2023
DOI: 10.3847/1538-4357/acaf80
|View full text |Cite
|
Sign up to set email alerts
|

Opportunistic Search for Continuous Gravitational Waves from Compact Objects in Long-period Binaries

Abstract: Most all-sky searches for continuous gravitational waves assume the source to be isolated. In this paper, we allow for an unknown companion object in a long-period orbit and opportunistically use previous results from an all-sky search for isolated sources to constrain the continuous gravitational-wave amplitude over a large and unexplored range of binary orbital parameters without explicitly performing a dedicated search for binary systems. The resulting limits are significantly more constraining than any exi… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1

Citation Types

0
3
0

Year Published

2023
2023
2024
2024

Publication Types

Select...
3
1

Relationship

1
3

Authors

Journals

citations
Cited by 4 publications
(3 citation statements)
references
References 24 publications
0
3
0
Order By: Relevance
“…In addition, searches for isolated stars retain some sensitivity to long-period binaries, as shown in a recent studies (Singh et al 2019;Singh and Papa 2023).…”
Section: Results From All-sky Isolated-star Searches Of Ligo and Virg...mentioning
confidence: 90%
“…In addition, searches for isolated stars retain some sensitivity to long-period binaries, as shown in a recent studies (Singh et al 2019;Singh and Papa 2023).…”
Section: Results From All-sky Isolated-star Searches Of Ligo and Virg...mentioning
confidence: 90%
“…Since one operates at a limited computing budget, this results in a lower sensitivity. We have not considered (Singh & Papa 2023), which presents the most stringent upper limits for continuous waves from binary systems, but with orbital parameters unlikely to pertain to recycled neutron stars. Since our synthetic signals contain no information on binary parameters, for any search considered, we count as detectable any signal whose amplitude lays above the most sensitive upper limit set at the signal's frequency, independently of ḟ and orbital parameters.…”
Section: Recycled Neutron Starsmentioning
confidence: 99%
“…Because one operates within a limited computing budget, this results in a lower sensitivity. We have not considered Singh & Papa (2023), who searched orbital parameters that are unlikely to pertain to recycled neutron stars. We determine the detectability of isolated neutron stars and neutron stars in binaries separately.…”
Section: Recycled Neutron Starsmentioning
confidence: 99%