108 citations · 339 across the 16 of their papers we have counts for
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When Galaxies Refuel: Evolution of the Perturbed Spiral Galaxy NGC1385
Xiaoyu Kang, Eva Sextl, Rolf-Peter Kudritzki +5
The spiral galaxy NGC 1385 is characterized by a vigorous and protracted history of star formation, particularly in its central regions, leading to a current star formation rate th…
Radial Profiles of Binary Fraction in Elliptical Galaxies
Xiejin Li, Fenghui Zhang, Yinghe Zhao +4
The radial profile of binary fraction may vary with environment and is of significant importance for studying the formation mechanisms of binary stars and their dynamical evolution…
A quantification of the effects using different stellar population synthesis models for epoch of reionization
Peiai Liu, Qingbo Ma, Yunkun Han +1
The luminosity and spectral energy distribution (SED) of high- galaxies are sensitive to the stellar population synthesis (SPS) models. In this paper, we study the effects of di…
BayeSED-GALAXIES I. Performance test for simultaneous photometric redshift and stellar population parameter estimation of galaxies in the CSST wide-field multiband imaging survey
Yunkun Han, Lulu Fan, XianZhong Zheng +2
The forthcoming CSST wide-field multiband imaging survey will produce seven-band photometric spectral energy distributions (SEDs) for billions of galaxies. The effective extraction…
A census of optically dark massive galaxies in the early Universe from magnification by lensing galaxy clusters
Xinwen Shu, Lei Yang, Daizhong Liu +10
We present ALMA 870um and JCMT SCUBA2 850um dust continuum observations of a sample of optically dark and strongly lensed galaxies in the cluster fields. The ALMA and SCUBA2 observ…
Alma Reveals A Gas-rich, Maximum-starburst In The Hyperluminous, Dust-obscured Quasar W0533-3401 AT
Lulu Fan, Kirsten K. Knudsen, Yunkun Han +1
We present ALMA observations and multiwavelength spectral energy distribution (SED) analysis in a WISE-selected, hyperluminous dust-obscured quasar W0533-3401 at . We derive…
Bayesian discrimination of the panchromatic spectral energy distribution modelings of galaxies
Yunkun Han, Zhanwen Han, Lulu Fan
Fitting the multi-wavelength spectral energy distributions (SEDs) of galaxies is a widely used technique to extract information about the physical properties of galaxies. However,…
A Comprehensive Bayesian Discrimination of the Simple Stellar Population Model, Star Formation History and Dust Attenuation Law in the Spectral Energy Distribution Modeling of Galaxies
Yunkun Han, Zhanwen Han
When modeling and interpreting the spectral energy distributions (SEDs) of galaxies, the simple stellar population (SSP) model, star formation history (SFH) and dust attenuation la…
A unique distant submillimeter galaxy with an X-ray-obscured radio-luminous active galactic nucleus
X. W. Shu, Y. Q. Xue, D. Z. Liu +10
We present a multiwavelength study of an atypical submillimeter galaxy in the GOODS-North field, with the aim to understand its physical properties of stellar and dust emission, as…
The SCUBA-2 850 follow-up of WISE-selected, luminous dust-obscured quasars
Lulu Fan, Suzy F. Jones, Yunkun Han +1
Hot dust-obscured galaxies (Hot DOGs) are a new population recently discovered in the \wise All-Sky survey. Multiwavelength follow-up observations suggest that they are luminous, d…
The most-luminous heavily-obscured quasars have a high merger fraction: morphological study of WISE-selected hot dust-obscured galaxies
Lulu Fan, Yunkun Han, Guanwen Fang +6
Previous studies have shown that WISE-selected hyperluminous, hot dust-obscured galaxies (Hot DOGs) are powered by highly dust-obscured, possibly Compton-thick AGNs. High obscurati…
BayeSED: A General Approach to Fitting the Spectral Energy Distribution of Galaxies
Yunkun Han, Zhanwen Han
We present a newly developed version of BayeSED, a general Bayesian approach to the spectral energy distribution (SED) fitting of galaxies. The new BayeSED code has been systematic…
Evolution of luminosity function and obscuration of AGN: connecting X-ray and Infrared
Yunkun Han, Benzhong Dai, Bo Wang +2
We present a detailed comparison between the 2-10 keV hard X-ray and infrared (IR) luminosity function (LF) of active galactic nuclei (AGN). The composite X-ray to IR spectral ener…