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 ...
Supply chain attacks,exemplified by the SUNBURST attack utilizing SolarWinds Orion updates,pose a growing cybersecurity threat to entities worldwide.However,the need for suitable datasets for detecting and anticipatin...
The Orion laser facility at AWE provides multiple beams to target delivering synchronized pulses at both nanosecond and sub-picosecond duration.In the latter,the peak power approaches the petawatt level.This paper pre...
supported by National Key R&D Program of China (Grant 2017YFA0402701);Key Research Program of Frontier Sciences of CAS (Grant QYZDJ-SSW-SLH047);support by the National Natural Science Foundation of China (NSFC,Grant No.1973091);supports by the NSFC (Nos.11503086 and 11503087)。
We identify 225 filaments from an H2 column density map constructed using simultaneous 12CO,13CO and C18O(J=1-0) observations carried out as a part of the Milky Way Imaging Scroll Painting(MWISP) project.We select 46 ...