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Limits on the strength of individual gravitational wave sources using high-cadence observations of PSR B1937+21 (2014)

First Author: Yi S

Attributed to: HYDRA: an HPC facility for Pulsar Astrophysics funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stu1826

Publication URI: http://dx.doi.org/10.1093/mnras/stu1826

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2