activity
20142024
most citedSciences with the 2.5-meter Wide Field Survey Telescope (WFST)

117 citations · 390 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2024★ 4 cited

The Host Galaxy Fluxes of Active Galaxy Nuclei Are Generally Overestimated by the Flux Variation Gradient Method

Minxuan Cai, Zhen Wan, Zhenyi Cai +2

In terms of the variable nature of normal active galaxy nuclei (AGN) and luminous quasars, a so-called flux variation gradient (FVG) method has been widely utilized to estimate the…

astro-ph.IM2023★ 117 cited

Sciences with the 2.5-meter Wide Field Survey Telescope (WFST)

WFST Collaboration, Tinggui Wang, Guilin Liu +60

The Wide Field Survey Telescope (WFST) is a dedicated photometric surveying facility being built jointly by the University of Science and Technology of China and the Purple Mountai…

astro-ph.HE2022★ 7 cited

Nucleosynthesis Contribution of Neutrino-dominated Accretion Flows to the Chemical Evolution of Active Galactic Nuclei

Yan-Qing Qi, Tong Liu, Zhen-Yi Cai +1

Recent observations of quasars show high line-flux ratios in their broad emission lines and the ratios appear to be independent of redshift up to , which indicate that…

astro-ph.CO2022★ 4 cited

Interpreting the statistical properties of high-z extragalactic sources detected by the South Pole Telescope survey

Zhen-Yi Cai, Mattia Negrello, Gianfranco De Zotti

The results of the recently published spectroscopically complete survey of dusty star-forming galaxies detected by the South Pole Telescope (SPT) over 2500 deg^2 proved to be chall…

astro-ph.GA2021★ 23 cited

Extreme Variability Quasars in Their Various States. I: The sample selection and composite SDSS spectra

Wenke Ren, Junxian Wang, Zhenyi Cai +1

Extremely variable quasars (EVQs) are a population of sources showing large optical photometric variability revealed by time-domain surveys. The physical origin of such extreme var…

astro-ph.GA2021★ 10 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★ 25 cited

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★ 11 cited

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★ 75 cited

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★ 12 cited

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★ 28 cited

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…

astro-ph.HE2018★ 20 cited

A falling Corona model for the anomalous behavior of the broad emission lines in NGC 5548

Mouyuan Sun, Yongquan Xue, Zhenyi Cai +1

NGC 5548 has been intensively monitored by the AGN Space Telescope and Optical Reverberation Mapping collaboration. Approximately after half of the light curves, the correlation be…

astro-ph.GA2018★ 47 cited

The morphological evolution, AGN fractions, dust content, environments, and downsizing of massive green valley galaxies at 0.5<z<2.5 in 3D-HST/CANDELS

Yizhou Gu, Guanwen Fang, Qirong Yuan +2

To explore the evolutionary connection among red, green, and blue galaxy populations, based on a sample of massive () galaxies at 0.5<z<2.5 in five 3D-HST…

astro-ph.GA2015★ 4 cited

Predictions for surveys with the SPICA Mid-infrared Instrument

M. Bonato, M. Negrello, Z. -Y. Cai +8

We present predictions for number counts and redshift distributions of galaxies detectable in continuum and in emission lines with the Mid-infrared (MIR) Instrument (SMI) proposed…

astro-ph.GA2014★ 3 cited

Radio Observations of Star Forming Galaxies in the SKA era

C. Mancuso, A. Lapi, Z-Y. Cai +4

We have combined determinations of the epoch-dependent star formation rate (SFR) function with relationships between SFR and radio (synchrotron and free-free) emission to work out…