &  &   92.14  & 0.018  & FeII            & J &92.08 &      1\\
  53.46  & 0.068  & FeII            &    J  & 53.64  & 2    &  &          &        & FeII            & J &92.40 &     \\
         &        & PII             &   NI  & 53.52  &      &  &   93.66  & 0.011  & FeII            & J &93.63 &     1\\
  54.77  & 0.010  & FeII            &    J  & 54.64  & 1    &  &   98.53  & 0.015  & FeII            & J &98.57 &      1\\
  57.25  & 0.020  & FeII            &    J  & 57.11  & 1    &  &   99.77  & 0.033  & PII             & NI &99.73  &   1\\
  60.25  & 0.041  & FeII            &    J  & 60.26  & 2    &  &          &        &                 &    &      &  \\
  64.34  & 0.043  & FeII            &    J  & 64.18  & 2    &  & 5500.00  &        &                 &    &      &\\
         &        & FeII            &    J  & 64.80  &      &  &   02.99  & 0.024  & FeII            &   J& 02.68&   1\\
  69.98  & 0.015  & FeII            &    J  & 70.03  & 1    &  &          &        & FeII            &   J& 03.22&      \\ 
  72.35  & 0.018  & FeII            &    J  & 72.40  & 1    &  &   06.27  & 0.036  & FeII            &    & 06.20&   2\\
  75.91  & 0.060  & FeII            &    J  & 75.99  & 2    &  &   10.69  & 0.055  & FeII            &   J& 10.67&      2\\
  79.79  & 0.023  & CrII            &   43  & 79.88  & 1    &  &          &        & FeII            &   J& 10.78&      \\
  84.14  & 0.025  & FeII            &    J  & 84.11  & 1    &  &   28.93  & 0.004  & FeII            &   J& 29.06&      1\\
  91.91  & 0.040  & FeII            &    J  & 91.67  & 2    &  &   29.74  & 0.005  & FeII            &   J& 29.92&      1\\
         &        & XeII            &   NI  & 92.22  &      &  &   31.99  & 0.008  & FeII            &   J& 32.09&      1  \\ 
  94.29  & 0.034  & MnII            &    I  & 94.32  & 1    &  &   34.86  & 0.025  & FeII            &   J& 34.83&      1  \\  
  95.52  & 0.064  & MnII            &    I  & 95.40  & 2    &  &   44.66  & 0.019  & FeII            &   J& 44.76&     1\\
  96.60  & 0.025  &                 &       &        & 1    &  &          &        & FeII            &  J& 44.20&      \\
  97.13  & 0.021  & MnII            &    I  & 97.06  & 1    &  &   48.65  & 0.015  & FeII            &   J& 48.21&      1\\
  99.30  & 0.061  & MnII            &    I  & 99.39  & 2    &  &   59.06  & 0.030  & SII             &  61& 59.06&      1 \\
         &        &                 &       &        &      &  &          &        & MnII            &   I& 59.05&\\    
5300.00  &        &                 &       &        &      &  &   61.43  & 0.010  & FeII            &   J& 61.52&       1 \\
  02.50  & 0.053  & FeII            &    J  & 02.55  & 2    &  &   63.46  & 0.010  & FeII            &   J& 63.40&       1 \\  
  06.18  & 0.011  & FeII            &    J  & 06.18  & 1    &  &   67.76  & 0.019  & FeII            &   J& 67.84&      1\\
  13.58  & 0.017  & CrII            &   43  & 13.59  & 1    &  &   70.58  & 0.041  &                 &    &      &       1\\
  16.39  & 0.122  & FeII            &    J  & 16.23  & 5    &  &   78.06  & 0.032  & FeII            &  J & 77.92&       1\\
         &        & FeII            &    J  & 16.62  &      &  &          &        & MnII            &  I & 78.15& \\
         &        & FeII            &    J  & 16.78  &      &  &   88.16  & 0.018  & FeII            &  J & 88.22&      1\\
  25.53  & 0.018  & FeII            &    J  & 25.55  & 1    &  &          &        & FeII            &  J & 88.05&       \\
  29.51  & 0.014  & OI              &   12  & 29.10  & 1    &  &          &        &                 &     &      & \\    
         &        & OI              &   12  & 29.68  &      &  & 5600.00  &        &                 &     &      &\\
  30.72  & 0.031  & OI              &   12  & 30.74  & 1    &  &   06.08  & 0.011  & SII             &  11 &06.15 &     1\\
         &        & NeI             &    9  & 30.78  &      &  &   39.96  & 0.022  & SII             & 14 &39.97  &    1 \\
  34.85  & 0.013  & CrII            &   43  & 34.88  & 1    &  &   45.43  & 0.010  & FeII            &    J& 45.40&      1\\
  36.73  & 0.032  & TiII            &   69  & 36.78  & 1    &  &   46.93  & 0.003  & SII             &  14 &47.03 &     1/2\\
  39.55  & 0.040  & FeII            &    J  & 39.59  & 2    &  &   48.80  & 0.008  & FeII            &    J& 48.90&     1\\
  44.68  & 0.035  & PII             &   NI  & 44.71  & 1    &  &   51.56  & 0.006  & FeII            &    J& 51.54&      1\\
  46.23  & 0.017  &                 &       &        & 1    &  &   55.32  & 0.005  & FeII            &    J& 55.36&       1/2\\
  62.84  & 0.047  & FeII            &    J  & 62.87  & 2    &  &   57.86  & 0.003  & FeII            &    J& 57.92&       1/2\\
  66.25  & 0.014  & FeII            &    J  & 66.21  & 1    &  &   60.18  & 0.014  & FeII            &    J& 60.15  &     1\\
  70.34  & 0.010  & FeII            &    J  & 70.30  & 1    &  &   64.70  & 0.009  & SII             &  11 &64.78    &  1\\
  72.36  & 0.022  & XeII            &   NI  & 72.39  & 1    &  &   68.78  & 0.003  & FeII            &    J& 68.64   &   1/2\\
  75.91  & 0.011  & FeII            &    J  & 75.84  & 1    &  &   69.58  & 0.011  & SiII            & 7.33& 69.56&1\\
  86.95  & 0.066  & FeII            &    J  & 87.06  & 2    &  &   86.92  & 0.013  &                 &     &         & 1    \\
         &        & PII             &   NI  & 86.88  &      &  &   91.38  & 0.011  & FeII            &   47& 91.38   &  1    \\
  93.70  & 0.013  & FeII            &    J  & 93.85  & 1    &  &          &        &                 &      &        & \\
\bottomrule
\end{tabular}
\end{table*}

