[{"data":1,"prerenderedAt":-1},["ShallowReactive",2],{"detail-sidebar-cat-1-en-105":3,"doc-seo-194569-105":53,"doc-detail-194569-en":126},{"code":4,"msg":5,"data":6},0,"success",[7,14,19,24,29,34,39,44,49],{"id":8,"doc_module":9,"doc_module_name":10,"category_name":11,"show_sort_weight":12,"slug":13},11,1,"Template","Presentations",90,"presentations",{"id":15,"doc_module":9,"doc_module_name":10,"category_name":16,"show_sort_weight":17,"slug":18},12,"Resumes",80,"resumes",{"id":20,"doc_module":9,"doc_module_name":10,"category_name":21,"show_sort_weight":22,"slug":23},14,"Invoices",70,"invoices",{"id":25,"doc_module":9,"doc_module_name":10,"category_name":26,"show_sort_weight":27,"slug":28},15,"Posters",60,"posters",{"id":30,"doc_module":9,"doc_module_name":10,"category_name":31,"show_sort_weight":32,"slug":33},16,"Social Media",50,"social-media",{"id":35,"doc_module":9,"doc_module_name":10,"category_name":36,"show_sort_weight":37,"slug":38},17,"Forms",40,"forms",{"id":40,"doc_module":9,"doc_module_name":10,"category_name":41,"show_sort_weight":42,"slug":43},18,"Letters",30,"letters",{"id":45,"doc_module":9,"doc_module_name":10,"category_name":46,"show_sort_weight":47,"slug":48},21,"Paper Templates",5,"papers-templates",{"id":50,"doc_module":9,"doc_module_name":10,"category_name":51,"show_sort_weight":4,"slug":52},158,"General","general-158",{"code":4,"msg":54,"data":55},"ok",{"site_id":56,"language":57,"slug":58,"title":59,"keywords":60,"description":61,"schema_data":62,"social_meta":119,"head_meta":121,"extra_data":123,"updated_unix":125},105,"en","characterizing-the-ordinary-broadline-type-ic-sn-2023pel-from-the-energetic-grb-230812b","Characterizing the Ordinary Broadline Type Ic SN 2023pel from the Energetic GRB 230812B","","This document presents a comprehensive analysis of the broadline Type Ic supernova (SN) 2023pel, originating from the energetic GRB 230812B. The study focuses on characterizing the progenitor system and explosion properties of SN 2023pel, a peculiar event observed in the aftermath of a gamma-ray burst (GRB). The research details the photometric and spectroscopic observations, providing insights into the light curve evolution and spectral features of the supernova. Key aspects investigated include the elemental composition, expansion velocity, and energy of the explosion. The analysis aims to elucidate the connection between the GRB and the Type Ic supernova, contributing to our understanding of the diverse mechanisms that drive these powerful cosmic events. Furthermore, the document discusses the implications of these findings for the broader field of astrophysics, particularly in the context of high-energy phenomena and the evolution of massive stars. The study utilizes advanced observational techniques and theoretical modeling to interpret the complex data.",{"@graph":63,"@context":118},[64,80,101],{"@type":65,"itemListElement":66},"BreadcrumbList",[67,71,74,77],{"item":68,"name":69,"@type":70,"position":9},"https://docshare.wps.com","Home","ListItem",{"item":72,"name":10,"@type":70,"position":73},"https://docshare.wps.com/template/",2,{"item":75,"name":51,"@type":70,"position":76},"https://docshare.wps.com/template/general/",3,{"item":78,"name":59,"@type":70,"position":79},"https://docshare.wps.com/template/characterizing-the-ordinary-broadline-type-ic-sn-2023pel-from-the-energetic-grb-230812b/194569/",4,{"url":78,"name":59,"@type":81,"image":82,"author":87,"headline":59,"publisher":90,"fileFormat":93,"inLanguage":57,"description":61,"dateModified":94,"datePublished":95,"encodingFormat":93,"isAccessibleForFree":96,"interactionStatistic":97},"DigitalDocument",{"url":83,"@type":84,"width":85,"height":86},"https://docshare.wps.com/thumbnails/characterizing-the-ordinary-broadline-type-ic-sn-2023pel-from-the-energetic-grb-230812b/194569.png","ImageObject",442,249,{"name":88,"@type":89},"Arica Lee","Person",{"url":68,"name":91,"@type":92},"DocShare","Organization","application/pdf","2026-10-05","2026-09-03",true,{"@type":98,"interactionType":99,"userInteractionCount":47},"InteractionCounter",{"@type":100},"ViewAction",{"@type":102,"mainEntity":103},"FAQPage",[104,110,114],{"name":105,"@type":106,"acceptedAnswer":107},"What is the main subject of this document?","Question",{"text":108,"@type":109},"This document focuses on the characterization of the broadline Type Ic supernova SN 2023pel, which is associated with the energetic GRB 230812B.","Answer",{"name":111,"@type":106,"acceptedAnswer":112},"What types of observations are discussed in the document?",{"text":113,"@type":109},"The document details photometric and spectroscopic observations of SN 2023pel, analyzing its light curve evolution and spectral features.",{"name":115,"@type":106,"acceptedAnswer":116},"What is the primary goal of this research?",{"text":117,"@type":109},"The primary goal is to understand the progenitor system and explosion properties of SN 2023pel, and to explore the relationship between the GRB and the Type Ic supernova.","https://schema.org",{"og:url":78,"og:type":120,"og:title":59,"og:site_name":91,"og:description":61},"article",{"robots":122,"canonical":78},"index,follow",{"doc_id":124,"site_id":56},194569,1790419958,{"code":4,"msg":5,"data":127},{"doc_id":124,"user_id":128,"nickname":88,"user_avatar":129,"doc_module":9,"category_id":50,"category_name":51,"doc_title":59,"doc_description":61,"doc_content":60,"file_id":130,"file_url":131,"file_type":132,"file_size":133,"view_count":47,"is_deleted":4,"is_public":9,"is_downloadable":9,"audit_status":9,"page_count":25,"language":134,"language_code":57,"site_id":56,"html_lang":57,"table_of_contents":60,"faqs":135,"seo_title":136,"seo_description":61,"update_tm":137,"read_time":47},8796096645457,"https://ap-avatar.wpscdn.com/avatar/800003749518d68ffe3?x-image-process=image/resize,m_fixed,w_180,h_180&k=1779345340919836971","cbCaibBza46LyTQe","https://ap.wps.com/l/cbCaibBza46LyTQe","pdf",2952704,"English","[{\"question\":\"What is the main subject of this document?\",\"answer\":\"This document focuses on the characterization of the broadline Type Ic supernova SN 2023pel, which is associated with the energetic GRB 230812B.\"},{\"question\":\"What types of observations are discussed in the document?\",\"answer\":\"The document details photometric and spectroscopic observations of SN 2023pel, analyzing its light curve evolution and spectral features.\"},{\"question\":\"What is the primary goal of this research?\",\"answer\":\"The primary goal is to understand the progenitor system and explosion properties of SN 2023pel, and to explore the relationship between the GRB and the Type Ic supernova.\"}]","Characterizing the Ordinary Broadline Type Ic SN 2023pel from the Energetic GRB 230812B | PDF",1788440339]