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-...
The influence of intergalactic magnetic fields on the strong gravitational lensing of blazar secondary gamma radiation is discussed.Currently,two cases of strong gravitational lensing of blazar gamma-radiation are kno...
funded by the National Natural Science Foundation of China (NSFC) under No.11903028;the support from the “Yunnan Revitalization Talent Support Program” of Yunnan province, China;the University of Michigan Radio Astronomy Observatory, which is supported by the University of Michigan;by a series of grants from the National Science Foundation, most recently AST-0607523;NASA Fermi grants NNX09AU16G, NNX10AP16G, and NNX11AO13G.
We present periodicity search analyses on long-term radio light curves at 4.8,8,and 14.5 GHz of blazar PKS 0607–157 observed by the University of Michigan Radio Astronomical Observatory telescope.The highly variable ...
supported by the fund for the Youth Project of Basic Research Program of Yunnan Province (202001BB050012);the Joint Foundation of Department of Science and Technology of Yunnan Province and Yunnan University (202201BF070001-020);funded by the“Yunnan University Development Plan for World-Class Astronomy Discipline”。
3C 66A is one of our first batches of photometric monitoring objects with the 1 m optical telescope at Yunnan University Astronomical Observatory.In the present work,the observational campaign was performed from 2021 ...
supported by National Natural Science Foundation of China(Grant No.U1931106);Shandong Provincial Natural Science Foundation of China(Grant No.ZR2019YQ03);Project of Shandong Qing Chuang Science and Technology Plan(Grant No.2019KJJ006)。
We analyzed the optical monitoring data in the R band of Te V blazar 1ES 1959+650 from 2002 to 2018,and provided evidence of a quasi-periodic oscillation in this object.The light curve shows a stable and persistent pe...
the National Natural Science Foundation of China(Grant Nos.11873032 and 12173020)。
Based on the long-term light curves collected from the Catalina Sky Survey(CSS)(from 2005 to 2013)and the All-Sky Automated Survey for Supernovae(ASAS-SN)(from 2014 to 2018),optical quasi-periodic oscillations(QPOs)ab...
Supported by the National Key R&D Program of China (2016YFA0400200);the National Natural Science Foundation of China (U1738209,11851303)。
In this study,we explore the axion-like particle(ALP)-photon oscillation effect in the γ-ray spectra of the blazars Markarian 421(Mrk 421) and PG 1553+113,which are measured by the Major Atmospheric Gamma Imaging Che...
the support from National Natural Science Foundation of China (NSFC,Nos.U1831124 and 11273008);the Natural Science Foundation of Anhui Province of China (Grant No.1908085MA28)。
Long-term optical,X-ray and γ-ray data of blazar 3 C 279 have been compiled from Swift-XRT,RXTE-PCA,Fermi-LAT,SMARTS and literature.The source exhibits strong variability on long timescales.From the 1980 s until now,...
This work was supported by the National Key R&D Programme of China(2018YFA0404603);the Chinese Academy of Sciences(114231KYSB20170003);the Hungarian National Research,Development and Innovation Office(2018-2.1.14-T T-CN-2018-00001).The authors acknowledge the use of Astrogeo Center database of brightness distributions,correlated flux densities;images of compact radio sources produced with VLBI.YZ thanks Shu Fengchun,Alexey Melnikov,Jamie McCallum,and Bo Xia for providing the Asia-Oceania VLBI(AOV)data and auxiliary telescope system temperature files.
High-resolution observations of high-redshift(z > 4) radio quasars offer a unique insight into jet kinematics at early cosmological epochs, as well as constraints on cosmological model parameters.Due to the general we...