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19932023
most citedThe Formation of Galactic Disks

2.2k citations · 12.8k across the 221 of their papers we have counts for

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Showing 2019Show all

28 papers · 1 filter

astro-ph.GA2019★ 28 cited

SDSS-IV MaNGA: Internal mass distributions and orbital structures of early-type galaxies and their dependence on environment

Yunpeng Jin, Ling Zhu, R. J. Long +3

In our earlier 2019 paper, we evaluated the reliability of Schwarzschild's orbit-superposition dynamical modelling method in estimating the internal mass distribution, intrinsic st…

astro-ph.IM2019★ 26 cited

Spitzer + VLTI-GRAVITY Measure the Lens Mass of a Nearby Microlensing Event

Weicheng Zang, Subo Dong, Andrew Gould +24

We report the lens mass and distance measurements of the nearby microlensing event TCP J05074264+2447555. We measure the microlens parallax vector using Spitzer and gro…

astro-ph.GA2019★ 34 cited

Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile

Yunchong Wang, Mark Vogelsberger, Dandan Xu +8

We study the evolutionary trend of the total density profile of early-type galaxies (ETGs) in IllustrisTNG. To this end, we trace ETGs from to and measure the power-law…

astro-ph.EP2019★ 23 cited

OGLE-2015-BLG-1771Lb: A Microlens Planet Orbiting an Ultracool Dwarf?

Xiangyu Zhang, Weicheng Zang, Andrzej Udalski +31

We report the discovery and the analysis of the short (tE < 5 days) planetary microlensing event, OGLE-2015-BLG-1771. The event was discovered by the Optical Gravitational Lensing…

astro-ph.GA2019★ 17 cited

An accurate analytic mass model for lensing galaxies

Wei Du, Gong-Bo Zhao, Zuhui Fan +3

We develop an analytic mass model for lensing galaxies, based on a broken power-law (BPL) density profile, which is a power-law profile with a mass deficit or surplus in the centra…

astro-ph.EP2019★ 12 cited

ROME/REA: A gravitational microlensing search for exo-planets beyond the snow-line on a global network of robotic telescopes

Yiannis Tsapras, R. A. Street, M. Hundertmark +10

Planet population synthesis models predict an abundance of planets with semi-major axes between 1-10 au, yet they lie at the edge of the detection limits of most planet finding tec…