  It is well-known that there are two types of gamma-ray bursts (GRBs):
short/hard and long/soft ones, respectively. The long GRBs are coupled to
supernovae, but the short ones are associated with the so called macronovae
(also known as kilonovae), which can serve as the sources of gravitational
waves as well. The kilonovae can arise from the merging of two neutron-stars.
The neutron stars can be substituded by more massive black holes as well.
Hence, the topic of gamma-ray bursts (mainly the topic of short ones) and the
topic of massive binaries, are strongly connected.
  In this contribution, the redshifts of GRBs are studied. The surprising
result - namely that the apparently fainter GRBs can be in average at smaller
distances - is discussed again. In essence, the results of M\'esz\'aros et al.
(2011) are studied again using newer samples of GRBs. The former result is
confirmed by the newer data.
