title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð»Ð¸Ð½Ð½ÑÑ Ð¶ÐµÑÑÐºÐ¸Ñ Ð³Ð°Ð¼Ð¼Ð°-Ð²ÑÐ¿Ð»ÐµÑÐºÐ¾Ð² Ð¿Ð¾ Ð´Ð°Ð½Ð½ÑÐ¼ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ° ÐÐ¾Ð½ÑÑ-ÐÐ¸Ð½Ð´
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
title: Research of long hard gamma-ray bursts using data from the Konus-wind experiment
Creators: name: ÐÐµÐ¼Ð¸Ð½, ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2020
Subjects: Ð³Ð°Ð¼Ð¼Ð°-Ð²ÑÐ¿Ð»ÐµÑÐºÐ¸
ÐºÑÐ°ÑÐ½ÑÐµ ÑÐ¼ÐµÑÐµÐ½Ð¸Ñ Ð³Ð°Ð¼Ð¼Ð°-Ð²ÑÐ¿Ð»ÐµÑÐºÐ¾Ð²
ÑÐ½ÐµÑÐ³Ð¾Ð²ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð³Ð°Ð¼Ð¼Ð°-Ð²ÑÐ¿Ð»ÐµÑÐºÐ¾Ð²
Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐ¿ÐµÐºÑÑÐ°Ð»ÑÐ½Ð°Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ° Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð²ÑÑÐ¾ÐºÐ¸Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¹
gamma-ray burst
red shifts of gamma-ray bursts
energy release of gamma-ray burst
additional spectral component in the high energy region

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð»Ð¸Ð½Ð½ÑÑ ÑÑÐºÐ¸Ñ Ð¶ÐµÑÑÐºÐ¸Ñ Ð³Ð°Ð¼Ð¼Ð°-Ð²ÑÐ¿Ð»ÐµÑÐºÐ¾Ð², Ð·Ð°ÑÐµÐ³Ð¸ÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð¼ âKonus-Windâ Ñ 1994 Ð¿Ð¾ 2019 Ð³Ð¾Ð´. ÐÐ· 10% ÑÐ°Ð¼ÑÑ ÑÑÐºÐ¸Ñ Ð²ÑÐ¿Ð»ÐµÑÐºÐ¾Ð², Ð·Ð°ÑÐµÐ³Ð¸ÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ âKonus-Windâ Ð±ÑÐ»Ð¸ Ð¾ÑÐ¾Ð±ÑÐ°Ð½Ñ Ð²ÑÐ¿Ð»ÐµÑÐºÐ¸ ÑÐ¾ Ð·Ð½Ð°ÑÐ¸Ð¼ÑÐ¼ Ð¿ÑÐµÐ²ÑÑÐµÐ½Ð¸ÐµÐ¼ Ð½Ð°Ð´ ÑÐ¾Ð½Ð¾Ð¼ Ð½Ð° Ð²ÑÑÐ¾ÐºÐ¸Ñ ÑÐ½ÐµÑÐ³Ð¸ÑÑ, ÐºÐ¾ÑÐ¾ÑÑÐµ ÑÐ¾ÑÑÐ°Ð²Ð¸Ð»Ð¸ Ð²ÑÐ±Ð¾ÑÐºÑ Ð¸Ð· 46 Ð²ÑÐ¿Ð»ÐµÑÐºÐ¾Ð². ÐÐ¾Ð»ÑÑÐµÐ½Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ ÑÐ¿ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÑ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð´Ð»Ñ Ð²ÑÐ±ÑÐ°Ð½Ð½ÑÑ ÑÐ¿ÐµÐºÑÑÐ¾Ð² Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿Ð°ÐºÐµÑÐ° XSPEC. ÐÐ¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ ÑÐ¿ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð±ÑÐ»Ð¸ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ñ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð²ÑÐ¿Ð»ÐµÑÐºÐ¸ Ñ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ¿ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð¹ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð²ÑÑÐ¾ÐºÐ¸Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¹. ÐÑÐ»Ð° Ð¾ÑÐµÐ½ÐµÐ½Ð° ÑÐ°ÑÑÐ¾ÑÐ° Ð¿Ð¾Ð´Ð¾Ð±Ð½ÑÑ ÑÐ¾Ð±ÑÑÐ¸Ð¹. ÐÐ¾ ÐºÐ¾ÑÑÐµÐ»ÑÑÐ¸ÑÐ¼ Ð¸Ð·Ð¾ÑÑÐ¾Ð¿Ð½Ð¾Ðµ ÑÐ½ÐµÑÐ³Ð¾Ð²ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ â Ð¿Ð¸ÐºÐ¾Ð²Ð°Ñ ÑÐ½ÐµÑÐ³Ð¸Ñ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¿ÐµÐºÑÑÐ° (ÑÐ¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ðµ ÐÐ¼Ð°ÑÐ¸) Ð¸ Ð¸Ð·Ð¾ÑÑÐ¾Ð¿Ð½Ð°Ñ ÑÐ²ÐµÑÐ¸Ð¼Ð¾ÑÑÑ â Ð¿Ð¸ÐºÐ¾Ð²Ð°Ñ ÑÐ½ÐµÑÐ³Ð¸Ñ Ð¿Ð¸ÐºÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¿ÐµÐºÑÑÐ° (ÑÐ¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ðµ ÐÐ¾Ð½ÐµÑÐ¾ÐºÑ) Ð¾ÑÐµÐ½ÐµÐ½Ñ ÐºÑÐ°ÑÐ½Ð¾Ðµ ÑÐ¼ÐµÑÐµÐ½Ð¸Ðµ z, Ð¿Ð¸ÐºÐ¾Ð²Ð°Ñ ÑÐ½ÐµÑÐ³Ð¸Ñ Ð¸ ÑÐ½ÐµÑÐ³Ð¾Ð²ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð²ÑÐ¿Ð»ÐµÑÐºÐ° Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¾ÑÑÑÐµÑÐ° Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ°. ÐÐ¾Ð»ÑÑÐµÐ½Ð¾ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð²ÑÐ¿Ð»ÐµÑÐºÐ¾Ð² Ð¿Ð¾ Ð¿Ð¸ÐºÐ¾Ð²Ð¾Ð¹ ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¾ÑÑÑÐµÑÐ° Ð½Ð°Ð±Ð»ÑÐ´Ð°ÑÐµÐ»Ñ Ð¸ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¾ÑÑÑÐµÑÐ° Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ°.
description: In this paper, a detailed study of long, bright, hard gamma-ray bursts recorded by the Konus-Wind instrument from 1994 to 2019 was performed. From the 10% of the brightest bursts recorded by Konus-Wind, bursts with a significant excess over the background at high energies were selected, which made up a sample of 46 bursts. Parameters of spectral models for selected spectra were obtained using the XSPEC package. Based on the results of spectral analysis, bursts with an additional spectral component in the high-energy region were detected and studied. The correlations of isotropic energy release â peak energy of the integral spectrum (Amati ratio) and isotropic luminosity-peak energy of the peak spectrum (Yonetoku ratio) are used to estimate the redshift z, peak energy, and energy release of the burst in the source reference system. The distribution of bursts by peak energy in the observer's frame of reference and in the source's frame of reference is obtained.