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


%%%%% PAGINA 5 TABLA 1 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%

\setcounter{table}{0}
\begin{table*}[!t]
\vspace{0.1cm}
\centering
\centerline{TABLE~1 (CONTINUED)\smallskip}
\tablecols{13}
\casitiny
\begin{tabular}{rclrcccrclrcc}
\toprule  
   &  & \multicolumn{4}{c}{Identification}  &   &   &   & \multicolumn{4}{c}{Identification} \\
\cmidrule{3-6}
\cmidrule{10-13}
$\lambda$ [\AA] & $W_\mathrm{eq}$ & Element & Mult. & $\lambda_\mathrm{lab}$ & Intensity &  & $\lambda$ [\AA] & $W_\mathrm{eq}$ & Element & Mult. & $\lambda_\mathrm{lab}$ & Intensity \\
\cmidrule{1-6}
\cmidrule{8-13}
5700.00  &        &                 &       &        &      &  &   79.33  & 0.035  & FeII            &  J & 79.39  & 1 \\ 
  16.51  & 0.007  & FeII            &    J  & 16.58  & 1/2  &  & 6200.00  &        &                 &    &         &\\  
  48.30  & 0.006  & NeI             &   13  & 48.30  & 1    &  &   38.49  & 0.049  & FeII            &  J &38.39    &  2\\
  80.18  & 0.021  & FeII            &    J  & 80.13  & 1    &  &   39.65  & 0.029  & FeII            &  J &39.34    &  1\\
  83.79  & 0.014  & FeII            &    J  & 83.63  & 1    &  &          &        & FeII            &  J &39.90    &  \\ 
         &        &                 &       &        &      &  &   47.42  & 0.053  & FeII            &  J &47.37    &  2\\
5800.00  &        &                 &       &        &      &  &   61.75  & 0.003  & FeII            &  J &61.72    &  1/2 \\
  26.30  & 0.020  & FeII            &    J  & 26.11  & 1    &  &   66.44  & 0.026  & NeI             & 5 &66.50     & 1\\
         &        & FeII            &    J  & 26.51  &      &  &   69.28  & 0.004  & FeII            &  J &69.34    &  1/2 \\
  52.38  & 0.012  & NeI             &    6  & 52.48  & 1    &  &   71.27  & 0.014  & FeII            &  J &71.21    &  1\\
  75.62  & 0.168  & HeI             &   11  & 75.62  & 6    &  &   73.63  & 0.005  & FeII            &  J &73.59    &  1/2\\
         &        & HeI             &   11  & 75.65  &      &  &   82.64  & 0.012  & MnII            &  K &82.52    &  1\\
  78.57  & 0.013  & FeII            &    J  & 78.53  & 1    &  &   94.02  & 0.022  & FeII            &  J &94.14    &  1\\
  79.84  & 0.017  & FeII            &  K09  & 79.79  & 1    &  &          &        &                 &           &  & \\    
  80.80  & 0.013  & FeII            &  K09  & 80.84  & 1    &  & 6300.00  &        &                 &     &      &\\
  81.87  & 0.019  & NeI             &    1  & 81.89  & 1    &  &   05.32  & 0.023  & FeII            &   J & 05.29&    1\\
  82.82  & 0.022  & FeII            &  K09  & 82.78  & 1    &  &   31.97  & 0.011  & FeII            &   J &31.95 &    1\\
  84.99  & 0.034  & FeII            &    J  & 85.02  & 1    &  &   34.42  & 0.026  & NeI             &  1 &34.43  &    1\\
  89.95  & 0.013  & NaI             &    1  & 89.95  & 1    &  &   40.23  & 0.010  & FeII            &   J &40.24 &    1\\
  91.36  & 0.018  & FeII            &    J  & 91.33  & 1    &  &   47.09  & 0.151  & SiII            &   2 &47.09 &    6 \\
  95.38  & 0.012  & FeII            &    J  & 95.35  & 2    &  &   49.55  & 0.009  & FeII            &   J &49.58 &    1/2\\
