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We review the ensemble of anticipated gravitational-wave (GW) emission processes in stellar core collapse and postbounce core-collapse supernova evolution. We discuss recent progress in the modeling of these processes and summarize most…

Astrophysics · Physics 2009-11-19 Christian D. Ott

The terrestrial detection of a neutrino burst from the next galactic core-collapse supernova (CCSN) will provide profound insight into stellar astrophysics, as well as fundamental neutrino physics. Using Time-Of-Flight (ToF) effects, a CCSN…

High Energy Astrophysical Phenomena · Physics 2023-11-20 George Parker , Michael Wurm

Core collapse of massive stars leads to different fates for various physical factors, which gives different spectra of the emitted neutrinos. We focus on the supernova relic neutrinos (SRNs) as a probe to investigate the stellar collapse…

High Energy Astrophysical Phenomena · Physics 2022-09-27 Yosuke Ashida , Ken'ichiro Nakazato

We report the discovery of a confirmed supernova (SN) and a supernova-candidate in near-infrared images from the ALTAIR/NIRI adaptive optics system on the Gemini-North Telescope and NICMOS on the Hubble Space Telescope. The Gemini images…

This is the first paper of a series in which we present new measurements of the observed rates of supernovae (SNe) in the local Universe, determined from the Lick Observatory Supernova Search (LOSS). We have obtained 2.3 million…

Solar and Stellar Astrophysics · Physics 2015-05-19 Jesse Leaman , Weidong Li , Ryan Chornock , Alexei V. Filippenko

We report a radio detection of supernova SN 2004ip in the circumnuclear region of the luminous infrared galaxy IRAS 18293-3413, using Very Large Array (VLA) observations at 8.4 GHz on 11 June 2007. SN 2004ip had been previously discovered…

We present a systematic study of mid-infrared (mid-IR) emission from 141 nearby supernovae (SNe) observed with the InfraRed Array Camera (IRAC) on Spitzer.These SNe reside in one of the 190 galaxies within 20 Mpc drawn from the ongoing…

This paper describes the response of the IceCube neutrino telescope located at the geographic South Pole to outbursts of MeV neutrinos from the core collapse of nearby massive stars. IceCube was completed in December 2010 forming a lattice…

