Abstract:This article presents the early results of synchronous multiwavelength observations of one of the brightest gamma-ray bursts (GRBs) GRB 160625B with the detailed continuous fast optical photometry of its optical counterpart obtained by MASTER and with hard X-ray and gamma-ray emission, obtained by the Lomonosov and Konus-Wind spacecraft. The detailed photometry led us to detect the quasi-periodical emission components in the intrinsic optical emission. As a result of our analysis of synchronous multiwavelength… Show more
“…Thus, the work is devoted to the interpretation of synchronous multiwavelength observations of the gamma-ray burst GRB 160625B by Russian space and ground systems [13,27] On June 25, 2016, one of the brightest flares in the history of GRB observations -GRB 160625B, occurred. The most detailed optical observations were made by the Global Network of Robotic Telescopes of Moscow State University MASTER.…”
Section: Pos(multif2023)065mentioning
confidence: 99%
“…Extreme phenomena still have many problems and have been studied very intensively in recent years . The effective ways of their studing involve using multichannel and multi-wavelength observations by fully robotic telescopes, distributed by Earth for full time control of near and far space like MASTER Global Robotic Net [12][13][14][15][16]19,20,[22][23][24][25][26][27]35,43,47,[49][50][51]67,[85][86][87][88][89][90][91].…”
Section: Pos(multif2023)065mentioning
confidence: 99%
“…As a result of our analysis of synchronous multiwavelength observations, we propose a three-stage collapse scenario for this long and bright GRB. We suggest that quasiperiodic fluctuations during prompt stage may be associated with forced precession of a self-gravitating rapidly rotating superdense body (spinar [27], Figure 10 ), whose evolution is determined by a powerful magnetic field. The spinar's mass allows it to collapse into a black hole at the end of evolution.…”
mentioning
confidence: 96%
“…After the outstanding discovery of the intrinsic optical emission of 8th magnitude gamma-ray bursts (Akerloff et al in 1999 [11]), it became clear that extreme processes can be observed with the smallest but robotic telescopes. Since 2002, the MASTER team (Lipunov, 2003 [12]) has joined the search for superpowerful phenomena in the Universe, which has discovered more than 3500 optical flares in the Universe to date [12][13][14][15][16][17][18][19][20][22][23][24][25][26][27]. Among the most significant discoveries there were the discovery of the polarization of the intrinsic optical emission of gamma-ray bursts (Troja et al in 2017 [13]) and the independent discovery of the kilonova GW170817 (Lipunov et al in 2017 [14-17]) .…”
This article presents some of the results of the MASTER Global Robotic Network ov few years. But it begins with a theoretical substantiation of the main goal of our research study of extreme phenomena of the Universe. We are talking about processes that, in terms of their power, approach the power of the Big Bang and g observations are always part of multi the first registration of Orphan optical flare at the growth stage (AT2021lfa), the study of the brightest gamma-ray burst in the entire history of their study, extreme GRB 221009A, the multiwavelength study of the flat spectrum radio flaring episodes, the installation of a new MASTER highlights. We talk about the Three 160625B model and huge FRB monitoring by Global MASTER pandemic , about probing into emission mechanisms of GRB 190530A using time spectra and polarization data, about exploring the early afterglow of GRB 190829A. In conclusion, we discuss our proposed optical candidate for a high have discovered the effect of a rapid decrease in the brightness of the blazar PKS 0735+17 at the time of the unique multiple detection of the high Multifrequency Behaviour of High Energy Cosmic Sources XIV (
“…Thus, the work is devoted to the interpretation of synchronous multiwavelength observations of the gamma-ray burst GRB 160625B by Russian space and ground systems [13,27] On June 25, 2016, one of the brightest flares in the history of GRB observations -GRB 160625B, occurred. The most detailed optical observations were made by the Global Network of Robotic Telescopes of Moscow State University MASTER.…”
Section: Pos(multif2023)065mentioning
confidence: 99%
“…Extreme phenomena still have many problems and have been studied very intensively in recent years . The effective ways of their studing involve using multichannel and multi-wavelength observations by fully robotic telescopes, distributed by Earth for full time control of near and far space like MASTER Global Robotic Net [12][13][14][15][16]19,20,[22][23][24][25][26][27]35,43,47,[49][50][51]67,[85][86][87][88][89][90][91].…”
Section: Pos(multif2023)065mentioning
confidence: 99%
“…As a result of our analysis of synchronous multiwavelength observations, we propose a three-stage collapse scenario for this long and bright GRB. We suggest that quasiperiodic fluctuations during prompt stage may be associated with forced precession of a self-gravitating rapidly rotating superdense body (spinar [27], Figure 10 ), whose evolution is determined by a powerful magnetic field. The spinar's mass allows it to collapse into a black hole at the end of evolution.…”