  97.96  & 0.015  & FeII            &    J  & 98.03  & 1    &  &   57.22  & 0.028  & FeII            &   J &57.16 &     1\\
  98.90  & 0.044  & SiIII           &    K  & 98.79  & 2    &  &   62.54  & 0.004  & FeII            &   J &62.48 &     1/2 \\
         &        &                 &       &        &      &  &   67.34  & 0.009  & FeII            &   J &67.41 &     1/2\\
5900.00  &        &                 &       &        &      &  &   71.36  & 0.132  & SiII            &   2 &71.36 &     5 \\
  01.25  & 0.010  & FeII            &    J  & 01.39  & 2    &  &   83.21  & 0.026  & NeI             &  3 &82.99  & 1 \\     
  02.60  & 0.029  & FeII            &    J  & 02.82  & 1    &  &          &        &                 &       &        & \\   
  11.86  & 0.022  &                 &       &        & 1    &  & 6400.00  &        &                 &     &        &\\
  14.50  & 0.018  & FeII            &    J  & 14.53  & 1    &  &   02.25  & 0.035  & NeI             &   1 &02.24   &  1 \\
  21.39  & 0.025  &                 &       &        & 1    &  &   07.14  & 0.015  & FeII            &    J& 01.25  &  1\\     
  27.18  & 0.016  & SII             &   21  & 27.15  & 1    &  &   11.07  & 0.008  & MnII            &    K& 11.00  &  1/2\\
  44.41  & 0.028  & FeII            &    J  & 44.38  & 1    &  &   15.57  & 0.014  & FeII            &     J & 15.56&  1\\ 
  44.89  & 0.026  & NeI             &    1  & 44.83  & 1    &  &   16.92  & 0.021  & FeII            &     J &16.92 &  1\\
  48.42  & 0.029  & FeII            &    J  & 48.42  & 1    &  &   25.75  & 0.014  & FeII            &     J &25.74 &  1\\
  55.67  & 0.016  & FeII            &    J  & 55.70  & 1    &  &   33.43  & 0.025  &                 &      &       &  1\\
  57.52  & 0.100  & SiII            &    4  & 57.56  & 3    &  &   40.44  & 0.005  & FeII            &    J &40.48  &  1/2\\
  61.62  & 0.029  & FeII            &    J  & 61.71  & 1    &  &   46.52  & 0.008  & FeII            &    J &46.40  &  1/2\\ 
  65.52  & 0.036  & FeII            &    J  & 65.63  & 1    &  &   48.32  & 0.008  & FeII            &    J &48.22  &  1/2\\ 
  75.88  & 0.033  & NeI             &    1  & 75.53  & 1    &  &   52.92  & 0.009  & MnII            &    K &52.88  &  1/2\\
         &        & XeII            &   NI  & 76.46  &      &  &   55.94  & 0.020  & OI              &   9 &56.01   &  1\\
  78.97  & 0.048  & SiII            &    4  & 78.97  & 2    &  &   56.38  & 0.046  & FeII            &    J &56.38  &   2\\
  83.96  & 0.015  & FeII            &    J  & 83.86  & 1    &  &   58.62  & 0.013  & MnII            &    K &58.56  &   1\\   
         &        &                 &       &        &      &  &   59.93  & 0.031  & PII             &    K &59.94   &   1\\
6000.00  &        &                 &       &        &      &  &   62.21  & 0.020  & MnII            &   20 &62.21  &   1\\
  24.16  & 0.064  & PII             &   NI  & 24.18  & 2    &  &   63.20  & 0.017  & MnII            &   20 &63.20  &   1\\
  34.00  & 0.049  & PII             &   NI  & 34.04  & 2    &  &   78.12  & 0.020  & FeII            &    J &78.14  &   1\\
  43.04  & 0.074  & PII             &   NI  & 43.12  & 3    &  &   82.30  & 0.044  & FeII            &   J &82.20   &   2 \\
