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\newcommand{\utn}{Universit\`{a} degli Studi di Trento}

\name{Daniele Nicolodi}
\address{%
  SYRTE - Observatoire de Paris \\
  61 Avenue de l'Observatoire \\
  75014, Paris, France}
\info{% 
  Phone:   & 00 33 140 512074 \\ 
           & 00 33 674 792943 \\
  Email:   & \mailto{daniele.nicolodi@obspm.fr}}
 
\bibliography{publications}

\begin{document}
\maketitle
 
\section{Education}
\begin{description}
\item[2011 \enspace Ph.D. in Physics] \utn, Trento, Italy. Degree
  obtained with grade Excellent -- highest honours. Dissertation:
  <<Femto Newton level testing of free fall on ground>>. Supervisor:
  William Joseph Weber.
\item[2007 \enspace Master Degree in Physics] Laurea Magistrale, \utn,
  Trento, Italy. Degree obtained with grade 110/110 cum laude -- highest
  honours. Thesis: <<Toward a third generation torsion pendulum for
  the femto-Newton level testing of free fall in the laboratory>>.
\item[2004 \enspace Bachelor Degree in Applied Physics] Laurea, \utn, Trento,
  Italy. Degree obtained with grade 110/110. Thesis:
  <<Calibration system for the scintillators employed in the CRESST-II
  dark matter research experiment>>.
\end{description}

\section{Relevant work experiences}
\begin{description}
\item[2nd May 2012 - present] Post-doc fellow. Optical Frequency
  Group, SYRTE - Observatoire de Paris, Paris, France. Optical
  frequency comb activity for the low phase-noise microwave generation
  with photonic technique and low phase noise comparison of
  ultra-stable laser oscillators.
\item[1st April 2011 - 30th April 2012] Post-doc fellow. Experimental
  Gravitation Laboratory, University of Trento, Trento, Italy.
  Torsion balance experiment for the measurement of small forces in
  the context of the validation of the gravitational reference sensor
  for the LISA gravitational wave detector.
\item[1st November 2007 - 31st March 2012] PhD fellow. Experimental
  Gravitation Laboratory, University of Trento, Trento, Italy. Torsion
  balance experiment for the measurement of small forces in the
  context of the validation of the gravitational reference sensor for
  the LISA gravitational wave detector.
\item[1st February 2010 - 31st October 2011] Assistant Lecturer for the course
  <<Fisica 1>> -- Newtonian physics for 1st year students -- at the
  Faculty of Engineering, University of Trento, Trento, Italy.
\item[1st February 2009 - 31st October 2009] Assistant Lecturer for the course
  <<Laboratorio di Fisica 1>> -- introductory physics laboratory for
  1st year Physics students -- at the Faculty of Science, University
  of Trento, Trento, Italy.
%\item[1999 - 2007] Freelance in the Information Technology field with
%  particular, but not limited to, experience in the design,
%  development and integration of custom GNU-Linux solutions, design
%  and development of desktop and web-based applications, network
%  protocol analysis and implementation.
\end{description}

%% \section{Current research activity and interests}
%% \begin{dottedlist} 
%%   High precision frequency metrology \and Ultra-stable lasers \and
%%   Optical frequency combs \and Low-noise photonic microwave generation
%%   \and Optical clocks
%% \end{dottedlist}

%% \noindent
%% My current research activity focuses on the exploitation fiber-based
%% optical frequency combs systems for the transfer of frequency
%% stability from ultra-stable lasers to different wavelengths in the
%% optical domain or to the microwave domain.  In the optical domain, my
%% work aims at improving the state-of-the-art optical frequency
%% stability transfer solutions to make them suitable for transferring
%% frequency stability exceeding the thermal noise limit of high-finesse
%% optical cavities.  In the microwave domain, my work aims at developing
%% solutions for microwaves generation with short-term frequency
%% stability beyond the one of state-of-the-art cryogenic
%% oscillators. Those research topic have direct application to the
%% operation and development of atomic and optical frequency clocks at
%% SYRTE.

%% \section{Previous relevant research activity}
%% \begin{dottedlist} 
%%   High precision force metrology \and High sensitivity torsion
%%   pendulums \and Sources of force noise on geodesic reference
%%   macroscopic test masses \and Dissipation mechanisms in mechanical
%%   experiments \and Optical interferometry
%% \end{dottedlist}

%% \noindent
%% My previous research activity focused on the study of the limits for
%% achieving near perfect free-fall of macroscopic test masses for the
%% observation of gravitational waves. In particular, I contributed to
%% the on-ground measurement of small force disturbances on the test
%% masses of the Laser Interferometer Space Antenna space low-frequency
%% gravitational wave detector -- LISA -- and its precoursor mission LISA
%% Pathfinder, exploiting the femto-Newton level sensitivity of a torsion
%% pendulum. My work work included the experimental activity, the
%% development of data analysis routines for the extraction of stochastic
%% and coherent small force signals, and, concurrently it also aimed at
%% improving the sensitivity of the torsion pendulum apparatus itself,
%% pushing the current limits for small force metrology.  I lead the
%% initial effort for the realization of a low-noise torsion pendulum
%% angular position read-out based on an heterodyne wavefront-sensing
%% interferometer with nanoradian sensitivity, applying some of the LISA
%% Pathfinder interferometer techniques. I collaborated to the
%% development of the LTPDA Matlab Toolbox for the LISA Pathfinder data
%% analysis, with particular attention to the relational database data
%% storage component.

