The search for continuous gravitational waves in a wide parameter space at fixed computing cost is most efficiently done with semicoherent methods, e.g. StackSlide, due to the prohibitive computing cost of the fully coherent search strategies. Prix&Shaltev arXiv:1201.4321 have developed a semi-analytic method for finding \emph{optimal} StackSlide parameters at fixed computing cost under ideal data conditions, i.e. gap-less data and constant noise floor. In this work we consider more realistic conditions by allowing for gaps in the data and changes in noise level. We show how the sensitivity optimization can be decoupled from the data selection problem. To find optimal semicoherent search parameters we apply a numerical optimization using as...
Leveraging Markov chain Monte Carlo (MCMC) optimization of the F-statistic, we introduce a method fo...
We derive two different methods to compute the minimal required integration time of a fully coherent...
The search for continuous gravitational waves from unknown isolated sources is computationally limit...
The search for continuous gravitational waves in a wide parameter space at fixed computing cost is m...
Coherent wide parameter-space searches for continuous gravitational waves are typically limited in s...
This paper presents an efficient numerical sensitivity-estimation method and implementation for cont...
This paper presents an efficient numerical sensitivity-estimation method and implementation for cont...
All-sky surveys for isolated continuous gravitational waves present a significant data-analysis chal...
Wide parameter space searches for long lived continuous gravitational wave signals are computational...
We derive a simple algebraic criterion to select the optimal detector network for a coherent wide pa...
All-sky searches for gravitational-wave pulsars are generally limited in sensitivity by the finite a...
Fully coherent searches (over realistic ranges of parameter space and year-long observation times) f...
Continuous gravitational-wave (CW) signals such as emitted by spinning neutron stars are an importan...
Many continuous gravitational wave searches are affected by instrumental spectral lines that could b...
The search for continuous gravitational-wave signals requires the development of techniques that can...
Leveraging Markov chain Monte Carlo (MCMC) optimization of the F-statistic, we introduce a method fo...
We derive two different methods to compute the minimal required integration time of a fully coherent...
The search for continuous gravitational waves from unknown isolated sources is computationally limit...
The search for continuous gravitational waves in a wide parameter space at fixed computing cost is m...
Coherent wide parameter-space searches for continuous gravitational waves are typically limited in s...
This paper presents an efficient numerical sensitivity-estimation method and implementation for cont...
This paper presents an efficient numerical sensitivity-estimation method and implementation for cont...
All-sky surveys for isolated continuous gravitational waves present a significant data-analysis chal...
Wide parameter space searches for long lived continuous gravitational wave signals are computational...
We derive a simple algebraic criterion to select the optimal detector network for a coherent wide pa...
All-sky searches for gravitational-wave pulsars are generally limited in sensitivity by the finite a...
Fully coherent searches (over realistic ranges of parameter space and year-long observation times) f...
Continuous gravitational-wave (CW) signals such as emitted by spinning neutron stars are an importan...
Many continuous gravitational wave searches are affected by instrumental spectral lines that could b...
The search for continuous gravitational-wave signals requires the development of techniques that can...
Leveraging Markov chain Monte Carlo (MCMC) optimization of the F-statistic, we introduce a method fo...
We derive two different methods to compute the minimal required integration time of a fully coherent...
The search for continuous gravitational waves from unknown isolated sources is computationally limit...