  45.50  & 0.012  & FeII            &    J  & 45.46  & 1    &  &   91.61  & 0.051  & TiII            &   91 &91.56  &   1\\
  49.49  & 0.007  & FeII            &    J  & 49.45  & 1/2  &  &          &        & FeII            &    J &91.67  &    \\
  60.93  & 0.021  & FeII            &    J  & 60.99  & 1    &  &   93.11  & 0.009  & FeII            &    J &93.03  &   1\\
  69.63  & 0.006  & FeII            &    J  & 69.67  & 1/2  &  &   94.46  & 0.046  & MnII            &    K &94.42  &   2 \\
  71.43  & 0.009  & FeII            &    J  & 71.42  & 1    &  &          &        &                 &       &         & \\   
  74.41  & 0.012  & NeI             &    3  & 74.34  & 1    &  & 6500.00  &        &                 &      &       &\\
  84.19  & 0.006  & FeII            &    J  & 84.11  & 1/2  &  &   03.13  & 0.045  &                 &      &       &  2  \\
  87.76  & 0.030  & PII             &   NI  & 87.82  & 1    &  &   06.40  & 0.025  & NeI             &   3  &06.53  &1\\
  89.76  & 0.004  & CrII            &   87  & 89.69  & 1    &  &   10.76  & 0.028  & FeII            &    J &10.73  &  1\\
  96.29  & 0.017  &                 &       &        & 1    &  &   31.12  & 0.035  & FeII            &    J &31.16  &  1\\ 
         &        &                 &       &        &      &  &   41.27  & 0.018  & FeII            &    J &41.37  &  1\\   
6100.00  &        &                 &       &        &      &  &   42.68  & 0.040  & FeII            &    J &42.63  &  2\\
  05.33  & 0.006  & MnII            &    K  & 05.27  & 1/2  &  &   55.67  & 0.019  & MnII            &   K &55.69  &  1 \\
  22.55  & 0.032  & MnII            &    K  & 22.45  & 1    &  &   62.82  &        & H$\alpha$       &      &       &6\\
  28.91  & 0.023  & MnII            &    K  & 29.04  & 1    &  &   73.54  & 0.037  & FeII            &    J &73.49  &  5\\
  43.01  & 0.021  & NeI             &    1  & 43.06  & 1    &  &   78.03  & 0.033  & CII             &   2 &78.05   &   1 \\   
  47.77  & 0.016  & FeII            &    J  & 47.77  & 1    &  &   82.84  & 0.012  & CII             &   2 &82.85   &    1\\    
  49.19  & 0.018  & FeII            &    J  & 49.25  & 1    &  &   85.32  & 0.016  & MnII            &    K &85.24  &    1\\
  56.57  & 0.040  & OI              &   10  & 56.78  & 1    &  &   98.24  & 0.008  & FeII            &    J &98.31  &    1/2\\ 
         &        & OI              &   10  & 55.99  &      &  &          &        &                 &       &      & \\
  58.18  & 0.031  & OI              &   10  & 58.19  & 1    &  & 6600.00  &        &                 &      &       &\\
  63.53  & 0.013  & FeII            &    J  & 63.60  & 1    &  &   00.81  & 0.009  &                 &      &       &  1\\
  65.56  & 0.031  & PII             &   NI  & 65.59  & 1    &  &   04.30  & 0.006  & FeII            & K09 &04.30  &  1/2\\
  68.32  & 0.013  & MnII            &    K  & 68.35  & 1    &  &   11.32  & 0.005  & FeII            & K09 &11.40  &  1\\
  75.24  & 0.005  & FeII            &    J  & 75.14  &  1/2 &  &   22.04  & 0.014  & FeII            & J &21.98  &   1\\
         &        & FeII            &    J  & 75.44  &      &  &   47.62  & 0.005  & FeII            & J &47.70   &  1/2\\
\bottomrule
\end{tabular}
\end{table*}


