MASTER Real-Time Multi-Message Observations of High Energy Phenomena

This review considers synchronous and follow-up MASTER Global Robotic Net optical observations of high energy astrophysical phenomena such as fast radio bursts (FRB), gamma-ray bursts (including prompt optical emission polarization discovery), gravitational-wave events, detected by LIGO/VIRGO (inclu...

Full description

Bibliographic Details
Main Authors: Vladimir M. Lipunov, Viktor G. Kornilov, Kirill Zhirkov, Artem Kuznetsov, Evgenii Gorbovskoy, Nikolai M. Budnev, David A. H. Buckley, Rafael Rebolo Lopez, Miquel Serra-Ricart, Carlos Francile, Nataly Tyurina, Oleg Gress, Pavel Balanutsa, Gleb Antipov, Daniil Vlasenko, Vladislav Topolev, Aristarkh Chasovnikov, Sergei I. Svertilov, Ricardo Podesta, Federico Podesta, Ekaterina Minkina, Andrei G. Tlatov, Vladimir V. Yurkov, Alexandre Gabovich, Olga Ershova, Viktor Senik, Dmitrii Kuvshinov
Format: Article
Language:English
Published: MDPI AG 2022-05-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/8/5/271
_version_ 1797494958790279168
author Vladimir M. Lipunov
Viktor G. Kornilov
Kirill Zhirkov
Artem Kuznetsov
Evgenii Gorbovskoy
Nikolai M. Budnev
David A. H. Buckley
Rafael Rebolo Lopez
Miquel Serra-Ricart
Carlos Francile
Nataly Tyurina
Oleg Gress
Pavel Balanutsa
Gleb Antipov
Daniil Vlasenko
Vladislav Topolev
Aristarkh Chasovnikov
Sergei I. Svertilov
Ricardo Podesta
Federico Podesta
Ekaterina Minkina
Andrei G. Tlatov
Vladimir V. Yurkov
Alexandre Gabovich
Olga Ershova
Viktor Senik
Dmitrii Kuvshinov
author_facet Vladimir M. Lipunov
Viktor G. Kornilov
Kirill Zhirkov
Artem Kuznetsov
Evgenii Gorbovskoy
Nikolai M. Budnev
David A. H. Buckley
Rafael Rebolo Lopez
Miquel Serra-Ricart
Carlos Francile
Nataly Tyurina
Oleg Gress
Pavel Balanutsa
Gleb Antipov
Daniil Vlasenko
Vladislav Topolev
Aristarkh Chasovnikov
Sergei I. Svertilov
Ricardo Podesta
Federico Podesta
Ekaterina Minkina
Andrei G. Tlatov
Vladimir V. Yurkov
Alexandre Gabovich
Olga Ershova
Viktor Senik
Dmitrii Kuvshinov
author_sort Vladimir M. Lipunov
collection DOAJ
description This review considers synchronous and follow-up MASTER Global Robotic Net optical observations of high energy astrophysical phenomena such as fast radio bursts (FRB), gamma-ray bursts (including prompt optical emission polarization discovery), gravitational-wave events, detected by LIGO/VIRGO (including GW170817 and independent Kilonova discovery), high energy neutrino sources (including the detection of IC-170922A progenitor) and others. We report on the first large optical monitoring campaign of the closest at that moment radio burster FRB 180916.J0158+65 simultaneously with a radio burst. We obtained synchronous limits on the optical flux of the FRB 180916.J0158+65 and FRB 200428 (soft gamma repeater SGR 1935+2154) (The CHIME/FRB Collaboration, <i>Nature</i> 2020, 587) at 155093 MASTER images with the total exposure time equal to 2,705,058 s, i.e., 31.3 days. It follows from these synchronous limitations that the ratio of the energies released in the optical and radio ranges does not exceed 4 × 10<sup>5</sup>. Our optical monitoring covered a total of 6 weeks. On 28 April 2020, MASTER automatically following up on a Swift alert began to observe the galactic soft gamma repeater SGR 1935+2154 experienced another flare. On the same day, radio telescopes detected a short radio burst FRB 200428 and MASTER-Tavrida telescope determined the best prompt optical limit of FRB/SGR 1935+2154. Our optical limit shows that X-ray and radio emissions are not explained by a single power-law spectrum. In the course of our observations, using special methods, we found a faint extended afterglow in the FRB 180916.J0158+65 direction associated with the extended emission of the host galaxy.