High Energy Astrophysical Phenomena · Physics 2017-04-26 IceCube Collaboration , R. Abbasi , Y. Abdou , T. Abu-Zayyad , M. Ackermann , J. Adams , J. A. Aguilar , M. Ahlers , M. M. Allen , D. Altmann , K. Andeen , J. Auffenberg , X. Bai , M. Baker , S. W. Barwick , V. Baum , R. Bay , J. L. Bazo Alba , K. Beattie , J. J. Beatty , S. Bechet , J. K. Becker , K. -H. Becker , M. L. Benabderrahmane , S. BenZvi , J. Berdermann , P. Berghaus , D. Berley , E. Bernardini , D. Bertrand , D. Z. Besson , D. Bindig , M. Bissok , E. Blaufuss , J. Blumenthal , D. J. Boersma , C. Bohm , D. Bose , S. Böser , O. Botner , A. M. Brown , S. Buitink , K. S. Caballero-Mora , M. Carson , D. Chirkin , B. Christy , F. Clevermann , S. Cohen , C. Colnard , D. F. Cowen , A. H. Cruz Silva , M. V. D'Agostino , M. Danninger , J. Daughhetee , J. C. Davis , C. De Clercq , T. Degner , L. Demirörs , F. Descamps , P. Desiati , G. de Vries-Uiterweerd , T. DeYoung , J. C. Diaz-Vélez , M. Dierckxsens , J. Dreyer , J. P. Dumm , M. Dunkman , J. Eisch , R. W. Ellsworth , O. Engdegård , S. Euler , P. A. Evenson , O. Fadiran , A. R. Fazely , A. Fedynitch , J. Feintzeig , T. Feusels , K. Filimonov , C. Finley , T. Fischer-Wasels , B. D. Fox , A. Franckowiak , R. Franke , T. K. Gaisser , J. Gallagher , L. Gerhardt , L. Gladstone , T. Glüsenkamp , A. Goldschmidt , J. A. Goodman , D. Góra , D. Grant , T. Griesel , A. Groß , S. Grullon , M. Gurtner , C. Ha , A. Haj Ismail , A. Hallgren , F. Halzen , K. Han , K. Hanson , D. Heinen , K. Helbing , R. Hellauer , S. Hickford , G. C. Hill , K. D. Hoffman , B. Hoffmann , A. Homeier , K. Hoshina , W. Huelsnitz , J. -P. Hülß , P. O. Hulth , K. Hultqvist , S. Hussain , A. Ishihara , E. Jakobi , J. Jacobsen , G. S. Japaridze , H. Johansson , K. -H. Kampert , A. Kappes , T. Karg , A. Karle , P. Kenny , J. Kiryluk , F. Kislat , S. R. Klein , H. Köhne , G. Kohnen , H. Kolanoski , L. Köpke , S. Kopper , D. J. Koskinen , M. Kowalski , T. Kowarik , M. Krasberg , G. Kroll , N. Kurahashi , T. Kuwabara , M. Labare , K. Laihem , H. Landsman , M. J. Larson , R. Lauer , J. Lünemann , J. Madsen , A. Marotta , R. Maruyama , K. Mase , H. S. Matis , K. Meagher , M. Merck , P. Mészáros , T. Meures , S. Miarecki , E. Middell , N. Milke , J. Miller , T. Montaruli , R. Morse , S. M. Movit , R. Nahnhauer , J. W. Nam , U. Naumann , D. R. Nygren , S. Odrowski , A. Olivas , M. Olivo , A. O'Murchadha , S. Panknin , L. Paul , C. Pérez de los Heros , J. Petrovic , A. Piegsa , D. Pieloth , R. Porrata , J. Posselt , P. B. Price , G. T. Przybylski , K. Rawlins , P. Redl , E. Resconi , W. Rhode , M. Ribordy , A. S. Richard , M. Richman , J. P. Rodrigues , F. Rothmaier , C. Rott , T. Ruhe , D. Rutledge , B. Ruzybayev , D. Ryckbosch , H. -G. Sander , M. Santander , S. Sarkar , K. Schatto , T. Schmidt , A. Schönwald , A. Schukraft , L. Schulte , A. Schultes , O. Schulz , M. Schunck , D. Seckel , B. Semburg , S. H. Seo , Y. Sestayo , S. Seunarine , A. Silvestri , K. Singh , A. Slipak , G. M. Spiczak , C. Spiering , M. Stamatikos , T. Stanev , T. Stezelberger , R. G. Stokstad , A. Stößl , E. A. Strahler , R. Ström , M. Stüer , G. W. Sullivan , Q. Swillens , H. Taavola , I. Taboada , A. Tamburro , A. Tepe , S. Ter-Antonyan , S. Tilav , P. A. Toale , S. Toscano , D. Tosi , N. van Eijndhoven , J. Vandenbroucke , A. Van Overloop , J. van Santen , M. Vehring , M. Voge , C. Walck , T. Waldenmaier , M. Wallraff , M. Walter , Ch. Weaver , C. Wendt , S. Westerhoff , N. Whitehorn , K. Wiebe , C. H. Wiebusch , D. R. Williams , R. Wischnewski , H. Wissing , M. Wolf , T. R. Wood , K. Woschnagg , C. Xu , D. L. Xu , X. W. Xu , J. P. Yanez , G. Yodh , S. Yoshida , P. Zarzhitsky , M. Zoll

Young core-collapse supernovae with dense-wind progenitors may be able to accelerate cosmic-ray hadrons beyond the knee of the cosmic-ray spectrum, and this may result in measurable gamma-ray emission. We searched for gamma-ray emission…

