Literature DB >> 32004015

Multiple Galactic Sources with Emission Above 56 TeV Detected by HAWC.

A U Abeysekara1, A Albert2, R Alfaro3, J R Angeles Camacho3, J C Arteaga-Velázquez4, K P Arunbabu5, D Avila Rojas3, H A Ayala Solares6, V Baghmanyan7, E Belmont-Moreno3, S Y BenZvi8, C Brisbois9, K S Caballero-Mora10, T Capistrán11, A Carramiñana11, S Casanova7, U Cotti4, J Cotzomi12, S Coutiño de León11, E De la Fuente13,14, C de León4, S Dichiara15, B L Dingus2, M A DuVernois16, J C Díaz-Vélez13,14, R W Ellsworth9, K Engel9, C Espinoza3, H Fleischhack17, N Fraija15, A Galván-Gámez15, D Garcia3, J A García-González3, F Garfias15, M M González15, J A Goodman9, J P Harding2, S Hernandez3, J Hinton18, B Hona17, D Huang17, F Hueyotl-Zahuantitla10, P Hüntemeyer17, A Iriarte15, A Jardin-Blicq18, V Joshi19, S Kaufmann20, D Kieda1, A Lara5, W H Lee15, H León Vargas3, J T Linnemann21, A L Longinotti11, G Luis-Raya20, J Lundeen21, R López-Coto22, K Malone2,6, S S Marinelli21, O Martinez12, I Martinez-Castellanos9, J Martínez-Castro23, H Martínez-Huerta24, J A Matthews25, P Miranda-Romagnoli26, J A Morales-Soto4, E Moreno12, M Mostafá6, A Nayerhoda7, L Nellen27, M Newbold1, M U Nisa21, R Noriega-Papaqui26, A Peisker21, E G Pérez-Pérez20, J Pretz6, Z Ren25, C D Rho8, C Rivière9, D Rosa-González11, M Rosenberg6, E Ruiz-Velasco18, F Salesa Greus7, A Sandoval3, M Schneider9, H Schoorlemmer18, G Sinnis2, A J Smith9, R W Springer1, P Surajbali18, E Tabachnick9, M Tanner6, O Tibolla20, K Tollefson21, I Torres11, R Torres-Escobedo13,14, L Villaseñor12, T Weisgarber16, J Wood28, T Yapici8, H Zhang29, H Zhou2.   

Abstract

We present the first catalog of gamma-ray sources emitting above 56 and 100 TeV with data from the High Altitude Water Cherenkov Observatory, a wide field-of-view observatory capable of detecting gamma rays up to a few hundred TeV. Nine sources are observed above 56 TeV, all of which are likely galactic in origin. Three sources continue emitting past 100 TeV, making this the highest-energy gamma-ray source catalog to date. We report the integral flux of each of these objects. We also report spectra for three highest-energy sources and discuss the possibility that they are PeVatrons.

Entities:  

Year:  2020        PMID: 32004015     DOI: 10.1103/PhysRevLett.124.021102

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN: 0031-9007            Impact factor:   9.161


  2 in total

1.  Ultrahigh-energy photons up to 1.4 petaelectronvolts from 12 γ-ray Galactic sources.

Authors:  Zhen Cao; F A Aharonian; Q An; L X Bai; Y X Bai; Y W Bao; D Bastieri; X J Bi; Y J Bi; H Cai; J T Cai; Zhe Cao; J Chang; J F Chang; X C Chang; B M Chen; J Chen; L Chen; Liang Chen; Long Chen; M J Chen; M L Chen; Q H Chen; S H Chen; S Z Chen; T L Chen; X L Chen; Y Chen; N Cheng; Y D Cheng; S W Cui; X H Cui; Y D Cui; B Z Dai; H L Dai; Z G Dai; D Della Volpe; B D Ettorre Piazzoli; X J Dong; J H Fan; Y Z Fan; Z X Fan; J Fang; K Fang; C F Feng; L Feng; S H Feng; Y L Feng; B Gao; C D Gao; Q Gao; W Gao; M M Ge; L S Geng; G H Gong; Q B Gou; M H Gu; J G Guo; X L Guo; Y Q Guo; Y Y Guo; Y A Han; H H He; H N He; J C He; S L He; X B He; Y He; M Heller; Y K Hor; C Hou; X Hou; H B Hu; S Hu; S C Hu; X J Hu; D H Huang; Q L Huang; W H Huang; X T Huang; Z C Huang; F Ji; X L Ji; H Y Jia; K Jiang; Z J Jiang; C Jin; D Kuleshov; K Levochkin; B B Li; Cong Li; Cheng Li; F Li; H B Li; H C Li; H Y Li; J Li; K Li; W L Li; X Li; Xin Li; X R Li; Y Li; Y Z Li; Zhe Li; Zhuo Li; E W Liang; Y F Liang; S J Lin; B Liu; C Liu; D Liu; H Liu; H D Liu; J Liu; J L Liu; J S Liu; J Y Liu; M Y Liu; R Y Liu; S M Liu; W Liu; Y N Liu; Z X Liu; W J Long; R Lu; H K Lv; B Q Ma; L L Ma; X H Ma; J R Mao; A Masood; W Mitthumsiri; T Montaruli; Y C Nan; B Y Pang; P Pattarakijwanich; Z Y Pei; M Y Qi; D Ruffolo; V Rulev; A Sáiz; L Shao; O Shchegolev; X D Sheng; J R Shi; H C Song; Yu V Stenkin; V Stepanov; Q N Sun; X N Sun; Z B Sun; P H T Tam; Z B Tang; W W Tian; B D Wang; C Wang; H Wang; H G Wang; J C Wang; J S Wang; L P Wang; L Y Wang; R N Wang; W Wang; W Wang; X G Wang; X J Wang; X Y Wang; Y D Wang; Y J Wang; Y P Wang; Zheng Wang; Zhen Wang; Z H Wang; Z X Wang; D M Wei; J J Wei; Y J Wei; T Wen; C Y Wu; H R Wu; S Wu; W X Wu; X F Wu; S Q Xi; J Xia; J J Xia; G M Xiang; G Xiao; H B Xiao; G G Xin; Y L Xin; Y Xing; D L Xu; R X Xu; L Xue; D H Yan; C W Yang; F F Yang; J Y Yang; L L Yang; M J Yang; R Z Yang; S B Yang; Y H Yao; Z G Yao; Y M Ye; L Q Yin; N Yin; X H You; Z Y You; Y H Yu; Q Yuan; H D Zeng; T X Zeng; W Zeng; Z K Zeng; M Zha; X X Zhai; B B Zhang; H M Zhang; H Y Zhang; J L Zhang; J W Zhang; L Zhang; Li Zhang; L X Zhang; P F Zhang; P P Zhang; R Zhang; S R Zhang; S S Zhang; X Zhang; X P Zhang; Yong Zhang; Yi Zhang; Y F Zhang; Y L Zhang; B Zhao; J Zhao; L Zhao; L Z Zhao; S P Zhao; F Zheng; Y Zheng; B Zhou; H Zhou; J N Zhou; P Zhou; R Zhou; X X Zhou; C G Zhu; F R Zhu; H Zhu; K J Zhu; X Zuo
Journal:  Nature       Date:  2021-05-17       Impact factor: 49.962

2.  Hunting the strongest accelerators in our Galaxy.

Authors:  Petra Huentemeyer
Journal:  Nature       Date:  2021-06       Impact factor: 49.962

  2 in total

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