supported by the National Natural Science Foundation of China(NSFC,11573024,11473025,11421303,11573001and 11822301);the National Basic Research Program of China(the 973 Program 2013CB834905and 2015CB857005);supported by the NSFC(11503022);the Natural Science Foundation of Shanghai(No.15ZR 1444200);supported by the NSFC(11233002);support from the Anhui Provincial NSF(1608085QA06);Young Wanjiang Scholar program;funded by the Strategic Priority Research Program;the Emergence of Cosmological Structures(XDB09000000),National Astronomical Observatories,Chinese Academy of Sciences;the Special Fund for Astronomy from the Ministry of Finance;Funding for SDSS-Ⅲhas been provided by the Alfred P.Sloan Foundation;the Participating Institutions;the National Science Foundation;the U.S.Department of Energy Office of Science。
We report on the discovery of unusual broad absorption lines(BALs)in the bright quasar SDSS J075133.35+134548.3 at z~1,using archival and newly obtained optical and NIR spectroscopic data.The BALs are detected reliabl...
supported by the SOC program (CHINARE 2012-02-03);the National Natural Science Foundation of China (NSFC 11473025, 11033007, 11421303, 11503022 and 11473305);the National Basic Research Program of China (the 973 Program 2013CB834905);Strategic Priority Research Program “The Emergence of Cosmological Structures” (XDB 09030200);provided by the Alfred P. Sloan Foundation, Participating Institutions, National Science Foundation, U.S. Department of Energy, NASA, Japanese Monbukagakusho, Max Planck Society,and Higher Education Funding Council for England
Emission lines from the broad emission line region (BELR) and the narrow emission line region (NELR) of active galactic nuclei (AGNs) have been extensively studied. However, emission lines are rarely detected be...
supported by the National Basic Research Programof China (973 Program,2009CB24900);the Guangxi Natural Science Foundation (0991018Z);the Science and Technology Commission of Shanghai Municipality (06DZ22101);supported by a grant from the Chinese Academy of Sciences;a visitor grant from the The Netherlands Science Foundation;supported by funds from the NSF,NASA,and the University of Michigan
A periodicity analysis of the radio light curves of the blazar NRAO 530 at 14.5, 8.0, and 4.8 GHz is presented employing an improved phase dispersion mini- mization technique. The result, which shows two persistent pe...
supported by the National Natural Science Foundation of China(NSFC; Grant Nos. 10878010, 11003007 and 10633040);the National Basic Research Program(973 program No. 2007CB815405)
We analyze the optical spectrum of type 1 QSO SDSS J1425+3231. This object is interesting since its narrow emission lines, such as [O Ⅲ]λλ4959, 5007, are double-peaked, and the line structure can be modeled well b...
Supported by NSF (10975128);973 Program of China (2007CB815401)
I show the formulation of de Sitter Special Relativity (dS-SR) based on Dirac-Lu-Zou-Guo’s discussions. dS-SR quantum mechanics is formulated, and the dS-SR Dirac equation for hydrogen is suggested. The equation in...
supported by the National Natural Science Foundation of China (Grant Nos. 10821061,10763002,and 10663002);the National Basic Research Program of China (Grant No. 2009CB824800)
We analyze the radio light curve of 3C 273 at 15 GHz from 1963 to 2006 taken from the database of the literature,and find evidence of quasi-periodic activity.Using the wavelet analysis method to analyze these data,our...
Supported by the National Natural Science Foundation of China (Grant Nos. 10821061, 10763002, and 10663002);the National Basic Research Program of China (Grant No. 2007CB815103);the Natural Science Foundation of Yunnan Province (Grant No. 2008CC011)
A wavelet analysis method is introduced to study the possible periods of PKS 1510-089 in radio bands. By compiling the radio light curve of PKS 1510-089 at frequencies of 22 and 37 GHz from 1990 to 2005, and using the...