While gravitational waves have not yet been measured directly, data analysis from detection experiments commonly includes an upper limit statement. Such upper limits may be derived via a frequentist or Bayesian approach; the theoretical implications are very different, and on the technical side, one notable difference is that one case requires maximization of the likelihood function over parameter space, while the other requires integration. Using a simple example (detection of a sinusoidal signal in white Gaussian noise), we investigate the differences in performance and interpretation, and the effect of the "trials factor", or "look-elsewhere effect"
We present a method of searching for, and parametrizing, signals from known radio pulsars in data fr...
When searching over a large parameter space for anomalies such as events, peaks, objects, or particl...
The first science run of the LIGO and GEO gravitational wave detectors presented the opportunity to ...
While gravitational waves have not yet been measured directly, data analysis from detection experime...
We investigate the Bayesian framework for detection of continuous gravitational waves (GWs) in the c...
This work concerns Bayesian detection statistics in targeted searches for continuous gravitational w...
A recent letter (Allen et al., to appear in PRL) reports an upper limit on the galactic compact bina...
The phase parameters of matched-filtering searches for continuous gravitational-wave signals are sky...
In counting experiments, one can set an upper limit on the rate of a Poisson process based on a coun...
When looking for gravitational wave signals from known pulsars, targets have been treated using inde...
We develop a Bayesian treatment of the problem of detecting unmodelled gravitational wave bursts usi...
In a previous paper (paper I), we derived a set of near-optimal signal detection techniques for grav...
The use of the loudest observed event to generate statistical statements about rate and strength has...
Recently, many different pulsar timing array (PTA) collaborations have reported strong evidence for ...
We consider the problem of detecting a burst signal of unknown shape. We introduce a statistic which...
We present a method of searching for, and parametrizing, signals from known radio pulsars in data fr...
When searching over a large parameter space for anomalies such as events, peaks, objects, or particl...
The first science run of the LIGO and GEO gravitational wave detectors presented the opportunity to ...
While gravitational waves have not yet been measured directly, data analysis from detection experime...
We investigate the Bayesian framework for detection of continuous gravitational waves (GWs) in the c...
This work concerns Bayesian detection statistics in targeted searches for continuous gravitational w...
A recent letter (Allen et al., to appear in PRL) reports an upper limit on the galactic compact bina...
The phase parameters of matched-filtering searches for continuous gravitational-wave signals are sky...
In counting experiments, one can set an upper limit on the rate of a Poisson process based on a coun...
When looking for gravitational wave signals from known pulsars, targets have been treated using inde...
We develop a Bayesian treatment of the problem of detecting unmodelled gravitational wave bursts usi...
In a previous paper (paper I), we derived a set of near-optimal signal detection techniques for grav...
The use of the loudest observed event to generate statistical statements about rate and strength has...
Recently, many different pulsar timing array (PTA) collaborations have reported strong evidence for ...
We consider the problem of detecting a burst signal of unknown shape. We introduce a statistic which...
We present a method of searching for, and parametrizing, signals from known radio pulsars in data fr...
When searching over a large parameter space for anomalies such as events, peaks, objects, or particl...
The first science run of the LIGO and GEO gravitational wave detectors presented the opportunity to ...