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


%%%%% TABLA 2

\setcounter{table}{1}
\begin{table*}[!t]
%\vspace{0.1cm}
\centering
%\caption{Comparison of HD53244 with other Hg-Mn stars}
\centerline{TABLE~2\smallskip}
\centerline{COMPARISON OF HD~53244 WITH OTHER HG-MN STARS\smallskip}
\label{tab:II}
\setlength{\tabnotewidth}{0.8\textwidth}
\tablecols{9}
%\setlength{\tabcolsep}{0.7\tabcolsep}
\scriptsize
\begin{tabular}{lcccccccccccc}
\toprule
Atomic    & HD    & HD     & HD     & HD     & 112  & HR   & HR   & HR   \\ 
Species   & 53244 & 175640 & 186122 & 144206 & HerA & 7361 & 7245 & 7143 \\
\midrule
He I      &Pres &Pres   &Abs   &Pres &Pres &Pres &\nodata&\nodata\\
Be II     &\nodata& Pres  &\nodata& \nodata&\nodata&\nodata&\nodata&\nodata    \\
B II      &\nodata&  Abs  &\nodata&\nodata&\nodata&\nodata&\nodata&\nodata    \\
C I       &Abs &Pres   &Abs   &Pres &Abs  &Abs  &Pres&Pres \\
C II      &Pres &Pres   &Abs   &Pres &Pres &Pres &Pres&Pres \\
N II      &Abs  &Abs    &Abs   &\nodata&\nodata&\nodata&\nodata&\nodata    \\
O I       &Pres &Pres   &Pres  &Pres &Pres &Pres &\nodata&\nodata    \\
O II      &Doub &Pres   &Pres  &Pres &Abs  &Pres &\nodata&\nodata  \\
Ne I      &Pres & Pres  &Pres  &\nodata&\nodata&\nodata&\nodata&\nodata   \\
Na I      &Pres & Pres  &Pres  &\nodata&\nodata&\nodata&\nodata&\nodata    \\
Mg I      &Abs &Pres   &Abs   &Pres &Abs  &Abs  &Doub&Pres  \\
Mg II     &Pres &Pres   &Pres  &Pres &Pres &Pres &Pres&Pres \\
Al I,II   &\nodata&Abs    &Pres  &\nodata&Pres &Abs  &\nodata&\nodata    \\
Si II     &Pres & Pres  &Pres  &Pres &Pres &Pres &Pres&Pres \\
Si III    &Pres & Pres  &Abs   &Pres &Pres &Pres &\nodata&\nodata    \\
P II      &Pres & Pres  &Pres  &Pres &Pres &Pres &Pres&Abs   \\ 
S I       &Abs &Pres   &Abs   &Pres &Pres &\nodata&\nodata&\nodata    \\
S II      &Pres &Pres   &Abs   &Pres &Pres &\nodata&\nodata&\nodata    \\
Ca I      &Abs  &Pres  &\nodata&Pres &Pres  & Pres&\nodata&\nodata   \\
Ca II     &Pres &Pres  &\nodata&Pres &Pres  & Pres&\nodata&\nodata   \\
Sc II     &Pres &Pres  &\nodata&Pres &Pres &Pres &Doub&Abs    \\
Ti II     &Pres & Pres  &Pres  &Pres &Pres &Pres &Pres&Pres \\
Cr I      &Abs  &Pres   &Pres  &Pres &Abs  &Abs  &Abs &Pres     \\
Cr II     &Pres &Pres   &Pres  &Pres &Pres &Pres &Pres&Pres  \\
Mn I      &Abs &Pres   &Pres  &Pres &Abs  &Pres &Pres&Pres   \\
Mn II     &Pres &Pres   &Pres  &Pres &Pres &Pres &Pres&Pres \\
Fe I      &Abs &Pres   & Pres &Pres &Pres &Pres &Pres&Pres   \\
Fe II     &Pres &Pres   & Pres &Pres &Pres &Pres &Pres&Pres   \\
Fe III    &Pres  &\nodata&\nodata&Pres &Pres &Pres &Pres&Pres   \\
Co II     &\nodata&Doub & Pres &\nodata&Abs  &Abs  &\nodata&\nodata    \\
Ni II     &Pres &Pres   & Pres &Pres &Abs  &Pres &\nodata&\nodata     \\ 
Cu I      &Abs& Pres  &\nodata  &\nodata&\nodata&\nodata&\nodata&\nodata    \\
Cu II     &Abs& \nodata& Pres    & \nodata& \nodata& \nodata& \nodata & \nodata       \\
Zn II     &\nodata& Abs   &Pres  & \nodata&\nodata&\nodata&\nodata&\nodata     \\
Ga I,II   &Abs   &Pres  & Pres$^a$ &Pres &Pres &Pres &Pres&Pres   \\
As II     &\nodata     & Doub  &Pres  &\nodata&\nodata&\nodata&\nodata&\nodata     \\
