Effect of calibration errors on Bayesian parameter estimation for gravitational wave signals from inspiral binary systems in the advanced detectors era
Salvatore Vitale, Walter Del Pozzo, Tjonnie G. F. Li, Chris Van Den, Broeck, Ilya Mandel, Ben Aylott, John Veitch

TL;DR
This paper assesses how calibration uncertainties in advanced gravitational-wave detectors affect the accuracy of parameter estimation for inspiral binary signals, finding that typical calibration errors have limited impact on key parameters.
Contribution
It provides a quantitative analysis of calibration error effects on parameter estimation accuracy for gravitational wave signals from inspiral binaries.
Findings
Calibration errors cause less than 20% systematic bias in mass parameters.
Sky localization errors due to calibration are below 50% of statistical uncertainties.
Calibration errors at estimated levels are not significantly detrimental to parameter estimation.
Abstract
By 2015 the advanced versions of the gravitational-wave detectors Virgo and LIGO will be online. They will collect data in coincidence with enough sensitivity to potentially deliver multiple detections of gravitation waves from inspirals of compact-object binaries. This work is focused on understanding the effects introduced by uncertainties in the calibration of the interferometers. We consider plausible calibration errors based on estimates obtained during LIGO's fifth and Virgo's third science runs, which include frequency-dependent amplitude errors of and frequency-dependent phase errors of degrees in each instrument. We quantify the consequences of such errors estimating the parameters of inspiraling binaries. We find that the systematics introduced by calibration errors on the inferred values of the chirp mass and mass ratio are smaller than 20% of the…
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