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%% Sample TeX file for the HRMS Dijon 2023 abstracts
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\documentclass[11pt]{article}

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

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\title{CAVITY RINGDOWN SPECTROSCOPY OF DISSOCIATED NAPHTHALENE IN A RADIOFREQUENCY PLASMA JET}

%% Note that \author and \address macros must be paired.
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\author{\FirstName J. \LastName LECOMTE,
	\FirstName N. \LastName SUAS-DAVID, 
	\FirstName E. \LastName DUD\'AS,
	\FirstName S. \LastName PEROT,
	\FirstName L. \LastName RUTKOWSKI,
	\underline{\FirstName R. \LastName GEORGES}}
\address{IPR, Universit\'e de Rennes, UMR6251 CNRS, F-35042, France}

\author{\FirstName C. \LastName CHARLES,
	\FirstName R. W. \LastName BOSWELL}
\address{Research School of Physics, Australian National University, Canberra, ACT, Australia}

\author{\FirstName S. \LastName KASSI}
\address{LIPhy, UMR 5588, Universit\'e Grenoble Alpes, Saint Martin d'H\`eres, France}

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

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\usepackage{fancyhdr}
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\fancyhead[C]{{\footnotesize \textit{HRMS, 28th Colloquium, Dijon, France,
  Aug. 28 - Sept. 1, 2023}}}
\fancyfoot[C]{}
\renewcommand{\headrulewidth}{0.6pt}
\renewcommand{\footrulewidth}{0.6pt}

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\usepackage[colorlinks=true,urlcolor=blue,linkcolor=blue,citecolor=blue]{hyperref}
\voffset -.65 cm

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\category {8,5}
\begin{document}

\maketitle  %% This will also build the list of author(s) and addresse(s).
%% Index macro(s): see the abstract samples and the instructions
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Polycyclic aromatic hydrocarbons (PAHs) are abundant organic molecules detected in several objects in the universe, such as molecular clouds in the interstellar medium (ISM)\footnote{\href{https://doi.org/10.1086/184435}{doi:10.1086/184435}, L. J. Allamandola \textit{et al.}, The Astrophysical Journal, 290, L25-L28 (1985).}. Their structure can be modified through plasma-driven processes occurring in the ISM. The present study focuses on the dissociation of naphthalene (C$_{10}$H$_{8}$) in a radiofrequency (RF) plasma, probed using cavity ringdown spectroscopy (CRDS) in the near-infrared. Namely, the low-power RF plasma source, called Platypus, is adapted from a small plasma thruster (Pocket Rocket\footnote{\href{https://doi.org/10.1088/0963-0252/21/2/022002}{doi:10.1088/0963-0252/21/2/022002}, C. Charles and R. W. Boswell, Plasma Sources Science and Technology, 21.2, 022002 (2012).}) designed by the Space Plasma Power and Propulsion laboratory of the ANU. A stable supersonic jet plasma is generated by expanding a mixture of argon and C$_{10}$H$_{8}$ into a vacuum chamber through a 20 mm long, 4 mm wide slit nozzle\footnote{\href{https://theses.hal.science/tel-03341145/}{theses.hal.science/tel-03341145}, E. Dud\'as, Ph.D Thesis, 149-162 (2021).}. The jet-cooled fragmented C$_{10}$H$_{8}$ is finally probed with the ultra-sensitive CRDS technique. We recorded a spectrum from 5950 to 6120 cm$^{-1}$ composed of several hundred transitions originating from many different molecules, radicals, and probably ions\footnote{\href{https://doi.org/10.1021/acs.jpca.9b00100}{doi:10.1021/acs.jpca.9b00100}, M. Alliati \textit{et al.}, The Journal of Physical Chemistry, A 123.10, 2107-2113 (2019).}.


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