activity
20152021
most citedThe effect of the morphological quenching mechanism on star formation activity at 0.5 < z < 1.5 in 3D-HST/CANDELS

10 citations · 14 across the 2 of their papers we have counts for

collaborators

9 papers

astro-ph.GA202110 cited

The effect of the morphological quenching mechanism on star formation activity at 0.5 < z < 1.5 in 3D-HST/CANDELS

Shiying Lu, Guanwen Fang, Yizhou Gu +3

Several mechanisms for the transformation of blue star-forming to red quiescent galaxies have been proposed, and the green valley (GV) galaxies amid them are widely accepted in a t…

astro-ph.HE2021

Faint AGNs Favor Unexpectedly Long Inter-band Time Lags

Ting Li, Mouyuan Sun, Xiaoyu Xu +12

Inconsistent conclusions are obtained from recent active galactic nuclei (AGNs) accretion disk inter-band time-lag measurements. While some works show that the measured time lags a…

astro-ph.GA2020

An Extraordinary Response of Iron Emission to the Central Outburst in a Tidal Disruption Event Candidate

Zhicheng He, Ning Jiang, Tinggui Wang +9

Understanding the origin of \feii\ emission is important because it is crucial to construct the main sequence of Active Galactic Nuclei (AGNs). Despite several decades of observati…

astro-ph.HE2020

Corona-Heated Accretion-disk Reprocessing (CHAR): A Physical Model to Decipher the Melody of AGN UV/optical Twinkling

Mouyuan Sun, Yongquan Xue, W. N. Brandt +7

Active galactic nuclei (AGNs) have long been observed to "twinkle" (i.e., their brightness varies with time) on timescales from days to years in the UV/optical bands. Such AGN UV/o…

astro-ph.GA2019

The mass dependence of structure, star formation rate, and mass assembly mode at 0.5<z< 2.5

Yizhou Gu, Guanwen Fang, Qirong Yuan +5

To investigate the mass dependence of structural transformation and star formation quenching, we construct three galaxy samples using massive () red, green…

astro-ph.HE2018

Evolution of quasar stochastic variability along its main sequence

Mouyuan Sun, Yongquan Xue, Junxian Wang +2

We explore the evolution of the time variability (in the optical -band and on timescales of weeks to years) of SDSS Stripe 82 quasars along the quasar main sequence. A parent sa…