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...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , |
---|---|
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 |