The X-ray enhancements of radio-loud quasars at high redshift: new results at z=4-7

The Weakness of Soft X-Ray Intensity: Possible Physical Reason for Weak-line Quasars

The X-Ray Emission Reveals the Coronal Activities of Semi-detached Binaries

A Reverberation Mapping Study of a Highly Variable Active Galactic Nucleus 6dFGS gJ022550.0-060145

The X-ray enhancements of radio-loud quasars at high redshift: New results at z = 4-7

The weakness of soft X-ray intensity: possible physical reason for weak line quasars

The X-ray Emission Reveals the Coronal Activities of Semi-detached Binaries

A reverberation mapping study of a highly variable AGN 6dFGS gJ022550.0-060145

The nearest neutron star candidate in a binary revealed by optical time-domain surveys

The Disk Reverberation Mapping of X-Ray Weak Quasars: A Case Study of SDSS J153913.47+395423.4

The disk reverberation mapping of X-ray weak quasars: A case study of SDSS J153913.47+395423.4

H I Absorption in Low-power Radio AGNs Detected by FAST

HI Absorption in Low-power Radio AGNs Detected by FAST

Shedding New Light on Weak Emission-line Quasars in the C iv-H<i>β</i> Parameter Space

Inspiraling streams of enriched gas observed around a massive galaxy 11 billion years ago

Inspiraling streams of enriched gas observed around a massive galaxy 11 billion years ago

Shedding New Light on Weak Emission-Line Quasars in the C iv–Hβ Parameter Space

Bubble in the Whale: Identifying the Optical Counterparts and Extended Nebula for the Ultraluminous X-Ray Sources in NGC 4631

Bubble in the Whale: Identifying the Optical Counterparts and Extended Nebula for the Ultraluminous X-ray Sources in NGC 4631

A long-period pre-ELM system discovered from LAMOST medium-resolution survey

A White Dwarf-Main Sequence Binary Unveiled by Time-Domain Observations from LAMOST and TESS

A dynamically discovered and characterized non-accreting neutron star - M dwarf binary candidate

TCAD study of high breakdown voltage AlGaN/GaN HEMTs with embedded passivation layer

A White Dwarf-Main-sequence Binary Unveiled by Time-domain Observations from LAMOST and TESS

X-ray emission of contact binary variables within 1 kpc

Cylindrical Al Nano-Dimer Induced Polarization in Deep UV Region

A Long-period Pre-ELM System Discovered from the LAMOST Medium-resolution Survey

X-ray emission of contact binary variables within 1 kpc

Connecting Low- and High-redshift Weak Emission-line Quasars via Hubble Space Telescope Spectroscopy of Ly alpha Emission

Connecting Low- and High-Redshift Weak Emission-Line Quasars via HST Spectroscopy of Lyα Emission

Estimating the Spin of the Black Hole Candidate MAXI J1659-152 with the X-Ray Continuum-fitting Method

The Disk Veiling Effect of the Black Hole Low-mass X-Ray Binary A0620-00

High-Efficient Spin Injection in GaN at Room Temperature Through A Van der Waals Tunnelling Barrier

Estimating the spin of the black hole candidate MAXI J1659-152 with the X-ray continuum-fitting method

Optical and ultraviolet monitoring of the black hole X-ray binary MAXI J1820+070/ASASSN-18ey for 18 months

Proof of CMB-driven X-ray brightening of high-z radio galaxies

Modeling Quasar UV/Optical Variability with the Corona-heated Accretion-disk Reprocessing (CHAR) Model

Extended X-ray emission from the z=4.26 radio galaxy 4C 63.20

Phase-dependent Study of Near-infrared Disk Emission Lines in LB-1

On the Fraction of X-Ray-weak Quasars from the Sloan Digital Sky Survey

Extended X-ray emission from the z = 4.26 radio galaxy 4C 63.20

The L-x-L-uv-L-radio relation and corona-disc-jet connection in optically selected radio-loud quasars

The Lx–Luv–Lradio relation and corona-disk-jet connection in optically selected radio-loud quasars

An Extreme X-Ray Variability Event of a Weak-line Quasar

A wide star-black-hole binary system from radial-velocity measurements

Searching for Black Hole Candidates by LAMOST and ASAS-SN

A Method to Search for Black Hole Candidates with Giant Companions by LAMOST

Airy-like beams with parabolic accelerating trajectories in non-paraxial case

Investigating the X-ray enhancements of highly radio-loud quasars at z > 4

Connecting the X-ray properties of weak-line and typical quasars: testing for a geometrically thick accretion disk

Steep Hard-X-Ray Spectra Indicate Extremely High Accretion Rates in Weak Emission-line Quasars