Multi-messenger observation

[Introduction to models]
Rn (/yr/Gpc3):(Norm. factor of the merger rate density)
τ (Gyr):(Delay time from formation to merger)
µ(M☉):(lower limit of mass)
c:(related with mass peak)
γ:(index of mass functoin tail)
mcut(M☉): (high mass cut)
ql:(lower cut of mass ratio)
σχ:(dispersion of effective spin)

[Introduction to models]
Rn (/yr/Gpc3):(Norm. factor of the merger rate density)
τ (Gyr):(Delay time from formation to merger)
µ(M☉):(lower limit of mass)
c:(related with mass peak)
γ:(index of mass functoin tail)
mcut(M☉):(high mass cut)
m_peak(M☉):(location of Gaussian mass peak)
m_peak_scale:(relative height of Gaussian mass peak)
m_peak_sig(M☉):(width of Gaussian mass peak)
ql:(lower cut of mass ratio)
σχ: (dispersion of effective spin)

[Introduction to models]
Rn (/yr/Gpc3):(Norm. factor of the merger rate density)

m_peak(M☉):(Peak of Gaussian mass)
m_scale(M☉):(Width of Gaussian mass)
m_low(M☉):(lower limit of mass)
m_high(M☉):(Upper limit of mass)
σχ:(dispersion of effective spin)

[Introduction to models]
Rn (/yr/Gpc3):(Norm. factor of the merger rate density)

m_peak(M☉):(Peak of neutron star mass distr.)
m_scale(M☉):(Width of NS mass distr.)
m_low(M☉):(lower limit of NS mass)
m_high(M☉):(Upper limit of mass)
µ(M☉):(lower limit of mass)
c:(related with mass peak)
γ:(index of mass functoin tail)
mcut(M☉):(high mass cut)
σχ:(dispersion of effective spin)

[Introduction to models]
Rn (/yr/Gpc3):(Norm. factor of the merger rate density)

m_peak(M☉):(Peak of neutron star mass distr.)
m_scale(M☉):(Width of NS mass distr.)
m_low(M☉):(lower limit of NS mass)
m_high(M☉):(Upper limit of mass)
µ(M☉):(lower limit of mass)
c:(related with mass peak)
γ:(index of mass functoin tail)
mcut(M☉):(high mass cut)
m_peak(M☉):(location of BH Gaussian mass peak)
m_peak_scale(M☉):(relative height of BH Gaussian mass peak)
m_peak_sig(M☉): (width of BH Gaussian mass peak)
σχ:(dispersion of effective spin)