Characteristic strain amplitude of the stochastic gravitational wave background emitted by mergers of supermassive binary black holes
The table lists 18 sets of MBH-host galaxy relations occurred in the literature during the past two decades. For each MBH-host galaxy relation, the resulting characteristic strain amplitude of the stochastic gravitational wave background are estimated and given, along with the turnover frequency towards the low-frequency end of the spectra as well as the power index of the spectra. Please refer to Table 1 in Chen, Yu, & Lu (2020, ApJ, 897, 86).
· Data Access ·
Table1.txt
1.84 kB
♦Introduction♦
Keywords
Gravitational wave , Galaxy mergers , Massive black holes
Data Volume
2122317824 Bytes
2 files
Sharing Method
Sharing Scope
♦Contact Author♦
Author
Yunfeng Chen, Qingjuan Yu, Youjun Lu
Email
yuqj(at)pku.edu.cn
♦Contact Publisher
♦
Email
support(at)china-vo.org
Phone
+86-10-64807973
Institution
National Astronomical Data Center
♦Tags♦
subject
Cosmology and Galaxies
data type
Digitilized Data
data level
Level 3
production age
1980-
content level
Research