scholarly journals Fisher versus Bayes: A comparison of parameter estimation techniques for massive black hole binaries to high redshifts with eLISA

2015 ◽  
Vol 91 (10) ◽  
Author(s):  
Edward K. Porter ◽  
Neil J. Cornish
Keyword(s):  
Black Hole ◽  
Parameter Estimation ◽  
Massive Black Hole ◽  
Estimation Techniques ◽  
Black Hole Binaries ◽  
Parameter Estimation Techniques

scholarly journals Effect of data gaps on the detectability and parameter estimation of massive black hole binaries with LISA

2021 ◽  
Vol 104 (4) ◽  
Author(s):  
Kallol Dey ◽  
Nikolaos Karnesis ◽  
Alexandre Toubiana ◽  
Enrico Barausse ◽  
Natalia Korsakova ◽  
...  
Keyword(s):  
Black Hole ◽  
Parameter Estimation ◽  
Massive Black Hole ◽  
Black Hole Binaries ◽  
Data Gaps

scholarly journals Taiji program: Gravitational-wave sources

2020 ◽  
Vol 35 (17) ◽  
pp. 2050075 ◽  
Author(s):  
Wen-Hong Ruan ◽  
Zong-Kuan Guo ◽  
Rong-Gen Cai ◽  
Yuan-Zhong Zhang
Keyword(s):  
Black Hole ◽  
Parameter Estimation ◽  
Gravitational Wave ◽  
Low Frequency ◽  
Gravitational Wave Detector ◽  
Massive Black Hole ◽  
Detection Rates ◽  
Black Hole Binaries ◽  
Wave Detector

We review potential low-frequency gravitational-wave sources, which are expected to be detected by Taiji, a Chinese space-based gravitational-wave detector, estimate the detection rates of these gravitational-wave sources and present the parameter estimation of massive black hole binaries.

scholarly journals The TianQin project: Current progress on science and technology

2020 ◽  
Author(s):  
Jianwei Mei ◽  
Yan-Zheng Bai ◽  
Jiahui Bao ◽  
Enrico Barausse ◽  
Lin Cai ◽  
...  
Keyword(s):  
Black Hole ◽  
Ecliptic Plane ◽  
Mass Ratio ◽  
Massive Black Hole ◽  
Black Hole Binaries ◽  
Compact Binaries ◽  
Single Body ◽  
Science Operations ◽  
New Generation ◽  
Research Facilities

Abstract TianQin is a planned space-based gravitational wave (GW) observatory consisting of three Earth-orbiting satellites with an orbital radius of about $10^5 \, {\rm km}$. The satellites will form an equilateral triangle constellation the plane of which is nearly perpendicular to the ecliptic plane. TianQin aims to detect GWs between $10^{-4} \, {\rm Hz}$ and $1 \, {\rm Hz}$ that can be generated by a wide variety of important astrophysical and cosmological sources, including the inspiral of Galactic ultra-compact binaries, the inspiral of stellar-mass black hole binaries, extreme mass ratio inspirals, the merger of massive black hole binaries, and possibly the energetic processes in the very early universe and exotic sources such as cosmic strings. In order to start science operations around 2035, a roadmap called the 0123 plan is being used to bring the key technologies of TianQin to maturity, supported by the construction of a series of research facilities on the ground. Two major projects of the 0123 plan are being carried out. In this process, the team has created a new-generation $17 \, {\rm cm}$ single-body hollow corner-cube retro-reflector which was launched with the QueQiao satellite on 21 May 2018; a new laser-ranging station equipped with a $1.2 \, {\rm m}$ telescope has been constructed and the station has successfully ranged to all five retro-reflectors on the Moon; and the TianQin-1 experimental satellite was launched on 20 December 2019—the first-round result shows that the satellite has exceeded all of its mission requirements.

scholarly journals Accretion of clumpy cold gas onto massive black hole binaries: a possible fast route to binary coalescence

2018 ◽  
Vol 479 (3) ◽  
pp. 3438-3455 ◽  
Author(s):  
Felipe G Goicovic ◽  
Cristián Maureira-Fredes ◽  
Alberto Sesana ◽  
Pau Amaro-Seoane ◽  
Jorge Cuadra
Keyword(s):  
Black Hole ◽  
Massive Black Hole ◽  
Black Hole Binaries ◽  
Fast Route ◽  
Cold Gas
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