Reviewed ou2018optimal

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Manos Katsomallos 2021-09-07 15:16:37 +03:00
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@ -274,6 +274,22 @@ private and eligible for publishing.
The authors compare their design with that of~\cite{chen2012differentially} and~\cite{he2015dpt} by running several tests, and ascertain that it outperforms them in terms of data utility.
However, due to DP-Star's privacy budget distribution to its different phases, for small values of $\varepsilon$ the framework's privacy performance is inferior to that of its competitors.
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\hypertarget{ou2018optimal}{Ou et al.}~\cite{ou2018optimal} designed \emph{FGS-Pufferfish} for publishing temporally correlated trajectory data while protecting temporal correlation.
FGS-Pufferfish transforms a user's daily trajectories into a set of sine and cosine waves of different frequencies along with the corresponding Fourier coefficients.
Then, it adds Laplace noise to the Fourier coefficients' geometric sum.
The authors obtain the optimal noisy Fourier coefficients by solving the constrained optimization problem via the Lagrange Multiplier method depending on the available privacy budget.
They evaluate both the location data utility and the temporal correlation utility.
The experimental evaluation shows that FGS-Pufferfish outperforms CTS-DP~\cite{wang2017cts} in terms of the trade-off between privacy and location utility.
\subsection{Infinite observation}
\label{subsec:micro-infinite}
@ -422,7 +438,7 @@ Last but not least, the technique requires the calculation of the temporal priva
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