No tension between pulsar timing array upper limits on the nano-Hertz gravitational wave background and assembly models of massive black hole binaries (2020)
Attributed to:
Astrophysics at the University of Birmingham
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1088/1742-6596/1468/1/012214
Publication URI: http://dx.doi.org/10.1088/1742-6596/1468/1/012214
Type: Journal Article/Review
Parent Publication: Journal of Physics: Conference Series
Issue: 1