  The RELEC scientific instrumentation onboard the Vernov spacecraft launched
on July 8, 2014, included the DRGE gamma-ray and electron spectrometer. This
instrument incorporates a set of scintillation phoswich detectors, including
four identical X-ray and gamma-ray detectors in the energy range from 10 keV to
3 MeV with a total area of $\sim$500 $cm^{2}$ directed toward the nadir, and an
electron spectrometer containing three mutually orthogonal detector units with
a geometry factor of $\sim$2 $cm^{2} sr$, which is also sensitive to X-rays and
gamma-rays. The goal of the space experiment with the DRGE instrument was to
investigate phenomena with fast temporal variability, in particular,
terrestrial gamma-ray flashes (TGFs) and magnetospheric electron
precipitations. However, the detectors of the DRGE instrument could record
cosmic gamma-ray bursts (GRBs) and allowed one not only to perform a detailed
analysis of the gamma-ray variability but also to compare the time profiles
with the measurements made by other instruments of the RELEC scientific
instrumentation (the detectors of optical and ultraviolet flashes, the
radio-frequency and low-frequency analyzers of electromagnetic field
parameters). We present the results of our observations of cosmic GRB 141011A
and GRB 141104A, compare the parameters obtained in the GBM/Fermi and KONUSWind
experiments, and estimate the redshifts and Eiso for the sources of these GRBs.
The detectability of GRBs and good agreement between the independent estimates
of their parameters obtained in various experiments are an important factor of
the successful operation of similar detectors onboard the Lomonosov spacecraft.