%% \section{Skills and competences}

%% I have experience in designing and analyzing experiments and
%% measurement techniques, with the particular attention to detail and
%% sources of uncertainty required in high precision measurements. I have
%% experience with the design, setup and operation of precise mechanical
%% apparatuses, low noise electronics, high precision optical systems,
%% data acquisition hardware and software, computer controlled
%% experiments, and high vacuum systems, as well as with the development
%% of data analysis methods and numerical simulations. More recently I
%% acquired competences in the operation of fiber-based optical frequency
%% combs, ultra-stable laser stabilised on high-finesse optical cavities,
%% frequency and phase noise characterisation, and radio-frequency
%% electronics.

%% I'm fluent programming in C, C\texttt{++}, Python, Perl, Matlab, and
%% LabView, with specific experience in scientific computing and data
%% analysis.  I have experience in real-time data acquisition and
%% processing, and I have knowledge of the basic techniques for real-time
%% programming.  I master and routinely take advantage of version control
%% systems.  I'm passionate about Free Software and I contribute to
%% several Free Software projects.  I have experience in system
%% administration of GNU-Linux systems and I'm comfortable working in
%% Unix and Microsoft Windows computing environments. I have good
%% knowledge of the LaTeX typesetting system.

%% \section{Other relevant experiences}
%% \begin{description}
%% \item[October 4th - 8th 2010]
%%   Advanced Scientific Programming in Python Autumn School, Trento, Italy.
%% \item[May 5th - 9th 2008]
%%   3rd VESF School on Gravitational Waves Summer School, Virgo, Cascina, Italy.
%% \item[August 2005 - July 2006]
%%   Erasmus student at the Lunds Universitet, Lund, Sweden.
%% \item[April 2005 - June 2005]
%%   Visiting student at the Physics department of the
%%   T\"{u}binghen Universit\"{a}t, T\"{u}binghen, Germany.
%% \end{description}

%\section{Languages}
%\begin{description}[style=sameline]
%\item[Italian:]
%  mother tongue.
%\item[English:]
%  good spoken and written.
%\end{description}

% publications
%\printbibliography[heading=bibnumbered,title=Publications]

%% \section{Conference contributions}

%% \newcommand{\litem}[1]{\item{\it #1.}} 
%% \begin{enumerate}
%% \litem{Brownian force noise from residual gas damping and the
%%   sensitivity of advanced gravitational wave observatories} Talk.
%%   9th Amaldi Conference on Gravitational Waves, Cardiff, Wales, UK,
%%   July 10-15, \textbf{2011}.

%% \litem{Femto-Newton level testing of free-fall on-ground} Solicited
%%   talk. 38th COSPAR Scientific Assembly, Bremen, Germany, July 18-25,
%%   \textbf{2010}.

%% \litem{Experimental investigation of GRS force disturbance sources}
%%   Talk.  8th LISA Symposium, Stanford University, California USA, June
%%   28 - July 2, \textbf{2010}.

%% \litem{Improving torsion pendulum force sensitivity with LISA
%%   Pathfinder like interferometric angular read-out} Poster. 8th LISA
%%   Symposium, Stanford University, California USA, June 28 - July 02,
%%   \textbf{2010}.

%% \litem{Increased Brownian force noise from molecular impacts in a
%%   constrained volume} Talk.  From Quantum to Cosmos 4 - Q2C4, Bremen,
%%   Germany, September 21-24, \textbf{2009}.

%% \litem{Gas damping in the LISA noise budget} Poster. 8th Edoardo
%%   Amaldi Conference on Gravitational Waves, New York, USA, June 21-26,
%%   \textbf{2009}.

%% \litem{An improved torsion pendulum for on-ground verification of the
%%   LISA gravitational reference sensor} Poster. 7th LISA Symposium,
%%   Barcelona, June 16-20, \textbf{2008}.

%% \litem{Characterization of the LISA gravitational reference sensor with
%%   an upgraded torsion pendulum} Poster. 7th Edoardo Amaldi Conference
%%   on Gravitational Waves, Sydney, Australia, July 8-14, \textbf{2007}.
%% \end{enumerate}

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\centering\footnotesize Last updated: \today.

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