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20162019
most citedDistinguishing Mergers and Disks in High Redshift Observations of Galaxy Kinematics

72 citations · 154 across the 3 of their papers we have counts for

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7 papers · 1 filter

astro-ph.GA201972 cited

Distinguishing Mergers and Disks in High Redshift Observations of Galaxy Kinematics

Raymond C. Simons, Susan A. Kassin, Gregory F. Snyder +9

The majority of massive star-forming galaxies at have velocity gradients suggestive of rotation, in addition to large amounts of disordered motions. In this paper, we demo…

astro-ph.GA2018

Galaxy inclination and the IRX-beta relation: Effects on UV star-formation rate measurements at intermediate to high redshifts

Weichen Wang, Susan A. Kassin, Camilla Pacifici +11

At intermediate and high redshifts, measurements of galaxy star-formation rates are usually based on rest-frame ultraviolet (UV) data. A correction for dust attenuation, A_UV, is n…

astro-ph.GA2018

On the Transition of the Galaxy Quenching Mode at 0.5<z<1 in CANDELS

F. S. Liu, Meng Jia, Hassen M. Yesuf +19

We investigate the galaxy quenching process at intermediate redshift using a sample of galaxies with between redshift 0.5 and 1.0 in all fiv…

astro-ph.GA2018

The Isophotal Structure of Star-forming Galaxies at in CANDELS: Implications for the Evolution of Galaxy Structure

Dongfei Jiang, F. S. Liu, Xianzhong Zheng +15

We have measured the radial profiles of isophotal ellipticity () and disky/boxy parameter A out to radii of about three times the semi-major axes for s…

astro-ph.GA201727 cited

The Origins of UV-optical Color Gradients in Star-forming Galaxies at z ~ 2: Predominant Dust Gradients But Negligible sSFR Gradients

F. S. Liu, Dongfei Jiang, S. M. Faber +13

The rest-frame UV-optical (i.e., ) color is sensitive to both low-level recent star formation (specific star formation rate - sSFR) and dust. In this Letter, we extend our p…

astro-ph.GA201755 cited

UVI colour gradients of 0.4<z<1.4 star-forming main sequence galaxies in CANDELS: dust extinction and star formation profiles

Weichen Wang, S. M. Faber, F. S. Liu +10

This paper uses radial colour profiles to infer the distributions of dust, gas and star formation in z=0.4-1.4 star-forming main sequence galaxies. We start with the standard UVJ-b…