Ilsang Yoon

TL;DR: The Very Large Array Sky Survey (VLASS) as discussed by the authors is a synoptic, all-sky radio sky survey with a unique combination of high angular resolution (≈2.5"), sensitivity (a 1σ goal of 70 μJy/beam in the coadded data), full linear Stokes polarimetry, time domain coverage, and wide bandwidth (2-4 GHz).

TL;DR: The science case and observational strategy for the Very Large Array Sky Survey is presented, and also results from early survey observations are presented.

TL;DR: In this article, the authors present detailed submillimeter-through centimeter-wave observations of the extraordinary extragalactic transient AT2018cow, which is not naturally explained by an extension of the radio-submm synchrotron spectrum, nor by inverse Compton scattering of the dominant blackbody UV/optical/IR photons by energetic electrons within the forward shock.

TL;DR: In this article, an automated masking algorithm that operates within CLEAN called AUTO-MULTITHRESH is described. But this approach is not possible with today's large data volumes which require automated imaging pipelines.

TL;DR: In this article, the authors carried out N-body simulations for rotating star clusters with equal mass and compared the results with Fokker-Planck models, and confirmed the acceleration of the core collapse due to an initial non-zero angular momentum and found a similar evolutionary trend in the central density and velocity dispersion.