Br II     &\nodata     & Pres  &\nodata&\nodata&\nodata&\nodata&\nodata&\nodata     \\
Sr II     &Abs  & Pres  &\nodata&Pres &Pres &Doub &Pres&Pres \\
Y II      &Pres &Pres  &\nodata&Pres &Doub &Pres &Pres&Pres   \\
Zr II     &Doub &Pres  &\nodata&Pres &Pres  &Abs  &Abs &Abs   \\
Rh II     &\nodata     & Pres  & \nodata&\nodata&\nodata&\nodata&\nodata&\nodata    \\
Pd I,II   & \nodata    & Pres  & \nodata&\nodata&\nodata&\nodata&\nodata&\nodata    \\
Xe II     &Pres &  Pres &Pres  &Abs  & Pres&Pres &\nodata&\nodata   \\
Ba II     &\nodata&Pres  &\nodata&Pres & Abs &Abs  &\nodata&\nodata    \\
Ce II     &\nodata&Pres  &\nodata&\nodata&\nodata&\nodata&\nodata&\nodata    \\
Ce III    &\nodata&Abs   &\nodata&\nodata&\nodata&\nodata&\nodata&\nodata    \\
Pr II     &\nodata  &Abs   & \nodata&\nodata&\nodata& Abs &\nodata&\nodata    \\
Pr III    &\nodata&Doub  &\nodata&\nodata&\nodata& Abs &\nodata&\nodata  \\
Nd III    &\nodata&Pres  &\nodata&\nodata&Abs  &Abs  &Abs &Abs   \\
Yb II,III &\nodata& Pres  &\nodata&\nodata&\nodata&\nodata&\nodata&\nodata   \\
Os II     &\nodata& Doub  &\nodata&\nodata&\nodata&\nodata&\nodata&\nodata    \\
Ir II     &\nodata&  Pres &\nodata&\nodata&\nodata&\nodata&\nodata&\nodata    \\
Pt II     &Abs  & Pres  &\nodata&\nodata&Abs  &Abs  &Abs &Abs  \\
Au II     &Abs  & Pres  &\nodata&\nodata&Abs  &Abs  &Abs &Abs  \\
Hg I      &\nodata&Pres  &Pres  &Pres &Abs  &Abs &\nodata&\nodata    \\
Hg II     &Pres  &Pres  &Pres  &Pres &Pres &Pres&Pres&Pres    \\
\midrule
$T_\mathrm{eff}$ &13.781 & 12.050 & 13.000 & 12.000 & 13.450 & 13.650 & 12.293 & 12.050 \\
$v\sin i$     & 30 & 20 & 20 & 20 & 20 & 15 & 15 & 20 \\
\bottomrule
\noalign{\smallskip}
\tabnotetext{}{Notes: Abs = Absent, Pres = Present, Doub = Doubtful.}
\tabnotetext{a}{\citet{castelli09} did not observe Ga for this star on optical UVES spectra. Smith \& 
Dworetsky (1993) studied the star in the ultraviolet using IUE spectra. Maybe also HD 53244 would show 
Ga in the ultraviolet.}
\end{tabular}
\end{table*}

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


Table~\ref{tab:I} lists the line identifications. The first column shows the mean wavelength $\lambda$ in \AA\ as measured on HD 53244 and 
corrected by Doppler shift to the laboratory frame. The second column lists the equivalent width in \AA\ measured in our spectra. The values 
are averages of two spectra. Column~3 lists the identification of the ion producing the line (the symbol ? means  that the identification is 
doubtful). Column~4 provides the multiplet number or the source of the identification. The rest wavelengths are indicated in Column~5, while 
Column~6 provides the relative intensity of the line. The intensities are a measure of the depth of the line with respect to the continuum 
and they were estimated with a very rough scale in which lines (at the wavelength given) with a depth smaller than 4\% correspond to intensity 
$I=1$, those between 4\% and 6\% correspond to $I=2$; 6\% to 10\%, to $I=3$; 10\% to 15\%, to $I=4$; 15\% to 20\%, to $I=5$; 20\% to 30\%, to 
$I=6$; 30\% to 40\%, to $I=7$; 40\% to 60\%, to $I=8$; 60\% to 80\%, to $I=9$; and 80\% to 100\%, to $I=10$. 