first_indexed 2024-03-10T01:41:43Z
format Article
id doaj.art-c61fe43c0d6b4657b51bcaa4eaade6eb
institution Directory Open Access Journal
issn 2218-1997
language English
last_indexed 2024-03-10T01:41:43Z
publishDate 2022-05-01
publisher MDPI AG
record_format Article
series Universe
spelling doaj.art-c61fe43c0d6b4657b51bcaa4eaade6eb2023-11-23T13:24:13ZengMDPI AGUniverse2218-19972022-05-018527110.3390/universe8050271MASTER Real-Time Multi-Message Observations of High Energy PhenomenaVladimir M. Lipunov0Viktor G. Kornilov1Kirill Zhirkov2Artem Kuznetsov3Evgenii Gorbovskoy4Nikolai M. Budnev5David A. H. Buckley6Rafael Rebolo Lopez7Miquel Serra-Ricart8Carlos Francile9Nataly Tyurina10Oleg Gress11Pavel Balanutsa12Gleb Antipov13Daniil Vlasenko14Vladislav Topolev15Aristarkh Chasovnikov16Sergei I. Svertilov17Ricardo Podesta18Federico Podesta19Ekaterina Minkina20Andrei G. Tlatov21Vladimir V. Yurkov22Alexandre Gabovich23Olga Ershova24Viktor Senik25Dmitrii Kuvshinov26Physics Department, Lomonosov Moscow State University, Leninskie Gory, GSP-1, Moscow 119991, RussiaPhysics Department, Lomonosov Moscow State University, Leninskie Gory, GSP-1, Moscow 119991, RussiaPhysics Department, Lomonosov Moscow State University, Leninskie Gory, GSP-1, Moscow 119991, RussiaSAI, Lomonosov Moscow State University, Universitetsky Pr., 13, Moscow 119234, RussiaSAI, Lomonosov Moscow State University, Universitetsky Pr., 13, Moscow 119234, RussiaApplied Physics Institute, Irkutsk State University, 20 Gagarin Blvd, Irkutsk 664003, RussiaSouth African Astronomical Observatory, P.O. Box 9, Observatory, Cape Town 7935, South AfricaInstituto de Astrofisica de Canarias, Via Lactea, s/n, E38205 La Laguna, SpainInstituto de Astrofisica de Canarias, Via Lactea, s/n, E38205 La Laguna, SpainObservatorio Astronomico Felix Aguilar (OAFA), Avda Benavides 8175, Rivadavia, El Leonsito, San Juan 5400, ArgentinaSAI, Lomonosov Moscow State University, Universitetsky Pr., 13, Moscow 119234, RussiaSAI, Lomonosov Moscow State University, Universitetsky Pr., 13, Moscow 119234, RussiaSAI, Lomonosov Moscow State University, Universitetsky Pr., 13, Moscow 119234, RussiaSAI, Lomonosov Moscow State University, Universitetsky Pr., 13, Moscow 119234, RussiaPhysics Department, Lomonosov Moscow State University, Leninskie Gory, GSP-1, Moscow 119991, RussiaPhysics Department, Lomonosov Moscow State University, Leninskie Gory, GSP-1, Moscow 119991, RussiaPhysics Department, Lomonosov Moscow State University, Leninskie Gory, GSP-1, Moscow 119991, RussiaPhysics Department, Lomonosov Moscow State University, Leninskie Gory, GSP-1, Moscow 119991, RussiaObservatorio Astronomico Felix Aguilar (OAFA), Avda Benavides 8175, Rivadavia, El Leonsito, San Juan 5400, ArgentinaObservatorio Astronomico Felix Aguilar (OAFA), Avda Benavides 8175, Rivadavia, El Leonsito, San Juan 5400, ArgentinaSAI, Lomonosov Moscow State University, Universitetsky Pr., 13, Moscow 119234, RussiaKislovodsk Solar Station of the Pulkovo Observatory, P.O. Box 45, ul. Gagarina 100, Kislovodsk 357700, RussiaDepartment of Physics and Mathematics, Blagoveschensk State Pedagogical University, Lenin Str., 104, Blagoveschensk 675000, RussiaDepartment of Physics and Mathematics, Blagoveschensk State Pedagogical University, Lenin Str., 104, Blagoveschensk 675000, RussiaApplied Physics Institute, Irkutsk State University, 20 Gagarin Blvd, Irkutsk 664003, RussiaSAI, Lomonosov Moscow State University, Universitetsky Pr., 13, Moscow 119234, RussiaPhysics Department, Lomonosov Moscow State University, Leninskie Gory, GSP-1, Moscow 119991, RussiaThis review considers synchronous and follow-up MASTER Global Robotic Net optical observations of high energy astrophysical phenomena such as fast radio bursts (FRB), gamma-ray bursts (including prompt optical emission polarization discovery), gravitational-wave events, detected by LIGO/VIRGO (including GW170817 and independent Kilonova discovery), high energy neutrino sources (including the detection of IC-170922A progenitor) and others. We report on the first large optical monitoring campaign of the closest at that moment radio burster FRB 180916.J0158+65 simultaneously with a radio burst. We obtained synchronous limits on the optical flux of the FRB 180916.J0158+65 and FRB 200428 (soft gamma repeater SGR 1935+2154) (The CHIME/FRB Collaboration, <i>Nature</i> 2020, 587) at 155093 MASTER