Shuang-Nan Zhang

RADIATION MECHANISMS AND PHYSICAL PROPERTIES OF GeV-TeV BL Lac OBJECTS

Broadband spectral energy distributions (SEDs) are complied from literature for 24 TeV BL Lac objects. Two SEDs, which are identified as low and high states with their flux densities at

Active Galactic Nuclei with Double-peaked Narrow Lines: Are They Dual AGNs?

1\ {\rm TeV}

Comparing the Accretion Disk Evolution of Black Hole and Neutron Star X-Ray Binaries from Low to Super-Eddington Luminosity

(

Testing Einstein's weak equivalence principle with gravitational waves

F_{1 TeV}

WAVELENGTH MEASUREMENTS OF K TRANSITIONS OF OXYGEN, NEON, AND MAGNESIUM WITH X-RAY ABSORPTION LINES

), are available for each of 11 objects. We fit the SEDs with the single-zone synchrotron + synchrotron-self-Compton (SSC) model and determine the physical parameters of the jets. The model well represents the SEDs, and the observed relation between two peak frequencies

Radiation Mechanism and Jet Composition of Gamma-Ray Bursts and GeV-TeV-selected Radio-loud Active Galactic Nuclei

\nu_{\rm s}

The hard X-ray shortages prompted by the clock bursts in GS 1826-238

and

Blazar Anti-sequence of Spectral Variation within individual Blazars: Cases for Mrk?501 and 3C?279

\nu_{\rm c}

TYPE-I X-RAY BURSTS REVEAL A FAST CO-EVOLVING BEHAVIOR OF THE CORONA IN AN X-RAY BINARY

also favors the model. It is found that the break of the electron spectrum (

The Chinese-French SVOM Mission: studying the brightest astronomical explosions

\gamma_{\rm b}