An optical-ultraviolet flare with absolute AB magnitude of -39.4 detected in GRB 220101A

Hyperluminous optical-ultraviolet fares have been detected in gamma-ray bursts and the luminosity record was held by naked-eye event GRB 080319B. Such fares are widely attributed to internal shock or external reverse shock radiation. Here, with a new method developed to derive reliable photometry fr...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2024-06
Main Authors: Zhi-Ping Jin, Zhou, Hao, Wang, Yun, Jin-Jun, Geng, Covino, Stefano, Xue-Feng, Wu, Li, Xiang, Yi-Zhong, Fan, Da-Ming, Wei, Jian-Yan, Wei
Format: Article
Language:English
Subjects:
Deceleration
Energetic materials
Flares
Gamma ray bursts
Gamma rays
Red shift
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by
cites
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Zhi-Ping Jin
Zhou, Hao
Wang, Yun
Jin-Jun, Geng
Covino, Stefano
Xue-Feng, Wu
Li, Xiang
Yi-Zhong, Fan
Da-Ming, Wei
Jian-Yan, Wei
description Hyperluminous optical-ultraviolet fares have been detected in gamma-ray bursts and the luminosity record was held by naked-eye event GRB 080319B. Such fares are widely attributed to internal shock or external reverse shock radiation. Here, with a new method developed to derive reliable photometry from saturated sources of Swift/UVOT, we carry out time-resolved analysis of the initial white-band 150s exposure of GRB 220101A, a burst at a redshift of 4.618, and report a rapidly evolving optical-ultraviolet fare with a high absolute AB magnitude of -39.4\(\pm\)0.2. In contrast to GRB 080319B, the temporal behaviour of this new fare does not trace the gamma-ray activity. Instead of either internal shocks or reverse shock, this extremely energetic optical-ultraviolet fare is most likely to originate from the refreshed shocks induced by the late-ejected extremely energetic material catching up with the earlier-launched decelerating outflow. This finding reveals the diverse origins of the extremely energetic optical-ultraviolet fares and demonstrates the necessity of high-time-resolution observations at early times.
doi_str_mv 10.48550/arxiv.2301.02407
format article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2762491316</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2762491316</sourcerecordid><originalsourceid>FETCH-LOGICAL-a526-537e27994eade24439dd23720ebda3cfc10771040252f17d8ac4e423b53c71133</originalsourceid><addsrcrecordid>eNotzUFLwzAUwPEgCI65D-At4Ln15b2kaY_d0CkMBNnB20iTV-2ozWzT6cdX0NP_9vsLcaMg16UxcOfG7-6cI4HKATXYC7FAIpWVGvFKrKbpCABYWDSGFuK1HmQ8pc67Ppv7NLpzF3tOsu3dyPKrS-_SNVPs58SyXssP9zZ0aQ4sYyszqnItAyf2iYPsBrl9WUtEUKDqa3HZun7i1X-XYv9wv988Zrvn7dOm3mXOYJEZsoy2qjS7wKg1VSEgWQRugiPfegXWKtCABltlQ-m8Zo3UGPJWKaKluP1jT2P8nHlKh2Ocx-H3eEBboK4UqYJ-AO6GT5Q</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2762491316</pqid></control><display><type>article</type><title>An optical-ultraviolet flare with absolute AB magnitude of -39.4 detected in GRB 220101A</title><source>Publicly Available Content (ProQuest)</source><creator>Zhi-Ping Jin ; Zhou, Hao ; Wang, Yun ; Jin-Jun, Geng ; Covino, Stefano ; Xue-Feng, Wu ; Li, Xiang ; Yi-Zhong, Fan ; Da-Ming, Wei ; Jian-Yan, Wei</creator><creatorcontrib>Zhi-Ping Jin ; Zhou, Hao ; Wang, Yun ; Jin-Jun, Geng ; Covino, Stefano ; Xue-Feng, Wu ; Li, Xiang ; Yi-Zhong, Fan ; Da-Ming, Wei ; Jian-Yan, Wei</creatorcontrib><description>Hyperluminous optical-ultraviolet fares have been detected in gamma-ray bursts and the luminosity record was held by naked-eye event GRB 080319B. Such fares are widely attributed to internal shock or external reverse shock radiation. Here, with a new method developed to derive reliable photometry from saturated sources of Swift/UVOT, we carry out time-resolved analysis of the initial white-band 150s exposure of GRB 220101A, a burst at a