Lu Liu

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

27 citations · 27 across the 1 of their papers we have counts for

collaborators

3 papers

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 $\sim 4400$ galaxies with $M_{*} > 1 0^{9} M_{⊙}$ between redshift 0.5 and 1.0 in all fiv…

astro-ph.GA2018

The Isophotal Structure of Star-forming Galaxies at $0.5 < z < 1.8$ 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 ( $ε$ ) and disky/boxy parameter A $_{4}$ out to radii of about three times the semi-major axes for $\sim 4, 600$ s…

astro-ph.GA2017★ 27 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., $N U V - B$ ) color is sensitive to both low-level recent star formation (specific star formation rate - sSFR) and dust. In this Letter, we extend our p…

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

The Isophotal Structure of Star-forming Galaxies at 0.5<z<1.8 in CANDELS: Implications for the Evolution of Galaxy Structure

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

The Isophotal Structure of Star-forming Galaxies at $0.5 < z < 1.8$ in CANDELS: Implications for the Evolution of Galaxy Structure