supported by the National Key R&D Program of China(No.2022YFF0608303);the National Major Scientific Research Instrument Development Project(No.11927805);the NSFC Young Scientists Fund(No.12005134);the Shanghai-XFEL Beamline Project(SBP)(No.31011505505885920161A2101001);the Shanghai Municipal Science and Technology Major Project(No.2017SHZDZX02);the Open Fund of the Key Laboratory for Particle Astrophysics and Cosmology;Ministry of Education of China。
In the exploration of celestial bodies,such as Mars,the Moon,and asteroids,X-ray fluorescence analysis has emerged as a critical tool for elemental analysis.However,the varying selection rules and excitation sources i...
supported by the National Nature Science Foundation of China(12041305);the National Youth Thousand Talents Program in China,and the Sichuan Science and Technology Department,Institute of High Energy Physics(2023YFSY0014,E25156U1);supported by the Sichuan Province Science Foundation for Distin-guished Young Scholars(2022JDJQ0043);the Sichuan Science and Technology Department(2023YFSY0014);the Xiejialin Foundation of IHEP(E2546IU2);the National Natural Science Foundation of China(12261141691),and the Innovation Project of IHEP(E25451U2)。
The large array of imaging atmospheric Cherenkov telescopes(LACT)is a planned array of 32 Cherenkov telescopes,each featuring 6-m diameter mirrors,to be constructed at the LHAASO site.This study focused on optimizing ...
partially supported by the National Natural Science Foundation of China (NSFC, grant Nos. 12433004, U2031201, and 11733001);Guangdong Major Project of Basic and Applied Basic Research (grant No. 2019B030302001);the science research grants from the China Manned Space Project with No. CMS-CSST-2021-A06;the support for Astrophysics Key Subjects of Guangdong Province and Guangzhou City;The Key Laboratory for Astronomical Observation and Technology of Guangzhou also supports the work。
A Very High-energy(VHE) flare was observed by Major Atmospheric Gamma Imaging Cherenkov Telescopes on MJD 57788. This VHE flare was characterized by increased VHE flux and short timescales. In this study, we used one-...
supported by the National Natural Science Foundation of China(Nos.12105362,12375244,12275356,12135009,U2241281 and 12175310);the Natural Science Foundation of Hunan Province(No.2022JJ20042);the Innovation Foundation for Graduate Students(No.CX20220048)
Isolated multi-MeV γ-rays with attosecond duration,high collimation and beam angular momentum(BAM)may find many interesting applications in nuclear physics,astrophysics,etc.Here,we propose a scheme to generate such ...
Short-lived medical isotopes and their generators are typically produced in nuclear reactors and cyclotrons that require extensive facilities.However,considering the environmental concerns and economic costs of these ...
supported in part by the National Natural Science Foundation of China(NSFC,grant Nos.12233006 and 12163006);the Basic Research Program of Yunnan Province No.202201AT070137;the joint foundation of Department of Science and Technology of Yunnan Province and Yunnan University No.202201BF070001-020;support by the Xingdian Talent Support Plan—Youth Project。
We report a gradual brighteningγ-ray source,4FGL J1718.5+4237,in 0.1-500.0 GeV,which may be associated with a blazar NVSS J171822+423948 with a redshift of~2.7.We analyzed 15.25 yr ofγ-ray data recorded by the Large...
supported by the National Natural Science Foundation of China(grants 12022305,11973050,and 12203022)。
Theγ-ray emitting compact symmetric objects(CSOs)PKS 1718-649,NGC 3894,and TXS 0128+554 are lobedominated in the radio emission.In order to investigate theirγ-ray radiation properties,we analyze the~14yr Fermi/LAT o...
This work was supported by the National Key R&D Program of China(Nos.2022YFF0709503,2022YFB1902700,2017YFC0602101);the Key Research and Development Program of Sichuan province(No.2023YFG0347);the Key Research and Development Program of Sichuan province(No.2020ZDZX0007).
To detect radioactive substances with low activity levels,an anticoincidence detector and a high-purity germanium(HPGe)detector are typically used simultaneously to suppress Compton scattering background,thereby resul...
This work was supported by the Ministry of Science and Technology(No.2020YFE0202001);by the National Natural Science Foundation of China(Nos.11961141004 and 12205160);Tsinghua University Initiative Scientific Research Program.
The energetic bremsstrahlung photons up to 100 MeV produced in heavy ion collisions can be used as a sensitive probe for short-range correlation in atomic nuclei. The energy of the γ-rays can be measured by collectin...
supported in China by the National Key R&D Program of China(2018YFA0404201,2018YFA0404202,2018YFA0404203,and 2018YFA0404204);the National Natural Science Foundation of China(12105294,12022502,12261160362,12205314,U1931201,and U2031105);the Youth Innovation Promotion Association of Chinese Academy of Sciences(2022010);in Thailand by the National Science and Technology Development Agency(NSTDA)and National Research Council of Thailand(NRCT):High-Potential Research Team Grant Program(N42A650868).
We report the detection of aγ-ray bubble spanning at least 100deg2 in ultra-high energy(UHE)up to a few PeV in the direction of the star-forming region Cygnus X,implying the presence super PeVatron(s)accelerating pro...