supported in China by NSFC grant No.12393853;the Department of Science and Technology of Sichuan Province China with grant No.24NSFSC0449;NSFC grant No.U2031205。
With its high duty cycle, wide field of view and high detection sensitivity, Water Chereknov Detector Array as one of sub-arrays of Large High Altitude Air Shower Observatory is a promising facility to monitor transie...
funded by the National Natural Science Foundation of China (NSFC) under Nos. 41074132, 41274193, 41474166, and 41774085;the Special Fund of the Institute of Geophysics, China Earthquake Administration (Grant No. DQJB22X12)。
We studied the latitudinal and solar cycle distribution of extreme(≥X5) solar flares spanning 1976–2018. We found that all such flares were confined within the latitudinal range of [S30, N35]. Nonetheless, the major...
supported by Russian Science Foundation(project No.23-72-01114).
Herein,we have explored the recombination dynamics and defect concentration of a mixed cation mixed halide perovskite Cs_(0.17)FA_(0.83)PbI_(1.8)Br_(1.2)with 1.75 eV bandgap after exposure to a gamma-ray source(2.5 Gy...
supported by the National Key R&D Program of China(2022YFF0711404,2021YFA0718500);International Partnership Program of Chinese Academy of Sciences(grant No.113111KYSB20190020);the National Natural Science Foundation of China(NSFC,Grant No.U1938106);the open subject of the National HEP Data Center(E029S2S1);support from the Strategic Priority Research Program on Space Science,the Chinese Academy of Sciences(grant Nos.XDA15360102,XDA15360300,XDA15052700 and E02212A02S)。
The Gravitational wave burst high-energy Electromagnetic Counterpart All-sky Monitor(GECAM)is a dedicated mission for monitoring high-energy transients.Here we report the design of the GECAM Scientific Ground Segment(...
the Natural Science Foundation Youth Program of Sichuan Province(2023NSFSC1350);the Doctoral Initiation Fund of West China Normal University(22kE040);the Open Fund of Key Laboratory of Astroparticle Physics of Yunnan Province(2022Zibian3);the Sichuan Youth Science and Technology Innovation Research Team(21CXTD0038);the National Natural Science Foundation of China(NSFC,Grant No.12303048)。
We employ an efficient method for identifying γ-ray sources across the entire sky,leveraging advanced algorithms from Fermipy,and cleverly utilizing the Galactic diffuse background emission model to partition the ent...
supported by the National Science Foundation under Grant No.AST-2034437 and a collaboration including Caltech,IPAC;supported by the Basic Research Program of Yunnan Province(No.202201AS070005);the National Natural Science Foundation of China(NSFC,grant No.12273033);the Original Innovation Program of the Chinese Academy of Sciences(E085021002);the support of the science research program for graduate students of Yunnan University(KC-23234629)。
We analyze the optical light curve data,obtained with the Zwicky Transient Facility(ZTF)survey,for 47 γ-ray blazars monitored by the Large Area Telescope onboard the Fermi Gamma-ray Space Telescope(Fermi).These 47sou...
supported by National Key R&D Program of China(grant No.2023YFE0117200);the National Natural Science Foundation of China(NSFC,grant Nos.12133003,12103011);R-Z.Y.is supported by the NSFC under grants 11421303,12041305;Science and Technology Program of Guangxi(grant Nos.AD 21220075 and 2024GXNSFBA010375);the national youth thousand talents program in China。
We revisit the γ-ray emission above 300 Me V towards the massive star-forming region of Orion B by adopting14 yr observations with the Fermi Large Area Telescope and utilizing the updated software tools.The extended ...
supported by the National Natural Science Foundation of China(Nos.12220101003,12273114,U1931204,12103040,12147208 and U2031111);the Project for Young Scientists in Basic Research of Chinese Academy of Sciences(No.YSBR-061);the Program for Innovative Talents and Entrepreneur in Jiangsu。
In this paper,we analyze the spectral energy distributions of 17 powerful(with a spin-down luminosity greater than10~(35)erg s~(-1))young(with an age less than 15,000 yr)pulsar wind nebulae(PWNe)using a simple timein-...
supported by the Basic Research Program of Yunnan Province(No.202201AS070005);the National Natural Science Foundation of China(NSFC,grant No.12273033);the Original Innovation Program of the Chinese Academy of Sciences(E085021002);support of the science research program for graduate students of Yunnan University(KC-23234629)。
We report our identification of three gigaelectronvoltγ-ray sources,4FGL J0502.6+0036,4FGL J1055.9+6507,and 4FGL J1708.2+5519,as Active Galactic Nuclei(AGNs).They are listed in the latest Fermi-Large Area Telescope s...
support from the National Natural Science Foundation of China(NSFC,Grant No.12203034);from the Shanghai Science and Technology Fund under grant No.22YF1431500;from the science research grants from the China Manned Space Project;support from the National Natural Science Foundation of China(NSFC,grant No.12203043);support from the National Natural Science Foundation of China(NSFC,grant No.11933002);support from the National Natural Science Foundation of China(NSFC,grant No.12173026);the National Key Research and Development Program of China(grant No.2022YFC2807303);the Shanghai Science and Technology Fund(grant No.23010503900);the Program for Professor of Special Appointment(Eastern Scholar)at Shanghai Institutions of Higher Learning;the Shuguang Program(23SG39)of the Shanghai Education Development Foundation and Shanghai Municipal Education Commission;support from the National Natural Science Foundation of China(NSFC,grant No.U2031201,and 11733001);the Scientific and Technological Cooperation Projects(20202023)between the People’s Republic of China and the Republic of Bulgaria;the science research grants from the China Manned Space Project with No.CMS-CSST-2021A06;partially supported by the Bulgarian National Science Fund of the Ministry of Education and Science under grants KP-06-H38/4(2019),KP-06-KITAJ/2(2020),and KP-06-H68/4(2022)。
The location ofγ-ray emission of blazars remains a contested topic,inspiring the development of numerous investigative techniques to address this issue.In this work,we analyzed Fermiγ-ray light curves in the GeV and...