redshift of 4.618, and report a rapidly evolving optical-ultraviolet fare with a high absolute AB magnitude of -39.4\(\pm\)0.2. In contrast to GRB 080319B, the temporal behaviour of this new fare does not trace the gamma-ray activity. Instead of either internal shocks or reverse shock, this extremely energetic optical-ultraviolet fare is most likely to originate from the refreshed shocks induced by the late-ejected extremely energetic material catching up with the earlier-launched decelerating outflow. This finding reveals the diverse origins of the extremely energetic optical-ultraviolet fares and demonstrates the necessity of high-time-resolution observations at early times.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2301.02407</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Deceleration ; Energetic materials ; Flares ; Gamma ray bursts ; Gamma rays ; Red shift</subject><ispartof>arXiv.org, 2024-06</ispartof><rights>2024. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2762491316?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>780,784,25753,27925,37012,44590</link.rule.ids></links><search><creatorcontrib>Zhi-Ping Jin</creatorcontrib><creatorcontrib>Zhou, Hao</creatorcontrib><creatorcontrib>Wang, Yun</creatorcontrib><creatorcontrib>Jin-Jun, Geng</creatorcontrib><creatorcontrib>Covino, Stefano</creatorcontrib><creatorcontrib>Xue-Feng, Wu</creatorcontrib><creatorcontrib>Li, Xiang</creatorcontrib><creatorcontrib>Yi-Zhong, Fan</creatorcontrib><creatorcontrib>Da-Ming, Wei</creatorcontrib><creatorcontrib>Jian-Yan, Wei</creatorcontrib><title>An optical-ultraviolet flare with absolute AB magnitude of -39.4 detected in GRB 220101A</title><title>arXiv.org</title><description>Hyperluminous optical-ultraviolet fares have been detected in gamma-ray bursts and the luminosity record was held by naked-eye event GRB 080319B. Such fares are widely attributed to internal shock or external reverse shock radiation. Here, with a new method developed to derive reliable photometry from saturated sources of Swift/UVOT, we carry out time-resolved analysis of the initial white-band 150s exposure of GRB 220101A, a burst at a redshift of 4.618, and report a rapidly evolving optical-ultraviolet fare with a high absolute AB magnitude of -39.4\(\pm\)0.2. In contrast to GRB 080319B, the temporal behaviour of this new fare does not trace the gamma-ray activity. Instead of either internal shocks or reverse shock, this extremely energetic optical-ultraviolet fare is most likely to originate from the refreshed shocks induced by the late-ejected extremely energetic material catching up with the earlier-launched decelerating outflow. This finding reveals the diverse origins of the extremely energetic optical-ultraviolet fares and demonstrates the necessity of high-time-resolution observations at early times.</description><subject>Deceleration</subject><subject>Energetic materials</subject><subject>Flares</subject><subject>Gamma ray bursts</subject><subject>Gamma rays</subject><subject>Red shift</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNotzUFLwzAUwPEgCI65D-At4Ln15b2kaY_d0CkMBNnB20iTV-2ozWzT6cdX0NP_9vsLcaMg16UxcOfG7-6cI4HKATXYC7FAIpWVGvFKrKbpCABYWDSGFuK1HmQ8pc67Ppv7NLpzF3tOsu3dyPKrS-_SNVPs58SyXssP9zZ0aQ4sYyszqnItAyf2iYPsBrl9WUtEUKDqa3HZun7i1X-XYv9wv988Zrvn7dOm3mXOYJEZsoy2qjS7wKg1VSEgWQRugiPfegXWKtCABltlQ-m8Zo3UGPJWKaKluP1jT2P8nHlKh2Ocx-H3eEBboK4UqYJ-AO6GT5Q</recordid><startdate>20240605</startdate><enddate>20240605</enddate><creator>Zhi-Ping Jin</creator><creator>Zhou, Hao</creator><creator>Wang, Yun</creator><creator>Jin-Jun, Geng</creator><creator>Covino, Stefano</creator><creator>Xue-Feng, Wu</creator><creator>Li, Xiang</creator><creator>Yi-Zhong, Fan</creator><creator>Da-Ming, Wei</creator><creator>Jian-Yan, Wei</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20240605</creationdate><title>An