Subo Dong

TL;DR: In this article, the authors presented SN 2016jae, which was classified as a Type Ia supernova from a spectrum obtained soon after the discovery and reached a B-band peak of -17.93 +-0.34 mag, followed by a fast luminosity decline with sBV 0.56 +- 0.06 and inferred Dm15(B) of 1.10 mag.

TL;DR: In this paper, the authors examined the luminosity function of white dwarfs (WDs) in the local complete WD sample and found that the fraction of bright and young WDs is anomalously high among the WDs detected in multiple systems with main sequence (MS) companions compared to that of the single WDs and theoretical expectations.

TL;DR: In this paper, the authors presented the discovery of a planet on a very wide orbit in the microlensing event OGLE-2012-BLG-0838, where the signal of the planet is well separated from the main peak of the event and the projected separation is found to be twice larger than the Einstein ring radius, which roughly corresponds to a projected separation of ~4 AU.

TL;DR: Gamma-ray astronomy explores the most energetic photons in nature to address some of the most pressing puzzles in contemporary astrophysics as mentioned in this paper, and it encompasses a wide range of objects and phenomena: stars, supernovae, novae, neutron stars, stellar-mass black holes, nucleosynthesis, the interstellar medium, cosmic rays and relativistic-particle acceleration.

TL;DR: In this paper, the authors present observations of the extremely luminous but ambiguous nuclear transient (ANT) ASASSN-17jz, spanning roughly 1200 days of the object's evolution.