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Global Analysis of LISA Data with Galactic Binaries and Massive Black Hole Binaries
Stefan H. Strub, Luigi Ferraioli, Cédric Schmelzbach +2
The Laser Interferometer Space Antenna (LISA) is a planned space-based observatory to measure gravitational waves in the millihertz frequency band. This frequency band is expected…
Data series subtraction with unknown and unmodeled background noise
Stefano Vitale, Giuseppe Congedo, Rita Dolesi +20
LISA Pathfinder (LPF), ESA's precursor mission to a gravitational wave observatory, will measure the degree to which two test-masses can be put into free-fall, aiming to demonstrat…
Bayesian Model Selection for LISA Pathfinder
Nikolaos Karnesis, Miquel Nofrarias, Carlos F. Sopuerta +11
The main goal of the LISA Pathfinder (LPF) mission is to fully characterize the acceleration noise models and to test key technologies for future space-based gravitational-wave obs…
Bayesian Inference for LISA Pathfinder using Markov Chain Monte Carlo Methods
Luigi Ferraioli, Edward K. Porter, Eric Plagnol
We present a parameter estimation procedure based on a Bayesian framework by applying a Markov Chain Monte Carlo algorithm to the calibration of the dynamical parameters of a space…
Analysis of the residual force noise for the LISA Technology Package
Luigi Ferraioli, Michele Armano, Giuseppe Congedo +10
The analysis of the noise sources perturbing a test mass (TM) geodesic motion is the main scientific objective of the LISA Technology Package experiment (LTP) on board of the LISA…
Quantitative Analysis of LISA Pathfinder Test Mass Noise
Luigi Ferraioli, Martin Hewitson, Giuseppe Congedo +4
In this paper we discuss two main problems associated with the analysis of the data from LISA Pathfinder (LPF): i) Excess noise detection and ii) Noise parameter identification. Th…