images with the total exposure time equal to 2,705,058 s, i.e., 31.3 days. It follows from these synchronous limitations that the ratio of the energies released in the optical and radio ranges does not exceed 4 × 10<sup>5</sup>. Our optical monitoring covered a total of 6 weeks. On 28 April 2020, MASTER automatically following up on a Swift alert began to observe the galactic soft gamma repeater SGR 1935+2154 experienced another flare. On the same day, radio telescopes detected a short radio burst FRB 200428 and MASTER-Tavrida telescope determined the best prompt optical limit of FRB/SGR 1935+2154. Our optical limit shows that X-ray and radio emissions are not explained by a single power-law spectrum. In the course of our observations, using special methods, we found a faint extended afterglow in the FRB 180916.J0158+65 direction associated with the extended emission of the host galaxy.https://www.mdpi.com/2218-1997/8/5/271gamma-ray burstsFRBneutrinogravitational wavespromptafterglow emission
spellingShingle Vladimir M. Lipunov
Viktor G. Kornilov
Kirill Zhirkov
Artem Kuznetsov
Evgenii Gorbovskoy
Nikolai M. Budnev
David A. H. Buckley
Rafael Rebolo Lopez
Miquel Serra-Ricart
Carlos Francile
Nataly Tyurina
Oleg Gress
Pavel Balanutsa
Gleb Antipov
Daniil Vlasenko
Vladislav Topolev
Aristarkh Chasovnikov
Sergei I. Svertilov
Ricardo Podesta
Federico Podesta
Ekaterina Minkina
Andrei G. Tlatov
Vladimir V. Yurkov
Alexandre Gabovich
Olga Ershova
Viktor Senik
Dmitrii Kuvshinov
MASTER Real-Time Multi-Message Observations of High Energy Phenomena
Universe
gamma-ray bursts
FRB
neutrino
gravitational waves
prompt
afterglow emission
title MASTER Real-Time Multi-Message Observations of High Energy Phenomena
title_full MASTER Real-Time Multi-Message Observations of High Energy Phenomena
title_fullStr MASTER Real-Time Multi-Message Observations of High Energy Phenomena
title_full_unstemmed MASTER Real-Time Multi-Message Observations of High Energy Phenomena
title_short MASTER Real-Time Multi-Message Observations of High Energy Phenomena
title_sort master real time multi message observations of high energy phenomena
topic gamma-ray bursts
FRB
neutrino
gravitational waves
prompt
afterglow emission
url https://www.mdpi.com/2218-1997/8/5/271
work_keys_str_mv AT vladimirmlipunov masterrealtimemultimessageobservationsofhighenergyphenomena
AT viktorgkornilov masterrealtimemultimessageobservationsofhighenergyphenomena
AT kirillzhirkov masterrealtimemultimessageobservationsofhighenergyphenomena
AT artemkuznetsov masterrealtimemultimessageobservationsofhighenergyphenomena
AT evgeniigorbovskoy masterrealtimemultimessageobservationsofhighenergyphenomena
AT nikolaimbudnev masterrealtimemultimessageobservationsofhighenergyphenomena
AT davidahbuckley masterrealtimemultimessageobservationsofhighenergyphenomena
AT rafaelrebololopez masterrealtimemultimessageobservationsofhighenergyphenomena
AT miquelserraricart masterrealtimemultimessageobservationsofhighenergyphenomena
AT carlosfrancile masterrealtimemultimessageobservationsofhighenergyphenomena
AT natalytyurina masterrealtimemultimessageobservationsofhighenergyphenomena
AT oleggress masterrealtimemultimessageobservationsofhighenergyphenomena
AT pavelbalanutsa masterrealtimemultimessageobservationsofhighenergyphenomena
AT glebantipov masterrealtimemultimessageobservationsofhighenergyphenomena
AT daniilvlasenko masterrealtimemultimessageobservationsofhighenergyphenomena
AT vladislavtopolev masterrealtimemultimessageobservationsofhighenergyphenomena
AT aristarkhchasovnikov masterrealtimemultimessageobservationsofhighenergyphenomena
AT sergeiisvertilov masterrealtimemultimessageobservationsofhighenergyphenomena
AT ricardopodesta masterrealtimemultimessageobservationsofhighenergyphenomena
AT federicopodesta masterrealtimemultimessageobservationsofhighenergyphenomena
AT ekaterinaminkina masterrealtimemultimessageobservationsofhighenergyphenomena
AT andreigtlatov masterrealtimemultimessageobservationsofhighenergyphenomena
AT vladimirvyurkov masterrealtimemultimessageobservationsofhighenergyphenomena
AT alexandregabovich masterrealtimemultimessageobservationsofhighenergyphenomena
AT olgaershova masterrealtimemultimessageobservationsofhighenergyphenomena
AT viktorsenik masterrealtimemultimessageobservationsofhighenergyphenomena
AT dmitriikuvshinov masterrealtimemultimessageobservationsofhighenergyphenomena