optical-ultraviolet flare with absolute AB magnitude of -39.4 detected in GRB 220101A</title><author>Zhi-Ping Jin ; Zhou, Hao ; Wang, Yun ; Jin-Jun, Geng ; Covino, Stefano ; Xue-Feng, Wu ; Li, Xiang ; Yi-Zhong, Fan ; Da-Ming, Wei ; Jian-Yan, Wei</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a526-537e27994eade24439dd23720ebda3cfc10771040252f17d8ac4e423b53c71133</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Deceleration</topic><topic>Energetic materials</topic><topic>Flares</topic><topic>Gamma ray bursts</topic><topic>Gamma rays</topic><topic>Red shift</topic><toplevel>online_resources</toplevel><creatorcontrib>Zhi-Ping Jin</creatorcontrib><creatorcontrib>Zhou, Hao</creatorcontrib><creatorcontrib>Wang, Yun</creatorcontrib><creatorcontrib>Jin-Jun, Geng</creatorcontrib><creatorcontrib>Covino, Stefano</creatorcontrib><creatorcontrib>Xue-Feng, Wu</creatorcontrib><creatorcontrib>Li, Xiang</creatorcontrib><creatorcontrib>Yi-Zhong, Fan</creatorcontrib><creatorcontrib>Da-Ming, Wei</creatorcontrib><creatorcontrib>Jian-Yan, Wei</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content (ProQuest)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zhi-Ping Jin</au><au>Zhou, Hao</au><au>Wang, Yun</au><au>Jin-Jun, Geng</au><au>Covino, Stefano</au><au>Xue-Feng, Wu</au><au>Li, Xiang</au><au>Yi-Zhong, Fan</au><au>Da-Ming, Wei</au><au>Jian-Yan, Wei</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>An optical-ultraviolet flare with absolute AB magnitude of -39.4 detected in GRB 220101A</atitle><jtitle>arXiv.org</jtitle><date>2024-06-05</date><risdate>2024</risdate><eissn>2331-8422</eissn><abstract>Hyperluminous optical-ultraviolet fares have been detected in gamma-ray bursts and the luminosity record was held by naked-eye event GRB 080319B. Such fares are widely attributed to internal shock or external reverse shock radiation. Here, with a new method developed to derive reliable photometry from saturated sources of Swift/UVOT, we carry out time-resolved analysis of the initial white-band 150s exposure of GRB 220101A, a burst at a redshift of 4.618, and report a rapidly evolving optical-ultraviolet fare with a high absolute AB magnitude of -39.4\(\pm\)0.2. In contrast to GRB 080319B, the temporal behaviour of this new fare does not trace the gamma-ray activity. Instead of either internal shocks or reverse shock, this extremely energetic optical-ultraviolet fare is most likely to originate from the refreshed shocks induced by the late-ejected extremely energetic material catching up with the earlier-launched decelerating outflow. This finding reveals the diverse origins of the extremely energetic optical-ultraviolet fares and demonstrates the necessity of high-time-resolution observations at early times.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2301.02407</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2024-06
issn 2331-8422
language eng
recordid cdi_proquest_journals_2762491316
source Publicly Available Content (ProQuest)
subjects Deceleration
Energetic materials
Flares
Gamma ray bursts
Gamma rays
Red shift
title An optical-ultraviolet flare with absolute AB magnitude of -39.4 detected in GRB 220101A
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-07T19%3A08%3A40IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=An%20optical-ultraviolet%20flare%20with%20absolute%20AB%20magnitude%20of%20-39.4%20detected%20in%20GRB%20220101A&rft.jtitle=arXiv.org&rft.au=Zhi-Ping%20Jin&rft.date=2024-06-05&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.2301.02407&rft_dat=%3Cproquest%3E2762491316%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a526-537e27994eade24439dd23720ebda3cfc10771040252f17d8ac4e423b53c71133%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2762491316&rft_id=info:pmid/&rfr_iscdi=true