activity
20012026
most citedThe SINS survey of z~2 galaxy kinematics: properties of the giant star forming clumps

667 citations · 712 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Feedback-Free Star Formation in Clusters within a Galaxy Simulated at High Resolution in Cosmic Dawn

Hou-Zun Chen, Zhaozhou Li, Avishai Dekel +3

We perform a cosmological zoom-in simulation of a massive galaxy ( at ) using the GIZMO code. By employing resolution and a $3.4\…

astro-ph.GA2026★ 2 cited

A Bending in the Size-mass Relation of Star-forming Galaxies across at a Critical Stellar Mass of Revealed by JWST

Longyue Chen, Tao Wang, Hanwen Sun +12

We investigate the rest-frame optical size-stellar mass relation of galaxies at using deep JWST/NIRCam and MIRI imaging from the PRIMER survey. We find that star-formin…

astro-ph.GA2025

Connection between galaxy morphology and dark-matter halo structure II: predicting disk structure from dark-matter halo properties

Jinning Liang, Fangzhou Jiang, Houjun Mo +4

We investigate how galactic disk structures connect to the detailed properties of their host dark-matter halos using the TNG50 simulation. From the hydrodynamic and matched dark-ma…

astro-ph.CO2010★ 667 cited

The SINS survey of z~2 galaxy kinematics: properties of the giant star forming clumps

R. Genzel, S. Newman, T. Jones +24

We have studied the properties of giant star forming clumps in five z~2 star-forming disks with deep SINFONI AO spectroscopy at the ESO VLT. The clumps reside in disk regions where…

astro-ph2001★ 2 cited

Nonlinear Peculiar-Velocity Analysis and PCA

A. Dekel, A. Eldar, L. Silberman +1

We allow for nonlinear effects in the likelihood analysis of peculiar velocities, and obtain ~35%-lower values for the cosmological density parameter and for the amplitude of mass-…

astro-ph2001★ 41 cited

Cosmological Density and Power Spectrum from Peculiar Velocities: Nonlinear Corrections and PCA

L. Silberman, A. Dekel, A. Eldar +1

We allow for nonlinear effects in the likelihood analysis of galaxy peculiar velocities, and obtain ~35%-lower values for the cosmological density parameter Om and the amplitude of…