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