2001.4-2002.11 - University of Insubria, Milan, Italy - Postdoctoral Researcher
2002.12-2003.5 - Tsinghua University, Center for Astrophysics - Visiting Scholar
1999: Second Prize, Chinese Academy of Sciences Natural Science Award for Multi-wavelength Observations and Theoretical Studies of Active Galactic Nuclei (Ranked 5th)
2007: New Century Excellent Talents Support Plan by the Ministry of Education
Research
Astrophysical Optical Observations High Energy Astrophysics
XMM-Newton Observations of the TeV BL Lacertae Object PKS 2155-304 in 2006: Signature of Inverse Compton X-Ray Emission?, Zhang, Y. H., 2008
Multi-wavelength Observations of the BL Lacertae Object PKS 2155-304 with XMM-Newton, Zhang, Y. H., Bai, J. M., Zhang, S. N., Treves, A., Maraschi, L., Celotti, A., 2006
XMM-Newton View of PKS 2155-304: Hardness Ratio and Cross-Correlation Analysis of EPIC pn Observations, Zhang, Y. H.; Treves, A.; Maraschi, L.; Bai, J. M.; Liu, F. K., 2006
XMM-Newton view of PKS2155-304: characterizing the X-ray variability properties with EPIC pn, Zhang, Y.H., Treves, A., Celotti, A., Qin, Y.P., Bai, J.M., 2005
Phenomenological analogies in TeV blazars and black hole X-ray binaries in low state, Zhang, Y.H., 2005
The effects of periodically gapped time series on cross-correlation lag determinations, Zhang, Y. H., Cagnoni, I., Treves, A., Celotti, A., Maraschi, L., 2004
Cross-spectral analysis of the X-ray variability of Markarian 421, Zhang, Y. H., 2002
Four Years of Monitoring Blazar PKS 2155-304 with BeppoSAX: Probing the Dynamics of the Jet, Zhang, Y. H., Treves, A., Celotti, A., Chiappetti, L., Fossati, G., Ghisellini, G., Maraschi, L., Pian, E., Tagliaferri, G., Tavecchio, F., 2002
A new list of extra-galactic radio jets, Liu, F.K., Zhang, Y.H., 2002
X-ray emission of Markarian 421: new clues from its spectral evolution. II. Spectral analysis and physical constraints, Fossati, G., Celotti, A., Chiaberge, M., Zhang, Y. H., Chiappetti, L., Ghisellini, G., Maraschi, L., Tavecchio, F., Pian, E., Treves, A., 2000
X-ray emission of Markarian 421: new clues from its spectral evolution. I. Temporal analysis, Fossati, G., Celotti, A., Chiaberge, M., Zhang, Y. H., Chiappetti, L., Ghisellini, G., Maraschi, L., Tavecchio, F., Pian, E., Treves, A., 2000
ROSAT/ASCA observations of a serendipitous BL Lac Object PKS 2316-423: the variable high-energy tail of synchrotron radiation, Xue, S.J., Zhang, Y. H., Chen, J.S., 2000
Rapid X-ray variability of the BL Lacertae object PKS 2155-304, Zhang, Y.H., Celotti, A., Treves, A., Chiappetti, L., Ghisellini, G., Maraschi, L., Pian, E., Tagliaferri., G., Tavecchio, F., Urry, C.M., 1999
Spectral evolution of PKS 2155-304 observed with BeppoSAX during an active gamma-ray phase, Chiappetti, L., Maraschi, L., Tavecchio, F., Celotti, A., Fossati, G., Ghisellini, G., Giommi, P., Pian, E., Tagliaferri, G., Treves, A., Urry, C. M., Zhang, Y. H., 1999
The relation between gamma-Ray and near-infrared radiation in gamma-ray--loud blazars, Xie, G., Zhang, Y.H., Fan, J.H., 1997
Correlation between gamma-ray and far-infrared luminosity for EGRET-detected sources, Zhang, Y.H., Xie, G.Z., 1997
Infrared properties of OJ 287, Zhang, Y.H., Xie, G. Z., 1996
CCD photometry and long-term optical variability of PKS 2155-304, Zhang, Y.H., Xie, G. Z., 1996
CCD photometry of 12 BL Lacertae Objects, Xie, G. Z., Zhang, Y. H., Li, K. H., Liu, F. K., Wang, J. C., Wang, X. M, 1996
The optical variability of the Seyfert galaxies NGC 4051 and NGC 1068, Zhang, Y.H., Xie, G.Z., Cao, S.L., Li, K.H., Wang, J.C., Ye, B.X., 1996
Simultaneous multirange observations and detection of rapid variability of BL Lacertae objects, Xie, G.Z., Li, K.H., Zhang, Y.H., Liu, F.K., Fan, J.H., Wang, J.C, 1994
The relation between BL Lacertae objects and OVV quasars, and the unified model of BL Lacertae objects, FR-I and FR-II (G) radio galaxies, Xie, G.Z., Zhang, Y.H., Fan, J.H., Liu, F.K., 1993
Keywords
Active Galactic NucleiOptical VariabilitySimultaneous Multi-Band MonitoringSupernovaeGamma-Ray BurstsSpace-Based TelescopesData AnalysisQuasarsBlazarsX-Ray Emission
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