Lupin Chun-Che Lin

Evolution of the major merger galaxy pair fraction at z < 1

We present a study of the largest available sample of near-infrared selected (i.e., stellar mass selected) dynamically close pairs of galaxies at low redshifts (

LEPTON ACCELERATION IN THE VICINITY OF THE EVENT HORIZON: HIGH-ENERGY AND VERY-HIGH-ENERGY EMISSIONS FROM ROTATING BLACK HOLES WITH VARIOUS MASSES

z 90\%

EXPLORING THE INTRABINARY SHOCK FROM THE REDBACK MILLISECOND PULSAR PSR J2129-0429

spectroscopically complete. The depth and large volume of this sample allow us to investigate the low-redshift pair fraction and merger rate of galaxies over a wide range in

A possible 55-d X-ray period of the ultraluminous accreting pulsar M82 X–2

K-

Searches for Millisecond Pulsar Candidates among the Unidentified Fermi Objects

band luminosity. We find the major-merger pair fraction to be flat at

Observing two dark accelerators around the Galactic Centre with Fermi Large Area Telescope

\sim 2\%

Swift Detection of a 65 Day X-Ray Period from the Ultraluminous Pulsar NGC 7793 P13

as a function of

The X-ray properties of the energetic pulsar PSR J1838−0655

K-

Lepton Acceleration in the Vicinity of the Event Horizon: Very High Energy Emissions from Supermassive Black Holes

band luminosity for galaxies in the range

Searching for High-energy, Horizon-scale Emissions from Galactic Black Hole Transients during Quiescence

10^8 - 10^{12} L_{\odot}