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Table D.1.

List of variables used frequently in the text

Notation Definition Reference
tini cosmic time of the formation of a ZAMS binary tini = tobs − tdel
tobs cosmic time at which the compact binary is observed to merge.
tdel delay time tdel = tevol + tmerg
tevol time of evolution from ZAMS to the formation of a compact binary system
tmerg time from formation of a compact binary till the merger
ℛ(z) merger rate density per unit redshift as a function of redshift Eq. 1
SFR(z) star formation rate density as a function of redshift Figure 1
Z metallicity
Msim total mass of all stars accompanying the stellar evolution,
leading to formation of compact object binaries
including the binaries as well as the single stars.
s, mock, Ms, mock, zs, mock subscript (s, mock) denotes true source parameters
of a binary in the mock population
s, det, Ms, det, zs, det subscript (s, det) denotes true source parameters
of detected sources
med, det, Mmed, det, zmed, det subscript (med, det) denotes the median of the estimated see Fig. 5 in SB2
posterior distribution for each parameter for an example of
posterior distributions
Nmock number of binaries in a mock population
Ndet number of detected binaries
Nyr number of mergers per year
Tmock time during which binaries in the mock population are expected to merger Eq. 31
Rmer(zs, mock) merger rate densities as a function of redshift Eq. 32
assuming true source redshift in the mock population
Rmer(zs, det) merger rate densities as a function of redshift Eq. 32
assuming true sources redshift of detected sources
Rmer(zmed, det) merger rate densities as a function of redshift with the median Eq. 32
of the estimated posterior distribution of the redshift of detected sources
subscript ’sec’ parameters of the secondary population
𝒟(zi, zi + 1) detection efficiency in the redshift bin (zi, zi + 1) Eq. 34
Rmer, recon reconstructed merger rate density taking into account the detection efficiency Eq. 35
SFR′ merger-rate-weighted SFR

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