Cosmic Gamma-Ray Bursts Detected in the RELEC Experiment onboard the Vernov Satellite

TL;DR

This paper reports on the detection and analysis of cosmic gamma-ray bursts using the DRGE instrument onboard the Vernov satellite, comparing results with other experiments and estimating source parameters.

Contribution

It presents the first detailed analysis of cosmic GRBs detected by the Vernov satellite's DRGE instrument, including parameter comparison with other space-based detectors.

Findings

Detected and analyzed GRB 141011A and GRB 141104A.

Compared parameters with Fermi/GBM and KONUS-Wind data.

Estimated redshifts and Eiso for the GRB sources.

Abstract

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.