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How to find us L. (Lingyu) Wang


Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0

Deep learning for galaxy mergers in the galaxy main sequence

Galaxy and mass assembly: Luminosity and stellar mass functions in GAMA groups

Galaxy And Mass Assembly (GAMA): Properties and evolution of red spiral galaxies

Galaxy And Mass Assembly (GAMA): Defining passive galaxy samples and searching for the UV upturn

Galaxy and Mass Assembly (GAMA): A WISE Study of the Activity of Emission-line Systems in G23

Have we seen all the galaxies that comprise the cosmic infrared background at 250 μm ≤ λ ≤ 500 μm?

Mergers trigger active galactic nuclei out to z ˜ 0.6

Towards a consistent framework of comparing galaxy mergers in observations and simulations

A LOFAR-IRAS cross-match study: The far-infrared radio correlation and the 150 MHz luminosity as a star-formation rate tracer

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