  Bimodal distribution of the observed duration of gamma-ray bursts (GRBs) has
led to two distinct progenitors; compact star mergers, either two neutron stars
(NSs) or a NS and a black hole (BH), for short GRBs (SGRBs), and so-called
collapsars for long GRBs (LGRBs). It is therefore expected that formation rate
(FR) of LGRBs should be similar to the cosmic star formation rate (SFR), while
that of SGRBs to be delayed relative to the SFR. The localization of some LGRBs
in and around the star forming regions of host galaxies and some SGRBs away
form such regions support this expectation. Another distinct feature of SGRBs
is their association with gravitational wave (GW) sources and kilonovae.
However, several independent investigations of the FRs of long and short
bursts, using the Efron-Petrosian non-parametric method have shown a LGRB FR
that is significantly larger than SFR at low redhift, and similar to the FR of
SGRBs. In addition, recent discovery of association of a low redshift long
GRB211211A with a kilonova raises doubt about its collapsar origin. In this
letter we review these results and show that low redshift LGRBs could also have
compact star mergers as progenitor increasing the expected rate of the GW
sources and kilonovae significantly.
