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Shorter version for CNRS application
author Daniele Nicolodi <daniele.nicolodi@obspm.fr>
date Mon, 03 Mar 2014 18:01:03 +0100
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1 \documentclass[a4paper,11pt]{article}
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2 \usepackage[T1]{fontenc}
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3 \usepackage{cv}
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5 \newcommand{\utn}{Universit\`{a} degli Studi di Trento}
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7 \name{Daniele Nicolodi}
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8 \address{%
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9 SYRTE - Observatoire de Paris \\
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10 61 Avenue de l'Observatoire \\
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11 75014, Paris, France}
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12 \info{%
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13 Phone: & 00 33 140 512074 \\
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14 & 00 33 674 792943 \\
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15 Email: & \mailto{daniele.nicolodi@obspm.fr}}
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17 \bibliography{publications}
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19 \begin{document}
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20 \maketitle
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22 \section{Education}
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23 \begin{description}
Daniele Nicolodi <daniele@grinta.net>
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24 \item[2011 \enspace Ph.D. in Physics] \utn, Trento, Italy. Degree
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25 obtained with grade Excellent -- highest honours. Dissertation:
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26 <<Femto Newton level testing of free fall on ground>>. Supervisor:
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27 William Joseph Weber.
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28 \item[2007 \enspace Master Degree in Physics] Laurea Magistrale, \utn,
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29 Trento, Italy. Degree obtained with grade 110/110 cum laude -- highest
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30 honours. Thesis: <<Toward a third generation torsion pendulum for
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31 the femto-Newton level testing of free fall in the laboratory>>.
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32 \item[2004 \enspace Bachelor Degree in Applied Physics] Laurea, \utn, Trento,
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33 Italy. Degree obtained with grade 110/110. Thesis:
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34 <<Calibration system for the scintillators employed in the CRESST-II
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35 dark matter research experiment>>.
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36 \end{description}
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37
Daniele Nicolodi <daniele@grinta.net>
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38 \section{Relevant work experiences}
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39 \begin{description}
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40 \item[2nd May 2012 - present] Post-doc fellow. Optical Frequency
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41 Group, SYRTE - Observatoire de Paris, Paris, France. Optical
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42 frequency comb activity for the low phase-noise microwave generation
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43 with photonic technique and low phase noise comparison of
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44 ultra-stable laser oscillators.
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45 \item[1st April 2011 - 30th April 2012] Post-doc fellow. Experimental
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46 Gravitation Laboratory, University of Trento, Trento, Italy.
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47 Torsion balance experiment for the measurement of small forces in
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48 the context of the validation of the gravitational reference sensor
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49 for the LISA gravitational wave detector.
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50 \item[1st November 2007 - 31st March 2012] PhD fellow. Experimental
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51 Gravitation Laboratory, University of Trento, Trento, Italy. Torsion
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52 balance experiment for the measurement of small forces in the
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53 context of the validation of the gravitational reference sensor for
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54 the LISA gravitational wave detector.
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55 \item[1st February 2010 - 31st October 2011] Assistant Lecturer for the course
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56 <<Fisica 1>> -- Newtonian physics for 1st year students -- at the
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57 Faculty of Engineering, University of Trento, Trento, Italy.
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58 \item[1st February 2009 - 31st October 2009] Assistant Lecturer for the course
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59 <<Laboratorio di Fisica 1>> -- introductory physics laboratory for
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60 1st year Physics students -- at the Faculty of Science, University
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61 of Trento, Trento, Italy.
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62 %\item[1999 - 2007] Freelance in the Information Technology field with
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63 % particular, but not limited to, experience in the design,
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64 % development and integration of custom GNU-Linux solutions, design
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65 % and development of desktop and web-based applications, network
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66 % protocol analysis and implementation.
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67 \end{description}
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68
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69 %% \section{Current research activity and interests}
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70 %% \begin{dottedlist}
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71 %% High precision frequency metrology \and Ultra-stable lasers \and
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72 %% Optical frequency combs \and Low-noise photonic microwave generation
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73 %% \and Optical clocks
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74 %% \end{dottedlist}
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75
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76 %% \noindent
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77 %% My current research activity focuses on the exploitation fiber-based
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78 %% optical frequency combs systems for the transfer of frequency
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79 %% stability from ultra-stable lasers to different wavelengths in the
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80 %% optical domain or to the microwave domain. In the optical domain, my
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81 %% work aims at improving the state-of-the-art optical frequency
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82 %% stability transfer solutions to make them suitable for transferring
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83 %% frequency stability exceeding the thermal noise limit of high-finesse
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84 %% optical cavities. In the microwave domain, my work aims at developing
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85 %% solutions for microwaves generation with short-term frequency
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86 %% stability beyond the one of state-of-the-art cryogenic
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87 %% oscillators. Those research topic have direct application to the
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88 %% operation and development of atomic and optical frequency clocks at
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89 %% SYRTE.