In the vicinity of the Balmer lines, the intensities for the metal lines are measured with respect to the hydrogen line wings.The intensities for 
the Balmer lines are measured with respect to a continuum extrapolated across them. 

Let us comment, next, the results for some atomic species:\\
$\bullet$ \ion{H}{i}. The first line measured from the short wavelewngths region is $\lambda3759$.\\
$\bullet$ \ion{He}{i}. There are several lines identified.\\
$\bullet$ \ion{C}{ii}. \citep{moo} lines of multiplets 4 ($\lambda3918$ and $\lambda3920$) and $\lambda4267$ are present; lines of multiplet 2 
($\lambda6578.05$ and $\lambda6582.88$) were also found among the telluric lines present in the 6500~\AA\ region. \\
$\bullet$ \ion{N}{i} is not present.\\
$\bullet$ \ion{O}{i}. We identified three lines of \ion{O}{i} in the $\lambda5300$ region. They belong to multiplets 12 and 13 and one line of multiplet 3. 
We have also identified lines of multiplet 10 ($\lambda6155.99$ blended with $\lambda6156.78$) and also we found $\lambda6158.19$. We have also found 
the line of multiplet 9 $\lambda6456.01$. So the presence of \ion{O}{i} is certain.\\
$\bullet$ \ion{O}{ii}. The identification is very doubtful, only one line  is probably present.\\
$\bullet$ \ion{Ne}{i}. There are several lines identified, multiplets 1, 3, 5, 6, 9, 11 and 13.\\
$\bullet$ \ion{Na}{i}. There are many telluric lines present in the region, only $\lambda5889$ was identified. \\
$\bullet$ \ion{Mg}{i} is not present.\\
$\bullet$ \ion{Mg}{ii}. We have identified lines of multiplets 4, 5, 9 and 10.\\
$\bullet$ \ion{Si}{ii}. Several lines were identified from multiplets. 1, 3, 4, 5, 7.03, 7.05, 7.33.\\
$\bullet$ \ion{Si}{iii}. Lines of Multiplet 1 are present.\\
$\bullet$ \ion{P}{ii}. Several lines were identified. We have used NIST tables.\\
$\bullet$ \ion{S}{i} is not present.\\
$\bullet$ \ion{S}{ii}. A lot of lines were identified using Moore's tables \citep{moo}.\\
$\bullet$ \ion{Ca}{i} is not present.\\
$\bullet$ \ion{Ca}{ii} $\lambda3933$ and $\lambda3968$ are present.\\
$\bullet$ \ion{Sc}{ii}. The most intense lines are identified using Moore Tables \citep{moo}; $\lambda4246$ blended with \ion{Cr}{ii}, $\lambda4320.74$ 
and $\lambda4374.46$ blended with \ion{Ti}{ii}.\\
$\bullet$ \ion{Ti}{ii}. We have identified a lot of lines. Very probably this element is overabundant.\\
$\bullet$ \ion{Cr}{ii}. A lot of lines were identified using Moore's tables. There are no lines of \ion{Cr}{i}.\\
$\bullet$ \ion{Mn}{ii}. Using the tables from \citet{igle} we have identified a lot of lines. Mn is very well represented. \\
$\bullet$ \ion{Fe}{i}. There are no lines. Probably the effective temperature ($T_\mathrm{eff}=13781$~K) is too high.\\
$\bullet$ \ion{Fe}{ii}. A lot of lines are present. We have used Moore's tables. For $\lambda > 4800$~\AA\ we have used \citet{1978Phys. Scripta...18...217} 
and the more recent table by \citet{1994ApJS...94...221}.\\
$\bullet$ \ion{Fe}{iii}. We have identified lines of multiplet 4.\\
$\bullet$ \ion{Ni}{ii}. We have identified only two lines, $\lambda4015.50$ and $\lambda4067.05$.\\
$\bullet$ \ion{Cu}{ii} is not present.\\
$\bullet$ \ion{Y}{ii}. We identified $\lambda3950.3$5 (multiplet 6), $\lambda4235.73$, $\lambda4309.62$ (multiplet 5) and $\lambda4374.94$ (multiplet 13).\\
$\bullet$ \ion{Zr}{ii}. The most intense line $\lambda4149$ is ambiguously present although other weaker lines are identified $\lambda3843.03$ (multiplet 7), 
$\lambda3991.14$ (multiplet 30), $\lambda4018.38$, $\lambda4040.24$ (multiplet 54) and $\lambda4034.10$ (multiplet 42); we think that the presence 
of this element is doubtful.\\
$\bullet$ \ion{Xe}{ii}. The most intense lines are identified using the NIST tables.\\
$\bullet$ \ion{Hg}{ii}. The line $\lambda3983$ is definitely present.\\