High Energy Astrophysical Phenomena · Physics 2019-06-19 H. E. S. S. Collaboration , : , H. Abdalla , F. Aharonian , F. Ait Benkhali , E. O. Angüner , M. Arakawa , C. Arcaro , C. Armand , H. Ashkar , M. Backes , V. Barbosa Martins , M. Barnard , Y. Becherini , D. Berge , K. Bernlöhr , R. Blackwell , M. Böttcher , C. Boisson , J. Bolmont , S. Bonnefoy , J. Bregeon , M. Breuhaus , F. Brun , P. Brun , M. Bryan , M. Büchele , T. Bulik , T. Bylund , M. Capasso , S. Caroff , A. Carosi , S. Casanova , M. Cerruti , N. Chakraborty , T. Chand , S. Chandra , R. C. G. Chaves , A. Chen , S. Colafrancesco , M. Curylo , I. D. Davids , C. Deil , J. Devin , P. deWilt , L. Dirson , A. Djannati-Ataï , A. Dmytriiev , A. Donath , V. Doroshenko , L. O'C. Drury , J. Dyks , K. Egberts , G. Emery , J. -P. Ernenwein , S. Eschbach , K. Feijen , S. Fegan , A. Fiasson , G. Fontaine , S. Funk , M. Füßling , S. Gabici , Y. A. Gallant , F. Gaté , G. Giavitto , D. Glawion , J. F. Glicenstein , D. Gottschall , M. -H. Grondin , J. Hahn , M. Haupt , G. Heinzelmann , G. Henri , G. Hermann , J. A. Hinton , W. Hofmann , C. Hoischen , T. L. Holch , M. Holler , D. Horns , D. Huber , H. Iwasaki , M. Jamrozy , D. Jankowsky , F. Jankowsky , I. Jung-Richardt , M. A. Kastendieck , K. Katarzynski , M. Katsuragawa , U. Katz , D. Khangulyan , B. Khélifi , J. King , S. Klepser , W. Kluźniak , Nu. Komin , K. Kosack , D. Kostunin , M. Kraus , G. Lamanna , J. Lau , A. Lemière , M. Lemoine-Goumard , J. -P. Lenain , E. Leser , C. Levy , T. Lohse , I. Lypova , J. Mackey , J. Majumdar , D. Malyshev , V. Marandon , A. Marcowith , A. Mares , C. Mariaud , G. Martí-Devesa , R. Marx , G. Maurin , P. J. Meintjes , A. M. W. Mitchell , R. Moderski , M. Mohamed , L. Mohrmann , J. Muller , C. Moore , E. Moulin , T. Murach , S. Nakashima , M. de Naurois , H. Ndiyavala , F. Niederwanger , J. Niemiec , L. Oakes , P. O'Brien , H. Odaka , S. Ohm , E. de Ona Wilhelmi , M. Ostrowski , I. Oya , M. Panter , R. D. Parsons , C. Perennes , P. -O. Petrucci , B. Peyaud , Q. Piel , S. Pita , V. Poireau , A. Priyana Noel , D. A. Prokhorov , H. Prokoph , G. Pühlhofer , M. Punch , A. Quirrenbach , S. Raab , R. Rauth , A. Reimer , O. Reimer , Q. Remy , M. Renaud , F. Rieger , L. Rinchiuso , C. Romoli , G. Rowell , B. Rudak , E. Ruiz-Velasco , V. Sahakian , S. Saito , D. A. Sanchez , A. Santangelo , M. Sasaki , R. Schlickeiser , F. Schüssler , A. Schulz , H. Schutte , U. Schwanke , S. Schwemmer , M. Seglar-Arroyo , M. Senniappan , A. S. Seyffert , N. Shafi , K. Shiningayamwe , R. Simoni , A. Sinha , H. Sol , A. Specovius , M. Spir-Jacob , Ł. Stawarz , R. Steenkamp , C. Stegmann , C. Steppa , T. Takahashi , T. Tavernier , A. M. Taylor , R. Terrier , D. Tiziani , M. Tluczykont , C. Trichard , M. Tsirou , N. Tsuji , R. Tuffs , Y. Uchiyama , D. J. van der Walt , C. van Eldik , C. van Rensburg , B. van Soelen , G. Vasileiadis , J. Veh , C. Venter , P. Vincent , J. Vink , F. Voisin , H. J. Völk , T. Vuillaume , Z. Wadiasingh , S. J. Wagner , R. White , A. Wierzcholska , R. Yang , H. Yoneda , M. Zacharias , R. Zanin , A. A. Zdziarski , A. Zech , A. Ziegler , J. Zorn , N. Żywucka , Nigel Maxted

Core-collapse supernovae produce copious low-energy neutrinos and are also predicted to radiate gravitational waves. These two messengers can give us information regarding the explosion mechanism. The gravitational wave detection from these…

High Energy Astrophysical Phenomena · Physics 2021-11-01 O Halim , C Casentini , M Drago , V Fafone , K Scholberg , C F Vigorito , G Pagliaroli