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91 %% \section{Previous relevant research activity}
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92 %% \begin{dottedlist}
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93 %% High precision force metrology \and High sensitivity torsion
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94 %% pendulums \and Sources of force noise on geodesic reference
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95 %% macroscopic test masses \and Dissipation mechanisms in mechanical
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96 %% experiments \and Optical interferometry
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97 %% \end{dottedlist}
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99 %% \noindent
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100 %% My previous research activity focused on the study of the limits for
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101 %% achieving near perfect free-fall of macroscopic test masses for the
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102 %% observation of gravitational waves. In particular, I contributed to
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103 %% the on-ground measurement of small force disturbances on the test
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104 %% masses of the Laser Interferometer Space Antenna space low-frequency
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105 %% gravitational wave detector -- LISA -- and its precoursor mission LISA
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106 %% Pathfinder, exploiting the femto-Newton level sensitivity of a torsion
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107 %% pendulum. My work work included the experimental activity, the
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108 %% development of data analysis routines for the extraction of stochastic
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109 %% and coherent small force signals, and, concurrently it also aimed at
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110 %% improving the sensitivity of the torsion pendulum apparatus itself,
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111 %% pushing the current limits for small force metrology. I lead the
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112 %% initial effort for the realization of a low-noise torsion pendulum
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113 %% angular position read-out based on an heterodyne wavefront-sensing
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114 %% interferometer with nanoradian sensitivity, applying some of the LISA
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115 %% Pathfinder interferometer techniques. I collaborated to the
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116 %% development of the LTPDA Matlab Toolbox for the LISA Pathfinder data
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117 %% analysis, with particular attention to the relational database data
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118 %% storage component.
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120 %% \section{Skills and competences}
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122 %% I have experience in designing and analyzing experiments and
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123 %% measurement techniques, with the particular attention to detail and
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124 %% sources of uncertainty required in high precision measurements. I have
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125 %% experience with the design, setup and operation of precise mechanical
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126 %% apparatuses, low noise electronics, high precision optical systems,
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127 %% data acquisition hardware and software, computer controlled
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128 %% experiments, and high vacuum systems, as well as with the development
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129 %% of data analysis methods and numerical simulations. More recently I
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130 %% acquired competences in the operation of fiber-based optical frequency
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131 %% combs, ultra-stable laser stabilised on high-finesse optical cavities,
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132 %% frequency and phase noise characterisation, and radio-frequency
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133 %% electronics.
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135 %% I'm fluent programming in C, C\texttt{++}, Python, Perl, Matlab, and
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136 %% LabView, with specific experience in scientific computing and data
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137 %% analysis. I have experience in real-time data acquisition and
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138 %% processing, and I have knowledge of the basic techniques for real-time
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139 %% programming. I master and routinely take advantage of version control
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140 %% systems. I'm passionate about Free Software and I contribute to
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141 %% several Free Software projects. I have experience in system
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142 %% administration of GNU-Linux systems and I'm comfortable working in
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143 %% Unix and Microsoft Windows computing environments. I have good
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144 %% knowledge of the LaTeX typesetting system.
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146 %% \section{Other relevant experiences}
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147 %% \begin{description}
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148 %% \item[October 4th - 8th 2010]
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149 %% Advanced Scientific Programming in Python Autumn School, Trento, Italy.
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150 %% \item[May 5th - 9th 2008]
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151 %% 3rd VESF School on Gravitational Waves Summer School, Virgo, Cascina, Italy.
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152 %% \item[August 2005 - July 2006]
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153 %% Erasmus student at the Lunds Universitet, Lund, Sweden.
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154 %% \item[April 2005 - June 2005]
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155 %% Visiting student at the Physics department of the
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156 %% T\"{u}binghen Universit\"{a}t, T\"{u}binghen, Germany.
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157 %% \end{description}
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158
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159 %\section{Languages}
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160 %\begin{description}[style=sameline]
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161 %\item[Italian:]
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162 % mother tongue.
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163 %\item[English:]
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164 % good spoken and written.
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165 %\end{description}
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166
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167 % publications
4
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168 %\printbibliography[heading=bibnumbered,title=Publications]
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169
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170 %% \section{Conference contributions}
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171
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172 %% \newcommand{\litem}[1]{\item{\it #1.}}
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173 %% \begin{enumerate}
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174 %% \litem{Brownian force noise from residual gas damping and the
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175 %% sensitivity of advanced gravitational wave observatories} Talk.
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176 %% 9th Amaldi Conference on Gravitational Waves, Cardiff, Wales, UK,
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177 %% July 10-15, \textbf{2011}.
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178
4
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179 %% \litem{Femto-Newton level testing of free-fall on-ground} Solicited
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180 %% talk. 38th COSPAR Scientific Assembly, Bremen, Germany, July 18-25,
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181 %% \textbf{2010}.
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182
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183 %% \litem{Experimental investigation of GRS force disturbance sources}
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184 %% Talk. 8th LISA Symposium, Stanford University, California USA, June
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185 %% 28 - July 2, \textbf{2010}.
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186
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187 %% \litem{Improving torsion pendulum force sensitivity with LISA
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188 %% Pathfinder like interferometric angular read-out} Poster. 8th LISA
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189 %% Symposium, Stanford University, California USA, June 28 - July 02,
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190 %% \textbf{2010}.
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191
4
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192 %% \litem{Increased Brownian force noise from molecular impacts in a
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193 %% constrained volume} Talk. From Quantum to Cosmos 4 - Q2C4, Bremen,
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194 %% Germany, September 21-24, \textbf{2009}.
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195
4
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196 %% \litem{Gas damping in the LISA noise budget} Poster. 8th Edoardo
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197 %% Amaldi Conference on Gravitational Waves, New York, USA, June 21-26,
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198 %% \textbf{2009}.
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199
4
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200 %% \litem{An improved torsion pendulum for on-ground verification of the
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201 %% LISA gravitational reference sensor} Poster. 7th LISA Symposium,
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202 %% Barcelona, June 16-20, \textbf{2008}.
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203
4
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204 %% \litem{Characterization of the LISA gravitational reference sensor with
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205 %% an upgraded torsion pendulum} Poster. 7th Edoardo Amaldi Conference
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206 %% on Gravitational Waves, Sydney, Australia, July 8-14, \textbf{2007}.
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207 %% \end{enumerate}
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208
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209 \vfill
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210 \centering\footnotesize Last updated: \today.
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211
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212 \end{document}