We have not identified lines of \ion{Ga}{ii} and \ion{Sr}{ii}. We have not identified rare earths nor Au and Pt. The red regions of the spectra of 
HD 53244 have many telluric lines and it was difficult to identify with certainty some lines.

Thus, \ion{H}{i}, \ion{He}{i}, \ion{C}{ii}, \ion{O}{i}, \ion{Ne}{i}, \ion{Na}{i}, \ion{Mg}{ii}, \ion{Si}{ii}, \ion{P}{ii}, \ion{S}{ii}, \ion{Ca}{ii}, 
\ion{Sc}{ii}, \ion{Ti}{ii}, \ion{Cr}{ii}, \ion{Mn}{ii}, \ion{Fe}{ii}, \ion{Fe}{iii}, \ion{Ni}{ii}, \ion{Y}{ii}, \ion{Xe}{ii}, \ion{Hg}{ii} are definitely 
present. \ion{O}{ii} and \ion{Zr}{ii} are doubtful. There are a number of unidentified lines. These are likely to be lines of atomic species which have 
been already identified.

\vspace{0.3cm}

\section{Comparison With Other Field Bp-Ap Stars and Comments}
\label{sec:comp}

Line identification lists have been published for several other HgMn stars. In Table~2 we have indicated the atomic species present 
in the blue, visual and red regions of HD 53244 The spectrum in the photographic region of HD 53244 is compared in the table with those of other 
Hg-Mn stars: HD 144206 (Adelman, Gulliver, \& Rayle 2001), HD 186122 \citep{2001PASJ...53...1223}, HD 175640 \citep{2004A&A...425...263}, and 
112HerA, HR 7361, HR 7245 and HR 7143  \citep{1985MNRAS...216..1}.

Effective temperatures were  obtained from \citet{smith93} for HD 144206, HD 186122, 112 HerA and HR 7361; \citet{heacox79} for HR 7245; 
\citet{cenarro07} for HD 175640 and HR 7143. For HD 53244 we used $uvby-\beta$ mean colors from \citet{hauck98} and the TEMPLOGG program 
\citet{rogers95} to obtain this parameter. The $v \sin i$ were taken from \citet{abt02}.

As is usually the case, Hg-Mn stars seem to differ one from another. The Hg-Mn phenomenon seems to be heterogeneous with star to star diversity. 
Probably the absence of Ga I, II and Sr II is the distintive feature in HD 53244. It does not appear to be identical to any of the other stars 
in Table~2 although it shares many of their anomalies. Many of the atomic species which are present are represented by only a few lines. 
Differences in the magnetic field strength and configuration, apparent rotational velocity, effective temperature, surface gravity, elemental 
distributions on the stellar surface (see the recent paper by Briquet et al. 2010), and the exact wavelength region studied may well hide some 
of the underlying similarities. 

There is no evidence in the spectra of HD 53244 of doubly ionized rare-earth lines. This lack of identifications may be due to the choice of the 
region studied  (Adelman 1974).

The major similarity occur between HD 53244 and HD144206, which share almost the same anomalies except for the absence of Ga in  the former. We conclude 
that HD 53244 appears to be a Hg-Mn star without Ga or rare earth elements.

\vspace{0.3cm}

\acknowledgements

The present work was partially supported through a grant from Consejo Nacional de Investigaciones Cient\'ificas y T\'ecnicas de la Rep\'ublica Argentina 
(CONICET PIP 1113). The authors thank the help provided by CASLEO personnel during the observing runs and an anonymous referee for helping to 
improve the presentation of this paper.

\vspace{0.23cm}

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