%%
%% Sample TeX file for the HRMS Dijon 2023 abstracts
%% 
%% Lines (or parts of) beginning with at least one '%' are comments 
%% and are silently ignored by LaTeX
%%
%% Codings beginning with \ are LaTeX macros, or commands.
%% They are used to tell the LaTeX parser how to format the document.
%% All the macros below are mandatory.
%%
%% Various informations about latex may be found at
%%
%%   http://en.wikibooks.org/wiki/LaTeX
%%
%% *-----------------------------------------------------------------------------------------*
\documentclass[11pt]{article}

\usepackage{hrms}  %% Page settings, style ... for the HRMS abstract book.

%% *-----------------------------------------------------------------------------------------*

\title{LINE-SHAPE PARAMETERS AND THEIR TEMPERATURE DEPENDENCIES FOR THE AIR-BROADENED OXYGEN B-BAND LINES}

%% Note that \author and \address macros must be paired.
%% The names of authors must also appear IN CAPITALS.
%% The name(s) of author(s) presenting the work is(are) usually underlined.

\author{\underline{\FirstName K. \LastName BIELSKA},
  \FirstName D.~D. \LastName TRAN, \FirstName A.~A. \LastName BALASHOV, \FirstName J. \LastName DOMYS{\L}AWSKA, \FirstName S. \LastName W\'{O}JTEWICZ, \FirstName M. \LastName BOBER, \FirstName S. \LastName BILICKI, \FirstName R. \LastName CIURY{\L}O, \FirstName D. \LastName LISAK}
\address{Institute of Physics, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toru\'n, Grudziadzka 5, 87-100 Torun, Poland}

%% The \FirstName and \LastName macros are mandatory for each author
%% to make sure that the author index is properly auto-generated.
%% Otherwise, these macros do nothing in particular.

%% Add or remove \author and \address pair(s) below to suite your needs


%% *-----------------------------------------------------------------------------------------*

%% Place below other \usepackage{ ... }, if you need other packages.
%% See http://www.tug.org/texlive/doc.html for a description of available packages.

%% The macros below will change the page head and foot.
%% Please, do not modify the content of the \fancyhead macro nor the \fancyfoot line.
\usepackage{fancyhdr}
\pagestyle{fancy}
\fancyhead[C]{{\footnotesize \textit{HRMS, 28th Colloquium, Dijon, France,
  Aug. 28 - Sept. 1, 2023}}}
\fancyfoot[C]{}
\renewcommand{\headrulewidth}{0.6pt}
\renewcommand{\footrulewidth}{0.6pt}

%% The hyperref package allows to include hyperlinks in a document.
%% See the instructions for abstract submission for more details.
%% WARNING: Make sure that this package comes LAST since it re-defines many LaTeX macros.
\usepackage[colorlinks=true,urlcolor=blue,linkcolor=blue,citecolor=blue]{hyperref}
\voffset -.65 cm

%% *-----------------------------------------------------------------------------------------*

\category {9,2}
\begin{document}

\maketitle  %% This will also build the list of author(s) and addresse(s).

The B band $\left(b^1\Sigma^+_g\left(v=1\right)\leftarrow X^3\Sigma^-_g\left(v=0\right)\right)$ is the second most intense atmospheric band of molecular oxygen located in the spectral range near 690~nm. 
Considering its growing importance for the remote sensing and the need for reliable spectroscopic reference data,  we present the first complete set of the line-shape parameters and their pressure and temperature dependencies, going beyond the Voigt profile, for the air-broadened oxygen B-band transitions measured under controlled laboratory conditions.
The measurements were performed with the frequency-stabilized cavity ring-down spectroscopy (FS-CRDS) technique. The spectrometer\footnote{\href{http://dx.doi.org/10.1016/j.jqsrt.2021.107927}{doi:10.1016/j.jqsrt.2021.107927}, K. Bielska {\it et al.}, Simultaneous observation of speed dependence and Dicke narrowing for self-perturbed P-branch lines of O$_2$ B band, J. Quant. Spectrosc. Radiat. T. 276, 107927 (2021).} was linked to the optical frequency comb (OFC), which provided the absolute frequency axis. The line-shape analysis was done with the speed-dependent Nelkin-Ghatak profile (SDNGP)\footnote{\href{http://dx.doi.org/10.1006/jmsp.1997.7385}{doi:10.1006/jmsp.1997.7385}, B. Lance {\it et al.}, On the speed-dependent hard collision lineshape models: application to C$_2$H$_2$ perturbed by Xe, J. Mol. Spectrosc. 185, 262-271 (1997).}, which is a limiting case of the recommended Hartmann-Tran profile (HTP)\footnote{\href{http://dx.doi.org/10.1016/j.jqsrt.2013.05.034}{doi:10.1016/j.jqsrt.2013.05.034}, N.H. Ngo {\it et al.}, An isolated line-shape model to go beyond the Voigt profile in spectroscopic databases and radiative transfer codes, J. Quant. Spectrosc. Radiat. T. 129, 89-100 (2013).}. This approach enabled us to account for the line narrowing mechanisms as well as for the line asymmetry. 

We determined the temperature dependence of the collisional broadening and the collisional shift. However, we did not observe a significant temperature dependence of the speed-dependent parameters and the Dicke narrowing. The pressure broadening as well as its temperature dependence are very close to oxygen A band corresponding values\footnote{\href{http://dx.doi.org/10.1016/j.jqsrt.2020.107217}{doi:10.1016/j.jqsrt.2020.107217}, V.H. Payne {\it et al.}, Absorption coefficient (ABSCO) tables for the orbiting carbon observatories:
Version 5.1, J. Quant. Spectrosc. Radiat. T. 255,
107217 (2020).}, whereas the pressure shift for the B band is up to 100\% larger. 
We demonstrated that the temperature dependence of the collisional broadening can be estimated based on its speed dependence.

\end{document}