Paleo-detectors are a proposed experimental technique in which one would search for traces of recoiling nuclei in ancient minerals. Natural minerals on Earth are as old as $\mathcal{O}(1)\,$Gyr and, in many minerals, the damage tracks left…

Core-collapse supernovae (CCSNe) offer extremely valuable insights into the dynamics of galaxies. Neutrino time profiles from CCSNe, in particular, could reveal unique details about collapsing stars and particle behavior in dense…

We model the distance, extinction, and magnitude probability distributions of a successful Galactic core-collapse supernova (ccSN), its shock breakout radiation, and its massive star progenitor. We find, at very high probability (~100%),…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Scott M. Adams , C. S. Kochanek , John F. Beacom , Mark R. Vagins , K. Z. Stanek

The neutrino burst from a core-collapse supernova can provide information about the star explosion mechanism and the mechanisms of proto neutron star cooling but also about the intrinsic properties of the neutrino such as flavor…

Instrumentation and Detectors · Physics 2016-05-10 Inés Gil-Botella

The progenitors of core-collapse supernovae are stars with an initial mass greater than about 8M(sun). Understanding the evolution of these stars is necessary to comprehend the evolution and differences between supernovae. We have…

Astrophysics · Physics 2007-05-23 John J. Eldridge

A statistically significant detection of the diffuse supernova neutrino background (DSNB) is around the corner. To this purpose, we assess the contribution to the DSNB of magnetorotational collapses of massive stars, relying on a suite of…

High Energy Astrophysical Phenomena · Physics 2024-11-01 Pablo Martínez-Miravé , Irene Tamborra , Miguel Ángel Aloy , Martin Obergaulinger

Identifying the massive progenitor stars that give rise to core-collapse supernovae is one of the main pursuits of supernova and stellar evolution studies. In this talk I discuss some aspects of the pursuit of these progenitor stars in…

Astrophysics · Physics 2007-05-23 Schuyler D. Van Dyk

The explosion of core-collapse supernova depends on a sequence of events taking place in less than a second in a region of a few hundred kilometers at the center of a supergiant star, after the stellar core approaches the Chandrasekhar mass…

The core-collapse supernova (CCSN) is considered one of the most energetic astrophysical events in the universe. The early and prompt detection of neutrinos before (pre-SN) and during the supernova (SN) burst presents a unique opportunity…

