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19992024
most citedImproving PARSEC models for very low mass stars

660 citations · 4.6k across the 134 of their papers we have counts for

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Showing 2019Show all

14 papers · 1 filter

astro-ph.GA2019★ 9 cited

The growth of bulges and discs in relatively HI-rich galaxies: indication from HI scaling relations

Xinkai Chen, Jing Wang, Xu Kong +3

We study the relation between the properties of the bulge/disc components and the HI mass fraction of galaxies. We find that at fixed stellar mass, disc colours are correlated with…

astro-ph.GA2019★ 9 cited

A catalog of galaxy clusters identified from SCUSS, SDSS, and unWISE

Jinghua Gao, Hu Zou, Xu Zhou +1

This paper presents the identification of galaxy clusters from the photometric redshift catalog based on three imaging surveys of SCUSS, SDSS, and unWISE. By applying a fast cluste…

astro-ph.GA2019★ 27 cited

The Mass-Metallicity Relation at : Redshift Evolution and Parameter Dependency

Chi Huang, Hu Zou, Xu Kong +11

The spectra of emission-line galaxies (ELGs) from the extended Baryon Oscillation Spectroscopic Survey (eBOSS) of the Sloan Digit Sky Survey (SDSS) are used to study the mass-metal…

astro-ph.GA2019★ 6 cited

The evolution of baryonic mass function of galaxies to z=3

Zhizheng Pan, Yingjie Peng, Xianzhong Zheng +2

We combine the published stellar mass function (SMF) and gas scaling relations to explore the baryonic (stellar plus cold gas) mass function (BMF) of galaxies to redshift . We…

astro-ph.GA2019★ 8 cited

Color dependence of clustering of massive galaxies at 0.52.5: similar spatial distributions between green valley galaxies and AGNs

Xiaozhi Lin, Guanwen Fang, Zhen-Yi Cai +3

We present a measurement of the spatial clustering of rest-frame UV-selected massive galaxies at in the COSMOS/UltraVISTA field. Considering four separate redshi…

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…