English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

Deep learning for clustering of continuous gravitational wave candidates II: identification of low-SNR candidates

MPS-Authors
/persons/resource/persons243907

Beheshtipour,  Banafsheh
Searching for Continuous Gravitational Waves, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons20662

Papa,  Maria Alessandra
Searching for Continuous Gravitational Waves, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)

2012.04381.pdf
(Preprint), 4MB

Supplementary Material (public)
There is no public supplementary material available
Citation

Beheshtipour, B., & Papa, M. A. (2021). Deep learning for clustering of continuous gravitational wave candidates II: identification of low-SNR candidates. Physical Review D, 103(6): 064027. doi:10.1103/PhysRevD.103.064027.


Cite as: https://hdl.handle.net/21.11116/0000-0007-AE96-C
Abstract
Broad searches for continuous gravitational wave signals rely on hierarchies
of follow-up stages for candidates above a given significance threshold. An
important step to simplify these follow-ups and reduce the computational cost
is to bundle together in a single follow-up nearby candidates. This step is
called clustering and we investigate carrying it out with a deep learning
network. In our first paper [1], we implemented a deep learning clustering
network capable of correctly identifying clusters due to large signals. In this
paper, a network is implemented that can detect clusters due to much fainter
signals. These two networks are complementary and we show that a cascade of the
two networks achieves an excellent detection efficiency across a wide range of
signal strengths, with a false alarm rate comparable/lower than that of methods
currently in use.