High Energy Physics - Experiment · Physics 2023-12-05 Angel Abusleme , Thomas Adam , Shakeel Ahmad , Rizwan Ahmed , Sebastiano Aiello , Muhammad Akram , Abid Aleem , Fengpeng An , Qi An , Giuseppe Andronico , Nikolay Anfimov , Vito Antonelli , Tatiana Antoshkina , Burin Asavapibhop , João Pedro Athayde Marcondes de André , Didier Auguste , Weidong Bai , Nikita Balashov , Wander Baldini , Andrea Barresi , Davide Basilico , Eric Baussan , Marco Bellato , Marco Beretta , Antonio Bergnoli , Daniel Bick , Lukas Bieger , Svetlana Biktemerova , Thilo Birkenfeld , Iwan Morton-Blake , David Blum , Simon Blyth , Anastasia Bolshakova , Mathieu Bongrand , Clément Bordereau , Dominique Breton , Augusto Brigatti , Riccardo Brugnera , Riccardo Bruno , Antonio Budano , Jose Busto , Anatael Cabrera , Barbara Caccianiga , Hao Cai , Xiao Cai , Yanke Cai , Zhiyan Cai , Stéphane Callier , Antonio Cammi , Agustin Campeny , Chuanya Cao , Guofu Cao , Jun Cao , Rossella Caruso , Cédric Cerna , Vanessa Cerrone , Chi Chan , Jinfan Chang , Yun Chang , Auttakit Chatrabhuti , Chao Chen , Guoming Chen , Pingping Chen , Shaomin Chen , Yixue Chen , Yu Chen , Zhangming Chen , Zhiyuan Chen , Zikang Chen , Jie Cheng , Yaping Cheng , Yu Chin Cheng , Alexander Chepurnov , Alexey Chetverikov , Davide Chiesa , Pietro Chimenti , Yen-Ting Chin , Ziliang Chu , Artem Chukanov , Gérard Claverie , Catia Clementi , Barbara Clerbaux , Marta Colomer Molla , Selma Conforti Di Lorenzo , Alberto Coppi , Daniele Corti , Simon Csakli , Flavio Dal Corso , Olivia Dalager , Jaydeep Datta , Christophe De La Taille , Zhi Deng , Ziyan Deng , Xiaoyu Ding , Xuefeng Ding , Yayun Ding , Bayu Dirgantara , Carsten Dittrich , Sergey Dmitrievsky , Tadeas Dohnal , Dmitry Dolzhikov , Georgy Donchenko , Jianmeng Dong , Evgeny Doroshkevich , Wei Dou , Marcos Dracos , Frédéric Druillole , Ran Du , Shuxian Du , Katherine Dugas , Stefano Dusini , Hongyue Duyang , Jessica Eck , Timo Enqvist , Andrea Fabbri , Ulrike Fahrendholz , Lei Fan , Jian Fang , Wenxing Fang , Marco Fargetta , Dmitry Fedoseev , Zhengyong Fei , Li-Cheng Feng , Qichun Feng , Federico Ferraro , Amélie Fournier , Haonan Gan , Feng Gao , Alberto Garfagnini , Arsenii Gavrikov , Marco Giammarchi , Nunzio Giudice , Maxim Gonchar , Guanghua Gong , Hui Gong , Yuri Gornushkin , Alexandre Göttel , Marco Grassi , Maxim Gromov , Vasily Gromov , Minghao Gu , Xiaofei Gu , Yu Gu , Mengyun Guan , Yuduo Guan , Nunzio Guardone , Cong Guo , Wanlei Guo , Xinheng Guo , Caren Hagner , Ran Han , Yang Han , Miao He , Wei He , Tobias Heinz , Patrick Hellmuth , Yuekun Heng , Rafael Herrera , YuenKeung Hor , Shaojing Hou , Yee Hsiung , Bei-Zhen Hu , Hang Hu , Jianrun Hu , Jun Hu , Shouyang Hu , Tao Hu , Yuxiang Hu , Zhuojun Hu , Guihong Huang , Hanxiong Huang , Jinhao Huang , Junting Huang , Kaixuan Huang , Wenhao Huang , Xin Huang , Xingtao Huang , Yongbo Huang , Jiaqi Hui , Lei Huo , Wenju Huo , Cédric Huss , Safeer Hussain , Leonard Imbert , Ara Ioannisian , Roberto Isocrate , Arshak Jafar , Beatrice Jelmini , Ignacio Jeria , Xiaolu Ji , Huihui Jia , Junji Jia , Siyu Jian , Cailian Jiang , Di Jiang , Wei Jiang , Xiaoshan Jiang , Xiaoping Jing , Cécile Jollet , Philipp Kampmann , Li Kang , Rebin Karaparambil , Narine Kazarian , Ali Khan , Amina Khatun , Khanchai Khosonthongkee , Denis Korablev , Konstantin Kouzakov , Alexey Krasnoperov , Sergey Kuleshov , Nikolay Kutovskiy , Loïc Labit , Tobias Lachenmaier , Cecilia Landini , Sébastien Leblanc , Victor Lebrin , Frederic Lefevre , Ruiting Lei , Rupert Leitner , Jason Leung , Demin Li , Fei Li , Fule Li , Gaosong Li , Huiling Li , Jiajun Li , Mengzhao Li , Min Li , Nan Li , Qingjiang Li , Ruhui Li , Rui Li , Shanfeng Li , Tao Li , Teng Li , Weidong Li , Weiguo Li , Xiaomei Li , Xiaonan Li , Xinglong Li , Yi Li , Yichen Li , Yufeng Li , Zhaohan Li , Zhibing Li , Ziyuan Li , Zonghai Li , Hao Liang , Hao Liang , Jiajun Liao , Ayut Limphirat , Guey-Lin Lin , Shengxin Lin , Tao Lin , Jiajie Ling , Xin Ling , Ivano Lippi , Caimei Liu , Fang Liu , Fengcheng Liu , Haidong Liu , Haotian Liu , Hongbang Liu , Hongjuan Liu , Hongtao Liu , Hui Liu , Jianglai Liu , Jiaxi Liu , Jinchang Liu , Min Liu , Qian Liu , Qin Liu , Runxuan Liu , Shenghui Liu , Shubin Liu , Shulin Liu , Xiaowei Liu , Xiwen Liu , Xuewei Liu , Yankai Liu , Zhen Liu , Alexey Lokhov , Paolo Lombardi , Claudio Lombardo , Kai Loo , Chuan Lu , Haoqi Lu , Jingbin Lu , Junguang Lu , Peizhi Lu , Shuxiang Lu , Xianguo Lu , Bayarto Lubsandorzhiev , Sultim Lubsandorzhiev , Livia Ludhova , Arslan Lukanov , Daibin Luo , Fengjiao Luo , Guang Luo , Jianyi Luo , Shu Luo , Wuming Luo , Xiaojie Luo , Vladimir Lyashuk , Bangzheng Ma , Bing Ma , Qiumei Ma , Si Ma , Xiaoyan Ma , Xubo Ma , Jihane Maalmi , Marco Magoni , Jingyu Mai , Yury Malyshkin , Roberto Carlos Mandujano , Fabio Mantovani , Xin Mao , Yajun Mao , Stefano M. Mari , Filippo Marini , Agnese Martini , Matthias Mayer , Davit Mayilyan , Ints Mednieks , Yue Meng , Anita Meraviglia , Anselmo Meregaglia , Emanuela Meroni , David Meyhöfer , Lino Miramonti , Nikhil Mohan , Michele Montuschi , Axel Müller , Massimiliano Nastasi , Dmitry V. Naumov , Elena Naumova , Diana Navas-Nicolas , Igor Nemchenok , Minh Thuan Nguyen Thi , Alexey Nikolaev , Feipeng Ning , Zhe Ning , Hiroshi Nunokawa , Lothar Oberauer , Juan Pedro Ochoa-Ricoux , Alexander Olshevskiy , Domizia Orestano , Fausto Ortica , Rainer Othegraven , Alessandro Paoloni , Sergio Parmeggiano , Yatian Pei , Luca Pelicci , Anguo Peng , Haiping Peng , Yu Peng , Zhaoyuan Peng , Frédéric Perrot , Pierre-Alexandre Petitjean , Fabrizio Petrucci , Oliver Pilarczyk , Luis Felipe Piñeres Rico , Artyom Popov , Pascal Poussot , Ezio Previtali , Fazhi Qi , Ming Qi , Xiaohui Qi , Sen Qian , Xiaohui Qian , Zhen Qian , Hao Qiao , Zhonghua Qin , Shoukang Qiu , Manhao Qu , Zhenning Qu , Gioacchino Ranucci , Reem Rasheed , Alessandra Re , Abdel Rebii , Mariia Redchuk , Bin Ren , Jie Ren , Barbara Ricci , Komkrit Rientong , Mariam Rifai , Mathieu Roche , Narongkiat Rodphai , Aldo Romani , Bedřich Roskovec , Xichao Ruan , Arseniy Rybnikov , Andrey Sadovsky , Paolo Saggese , Deshan Sandanayake , Anut Sangka , Giuseppe Sava , Utane Sawangwit , Michaela Schever , Cédric Schwab , Konstantin Schweizer , Alexandr Selyunin , Andrea Serafini , Mariangela Settimo , Vladislav Sharov , Arina Shaydurova , Jingyan Shi , Yanan Shi , Vitaly Shutov , Andrey Sidorenkov , Fedor Šimkovic , Apeksha Singhal , Chiara Sirignano , Jaruchit Siripak , Monica Sisti , Mikhail Smirnov , Oleg Smirnov , Thiago Sogo-Bezerra , Sergey Sokolov , Julanan Songwadhana , Boonrucksar Soonthornthum , Albert Sotnikov , Ondřej Šrámek , Warintorn Sreethawong , Achim Stahl , Luca Stanco , Konstantin Stankevich , Hans Steiger , Jochen Steinmann , Tobias Sterr , Matthias Raphael Stock , Virginia Strati , Alexander Studenikin , Aoqi Su , Jun Su , Shifeng Sun , Xilei Sun , Yongjie Sun , Yongzhao Sun , Zhengyang Sun , Narumon Suwonjandee , Michal Szelezniak , Akira Takenaka , Jian Tang , Qiang Tang , Quan Tang , Xiao Tang , Vidhya Thara Hariharan , Eric Theisen , Alexander Tietzsch , Igor Tkachev , Tomas Tmej , Marco Danilo Claudio Torri , Francesco Tortorici , Konstantin Treskov , Andrea Triossi , Riccardo Triozzi , Wladyslaw Trzaska , Yu-Chen Tung , Cristina Tuve , Nikita Ushakov , Vadim Vedin , Carlo Venettacci , Giuseppe Verde , Maxim Vialkov , Benoit Viaud , Cornelius Moritz Vollbrecht , Katharina von Sturm , Vit Vorobel , Dmitriy Voronin , Lucia Votano , Pablo Walker , Caishen Wang , Chung-Hsiang Wang , En Wang , Guoli Wang , Jian Wang , Jun Wang , Li Wang , Lu Wang , Meng Wang , Meng Wang , Ruiguang Wang , Siguang Wang , Wei Wang , Wenshuai Wang , Xi Wang , Xiangyue Wang , Yangfu Wang , Yaoguang Wang , Yi Wang , Yi Wang , Yifang Wang , Yuanqing Wang , Yuyi Wang , Zhe Wang , Zheng Wang , Zhimin Wang , Apimook Watcharangkool , Wei Wei , Wei Wei , Wenlu Wei , Yadong Wei , Yuehuan Wei , Kaile Wen , Liangjian Wen , Jun Weng , Christopher Wiebusch , Rosmarie Wirth , Bjoern Wonsak , Diru Wu , Qun Wu , Yiyang Wu , Zhi Wu , Michael Wurm , Jacques Wurtz , Christian Wysotzki , Yufei Xi , Dongmei Xia , Fei Xiao , Xiang Xiao , Xiaochuan Xie , Yuguang Xie , Zhangquan Xie , Zhao Xin , Zhizhong Xing , Benda Xu , Cheng Xu , Donglian Xu , Fanrong Xu , Hangkun Xu , Jilei Xu , Jing Xu , Meihang Xu , Xunjie Xu , Yin Xu , Yu Xu , Baojun Yan , Qiyu Yan , Taylor Yan , Xiongbo Yan , Yupeng Yan , Changgen Yang , Chengfeng Yang , Jie Yang , Lei Yang , Xiaoyu Yang , Yifan Yang , Yifan Yang , Haifeng Yao , Jiaxuan Ye , Mei Ye , Ziping Ye , Frédéric Yermia , Zhengyun You , Boxiang Yu , Chiye Yu , Chunxu Yu , Guojun Yu , Hongzhao Yu , Miao Yu , Xianghui Yu , Zeyuan Yu , Zezhong Yu , Cenxi Yuan , Chengzhuo Yuan , Ying Yuan , Zhenxiong Yuan , Baobiao Yue , Noman Zafar , Vitalii Zavadskyi , Fanrui Zeng , Shan Zeng , Tingxuan Zeng , Yuda Zeng , Liang Zhan , Aiqiang Zhang , Bin Zhang , Binting Zhang , Feiyang Zhang , Haosen Zhang , Honghao Zhang , Jialiang Zhang , Jiawen Zhang , Jie Zhang , Jingbo Zhang , Jinnan Zhang , Lei ZHANG , Mohan Zhang , Peng Zhang , Ping Zhang , Qingmin Zhang , Shiqi Zhang , Shu Zhang , Shuihan Zhang , Siyuan Zhang , Tao Zhang , Xiaomei Zhang , Xin Zhang , Xuantong Zhang , Yinhong Zhang , Yiyu Zhang , Yongpeng Zhang , Yu Zhang , Yuanyuan Zhang , Yumei Zhang , Zhenyu Zhang , Zhijian Zhang , Jie Zhao , Rong Zhao , Runze Zhao , Shujun Zhao , Dongqin Zheng , Hua Zheng , Yangheng Zheng , Weirong Zhong , Jing Zhou , Li Zhou , Nan Zhou , Shun Zhou , Tong Zhou , Xiang Zhou , Jingsen Zhu , Kangfu Zhu , Kejun Zhu , Zhihang Zhu , Bo Zhuang , Honglin Zhuang , Liang Zong , Jiaheng Zou , Jan Züfle

Massive stars undergo a violent death when the supply of nuclear fuel in their cores is exhausted, resulting in a catastrophic "core-collapse" supernova. Such events are usually only detected at least a few days after the star has exploded.…