financial supports from the Science Foundation of Department of Education of Yunnan Province (2024J0935)。
A possible quasi-periodic oscillation(QPO) at frequency 7.045 × 10^(-5) Hz is found in the narrow-line Seyfert 1galaxy Mrk 142 in the data of XMM-Newton collected on 2020 April 11.We find that the QPO signal is stati...
financial support from ISRO(Sanction Order:No.DS_2B-13013(2)/11/2020-Section2);funded by the National Aeronautics and Space Administration。
We present the results from a long term X-ray analysis of Mrk 279 during the period 2018–2020.We use data from multiple missions–AstroSat,NuSTAR and XMM-Newton,for the purpose.The X-ray spectrum can be modeled as a ...
the financial support from the Council of Scientific&Industrial Research (CSIR),Government of India。
We use the recently discovered simple photometric parameter Central Intensity Ratio(CIR)determined for a sample of 57 nearby(z<0.02)Seyfert galaxies to explore the central features of galaxies and their possible conne...
supported from the research project of Qujing Normal University (Grant No. 2105098001/094);supported by the youth of Yunnan Provincial Science and Technology Department (Grant Nos. 202101AU070146 and 2103010006);supported by the National Natural Science Foundation of China (NSFC, Grant Nos.11733001, 11733002 and 11773013);supported by the National Key Research and Development Program of China (Grant No. 2017YFA0402703);financial support from the National Natural Science Foundation of China (NSFC, Grant No. 12103022);the Special Basic Cooperative Research Programs of Yunnan Provincial Undergraduate Universities Association (No.202101BA070001-043)。
We use a large sample of gamma-ray narrow-line Seyfert 1 galaxies(γ-NLS1 s) to study the jet formation mechanisms. We find that the jet power of γ-NLS1 s is lower than the maximum jet power of the Blandford–Payne(B...
supported by the National Key R&D Program of China with No. 2021YFA1600404;the National Natural Science Foundation of China (NSFC, grant Nos. 11991051, Y911080201, 12073068, 11673062, 11703077, 11703078);the CAS “Light of West China” Program, the Yunnan Province Foundation (2019FB004, 202001AT070069);Yunnan Province Youth Top Talent Project (YNWR-QNBJ-2020-116);the science research grants from the China Manned Space Project with NO. CMS-CSST-2021-A06 and CMS-CSST2021-A05。
In order to study the physical properties of the γ-ray emitting narrow-line Seyfert 1(NLS1) galaxy population,photometric and spectral observations of the γ-ray emitting NLS1 PMN J0948+0022 were made with the Lijian...
financial supports from the National Natural Science Foundation of China(Grant Nos.11133006 and 11173054);the National Basic Research Program of China(973 Program 2009CB824800);the Policy Research Program of Chinese Academy of Sciences(KJCX2-YW-T24)。
We review the Seyfert 1.5 Galaxy ESO 362-G18 for exploring the origin of the soft X-ray excess.The Warm Corona and Relativistic Reflection models are two main scenarios to interpret the soft X-ray excess in active gal...
support from the National Key Research and Development Project of China (grant 2020YFE0202100);supported by the National Natural Science Foundation of China (Grants No.11773036 and 12173009);Strategic Pioneer Program on Space Science;Chinese Academy of Sciences,grants XDA15052600 and XDA15016500;supported by the Natural Science Foundation of Guangxi(2020GXNSFDA238018);the Bagui Young Scholars Program;supported by the Open Project Program of the Key Laboratory of Optical Astronomy,NAOC,CAS;supported by the Christopher R.Redlich Fund and the Miller Institute for Basic Research in Science (in which A.V.F.is a Senior Miller Fellow) funded by the National Aeronautics and Space Administration (NASA);partially supported by a generous gift from Google。
Here we report an identification of B3 0749+460 A as a new double-peaked local "changing-look" active galactic nucleus(CL-AGN) in terms of our multi-epoch spectroscopic analysis. By comparing our new spectra taken in ...
funded by the the Fundamental Research Funds for the Universities in Hebei Province (No:JYQ202003)。
By means of the data sets from the Pan-STARRS1 survey, we have systematically examined the relationship between the variability characteristics and the physical parameters of the largest NLS1 galaxy sample up to now.T...
support from the National Natural Science Foundation of China (NSFC,Grant No.U1931203);support from NSFC (Grant Nos.12025303,11890693 and 11421303);the CAS Frontier Science Key Research Program (QYZDJ-SSWSLH006);the K.C.Wong Education Foundation.Z.C.He is supported by NSFC (Grant No.11903031);USTC Research Funds of the Double First-Class Initiative YD 3440002001;supported by NSF grant AST1907290。
X-ray changing-look active galactic nuclei(CL AGNs) are a subpopulation of AGNs,whose lineof-sight column densities increase/decrease within several years.The physical mechanism for the variation of column density is ...
the National Natural Science Foundation of China(Grant Nos.11533003,11851304 and U1731239);Guangxi Science Foundation and special funding for Guangxi distinguished professors(2017AD22006)。
High energy photon radiations of gamma-ray bursts(GRBs)and active galactic nuclei(AGNs)are dominated by their jet radiations.We examine whether the synchrotron radiations of jets in BL Lacs,flat spectrum radio quasars...