mentioning
confidence: 96%
“…After the outstanding discovery of the intrinsic optical emission of 8th magnitude gamma-ray bursts (Akerloff et al in 1999 [11]), it became clear that extreme processes can be observed with the smallest but robotic telescopes. Since 2002, the MASTER team (Lipunov, 2003 [12]) has joined the search for superpowerful phenomena in the Universe, which has discovered more than 3500 optical flares in the Universe to date [12][13][14][15][16][17][18][19][20][22][23][24][25][26][27]. Among the most significant discoveries there were the discovery of the polarization of the intrinsic optical emission of gamma-ray bursts (Troja et al in 2017 [13]) and the independent discovery of the kilonova GW170817 (Lipunov et al in 2017 [14-17]) .…”
This article presents some of the results of the MASTER Global Robotic Network ov few years. But it begins with a theoretical substantiation of the main goal of our research study of extreme phenomena of the Universe. We are talking about processes that, in terms of their power, approach the power of the Big Bang and g observations are always part of multi the first registration of Orphan optical flare at the growth stage (AT2021lfa), the study of the brightest gamma-ray burst in the entire history of their study, extreme GRB 221009A, the multiwavelength study of the flat spectrum radio flaring episodes, the installation of a new MASTER highlights. We talk about the Three 160625B model and huge FRB monitoring by Global MASTER pandemic , about probing into emission mechanisms of GRB 190530A using time spectra and polarization data, about exploring the early afterglow of GRB 190829A. In conclusion, we discuss our proposed optical candidate for a high have discovered the effect of a rapid decrease in the brightness of the blazar PKS 0735+17 at the time of the unique multiple detection of the high Multifrequency Behaviour of High Energy Cosmic Sources XIV (
“…All MASTER telescopes have identical optical schemes and are equipped with identical sets of polarization and BVRI filters (Kornilov et al 2012;Pruzhinskaya et al 2014;Lipunov et al 2017Lipunov et al , 2019Lipunov et al , 2022, enabling the derivation of a target light curve within one photometric framework (Lipunov et al 2010(Lipunov et al , 2023Troja et al 2017;Kornilov et al 2012;Gorbovskoy et al 2010). White light magnitudes are calculated using the equation W = 0.2B + 0.8R (Lipunov et al 2017).…”
The long gamma-ray burst GRB 191221B has abundant observations in X-ray, optical and radio bands. In the literature, the observed optical light curve of GRB 191221B displays a plateau around 0.1-day, which is rather peculiar in gamma-ray bursts.Here we performed detailed analysis of the observational data from Swift/UVOT, VLT and LCO, obtained the light curve of the multi-band afterglow of GRB 191221B. By examining optical, ultraviolet, X-ray, and radio data for this event, we demonstrate that an on-axis two-component jet model can explain the observations. Our analysis suggests that the narrow component has an initial Lorentz factor of 400 and a jet opening half-angle of 1.4 • , while the wide component has an initial Lorentz factor of 25 and a jet opening half-angle of 2.8 • . The narrow jet dominates the early decay, whereas the wider jet causes the optical plateau and dominates late decay. According to this model, the reason for the absence of the X-ray plateau is due to the steeper spectral index of the wide component, resulting in a less significant flux contribution from the wide jet in the X-ray bands than in the optical bands. Moreover, we have explained the inconsistency in the decay indices of the UVOT and Rc-band data around 2000 seconds using reverse shock emission.
The long gamma-ray burst GRB 191221B has abundant observations in X-ray, optical and radio bands. In the literature, the observed optical light curve of GRB 191221B displays a plateau around 0.1-day, which is rather peculiar in gamma-ray bursts. Here we performed detailed analysis of the observational data from Swift/UVOT, VLT and LCO, obtained the light curve of the multi-band afterglow of GRB 191221B. By examining optical, ultraviolet, X-ray, and radio data for this event, we demonstrate that an on-axis two-component jet model can explain the observations. Our analysis suggests that the narrow component has an initial Lorentz factor of 400 and a jet opening half-angle of 1.4○, while the wide component has an initial Lorentz factor of 25 and a jet opening half-angle of 2.8○. The narrow jet dominates the early decay, whereas the wider jet causes the optical plateau and dominates late decay. According to this model, the reason for the absence of the X-ray plateau is due to the steeper spectral index of the wide component, resulting in a less significant flux contribution from the wide jet in the X-ray bands than in the optical bands. Moreover, we have explained the inconsistency in the decay indices of the UVOT and Rc-band data around 2000 seconds using reverse shock emission.
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