Add to ORKGAbstract. We derive two different methods to compute the minimal required integration time of a fully coherent follow-up of candidates produced in wide parameter space semi-coherent searches, such as global correlation StackSlide searches using Einstein@Home. We numerically compare these methods in terms of integration duration and computing cost. In a Monte Carlo study we confirm that we can achieve the required detection probability. 1
We present a method for coherently combining short data segments from gravitational-wave detectors t...
The space of phase parameters (sky position, frequency, spindowns) of a coherent matched-filtering s...
A novel hierarchical semicoherent technique is presented for all-sky surveys for continuous gravitat...
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...
We characterize and present the details of the follow-up method used on the most significant outlier...
Fully coherent searches (over realistic ranges of parameter space and year-long observation times) f...
This article discusses the potential advantages of a data processing technique for continuous gravit...
Coherent wide parameter-space searches for continuous gravitational waves are typically limited in s...
We describe an efficient method of matched filtering over long (greater than 1 day) time baselines s...
Leveraging Markov chain Monte Carlo (MCMC) optimization of the F-statistic, we introduce a method fo...
We describe an efficient method of matched filtering over long (greater than 1 day) time baselines s...
Roughly every 2-10 min, a pair of stellar-mass black holes merge somewhere in the Universe. A small ...
The search for continuous gravitational waves in a wide parameter space at fixed computing cost is m...
This paper presents an efficient numerical sensitivity-estimation method and implementation for cont...
We present a method for coherently combining short data segments from gravitational-wave detectors t...
The space of phase parameters (sky position, frequency, spindowns) of a coherent matched-filtering s...
A novel hierarchical semicoherent technique is presented for all-sky surveys for continuous gravitat...
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...
We characterize and present the details of the follow-up method used on the most significant outlier...
Fully coherent searches (over realistic ranges of parameter space and year-long observation times) f...
This article discusses the potential advantages of a data processing technique for continuous gravit...
Coherent wide parameter-space searches for continuous gravitational waves are typically limited in s...
We describe an efficient method of matched filtering over long (greater than 1 day) time baselines s...
Leveraging Markov chain Monte Carlo (MCMC) optimization of the F-statistic, we introduce a method fo...
We describe an efficient method of matched filtering over long (greater than 1 day) time baselines s...
Roughly every 2-10 min, a pair of stellar-mass black holes merge somewhere in the Universe. A small ...
The search for continuous gravitational waves in a wide parameter space at fixed computing cost is m...
This paper presents an efficient numerical sensitivity-estimation method and implementation for cont...
We present a method for coherently combining short data segments from gravitational-wave detectors t...
The space of phase parameters (sky position, frequency, spindowns) of a coherent matched-filtering s...
A novel hierarchical semicoherent technique is presented for all-sky surveys for continuous gravitat...