supported by the National Natural Science Foundation of China(12033006,12192221,123B2042).
A recently released XMM-Newton note revealed a significant calibration issue between nuclear spectroscopic telescope array(NuSTAR)and XMM-Newton European Photon Imaging Camera(EPIC)and provided an empirical correction...
financial support from the SERB Core Research Grant project,the Government of India;support from the SRF INSPIRE(IF 170314)fellowship program,Government of India。
Marginal short-period contact binaries are important to understand as they pose a different physical scenario than the predicted theoretical model based on the thermal relaxation oscillation mechanism due to their sha...
supported by the National Natural Science Foundation of China through Grant 11873029;the National Key Research and Development Program of China(2016YFA0400803 and 2017YFA0402703)。
The distribution of the mass of white dwarfs(WDs)is one of the fundamental questions in the field of cataclysmic variables(CVs).In this work,we make a systematical investigation on the WD masses in two subclass of CVs...
funded by ESA Member States and NASA;support from the China Scholarship Council (CSC, Grant 2016GXZR89);supported by the Chinese Academy of Sciences (CAS) President’s International Fellowship Initiative (PIFI, Grant 2016VMB073);supported by the National Natural Science Foundation of China (Grant Nos. 11873073, 11473054 and U1531245);by the Science and Technology Commission of Shanghai Municipality (14ZR 1447100)
We present and analyze the variability of three Seyfert galaxies on intra-day timescales. We have analyzed in a uniform manner the 38 longest(> 30 ks) observations made for NGC 4051, MCG-06–30–15 and NGC 4151 by XMM...
supported by the National Basic Research Program of China (Grant No. 2009CB824800);the Chinese Academy of Sciences Key Project (Grant No. KJCX2-YW-T03);the National Natural Science Foundation of China (Grant No. 10773017);the Natural Science Foundation of Xinjiang Uygur Autonomous Region of China (Grant No. 200821164)
We present a new method for the analysis of Abell 1835 observed by XMM-Newton.The method is a combination of the Direct Demodulation technique and deprojection.We eliminate the effects of the point spread function(PSF...
supported by the National Basic Research Program of China (Grant No. 2009CB824800);the National Natural Science Foundation of China (Grant No. 10533050)
We present results of multi-epoch XMM-Newton observations separated by several years of the narrow-line Seyfert 1(NLS1) galaxy,SDSS J160508.87+323921.4.The NLS1 showed X-ray flux variations on timescales of years as w...
Supported by the National Natural Science Foundation of China(grant No. 10533050).
We report on our results of X-ray spectral analysis for a sample of radio-loud quasars covering a wide range of the radio core-dominance parameter, R, from core- dominated to lobe-dominated objects, using data obtaine...
Supported by the National Natural Science Foundation of China.
We revisit the XMM-Newton observation of the galaxy cluster Abell 1650 with a deprojection technique. We find that the radial deprojected spectra of Abell 1650 can be marginally fitted by a single-temperature model. I...
The X ray observatories XMM Newton and Chandra provided a wealth of exciting new results. Chandra delivered X ray images of outstanding detail, reaching subarcsecond spatial resolution for the first time in X ray astr...