activity
20172023
most citedSystematic KMTNet Planetary Anomaly Search, Paper I: OGLE-2019-BLG-1053Lb, A Buried Terrestrial Planet

61 citations · 343 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2023★ 1 cited

Black-Hole Formation Accompanied by the Supernova Explosion of a 40-M Progenitor Star

Adam Burrows, David Vartanyan, Tianshu Wang

We have simulated the collapse and evolution of the core of a solar-metallicity 40-M star and find that it explodes vigorously by the neutrino mechanism. This despite its…

astro-ph.HE2023★ 1 cited

The Gravitational-Wave Signature of Core-Collapse Supernovae

David Vartanyan, Adam Burrows, Tianshu Wang +2

We calculate the gravitational-wave (GW) signatures of detailed 3D core-collapse supernova simulations spanning a range of massive stars. Most of the simulations are carried out to…

astro-ph.SR2022★ 59 cited

The Essential Character of the Neutrino Mechanism of Core-Collapse Supernova Explosions

Tianshu Wang, David Vartanyan, Adam Burrows +1

Calibrating with detailed 2D core-collapse supernova simulations, we derive a simple core-collapse supernova explosion condition based solely upon the terminal density profiles of…

astro-ph.GA2021

Neutral Gas within 20,000 Schwarzschild radii of Sagittarius A*

Elena M. Murchikova, Tianshu Wang, Brian Mason +1

Murchikova et al 2019 discovered a disk of cool ionized gas within 20,000 Schwarzschild radii of the Milky Way's Galactic Center black hole Sagittarius A*. They further demonstrate…

astro-ph.EP2021★ 61 cited

Systematic KMTNet Planetary Anomaly Search, Paper I: OGLE-2019-BLG-1053Lb, A Buried Terrestrial Planet

Weicheng Zang, Kyu-Ha Hwang, Andrzej Udalski +69

In order to exhume the buried signatures of "missing planetary caustics" in the KMTNet data, we conducted a systematic anomaly search to the residuals from point-source point-lens…

astro-ph.IM2021★ 10 cited

Light Curve Calculations for Triple Microlensing Systems

Renkun Kuang, Shude Mao, Tianshu Wang +2

We present a method to compute the magnification of a finite source star lensed by a triple lens system based on the image boundary (contour integration) method. We describe a new…

astro-ph.HE2020★ 12 cited

A Generalized Kompaneets Formalism for Inelastic Neutrino-Nucleon Scattering in Supernova Simulations

Tianshu Wang, Adam Burrows

Based on the Kompaneets approximation, we develop a robust methodology to calculate spectral redistribution via inelastic neutrino-nucleon scattering in the context of core-collaps…

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.EP2019★ 7 cited

KMT-2016-BLG-1836Lb: A Super-Jovian Planet From A High-Cadence Microlensing Field

Hongjing Yang, Xiangyu Zhang, Kyu-Ha Hwang +24

We report the discovery of a super-Jovian planet in the microlensing event KMT-2016-BLG-1836, which was found by the Korea Microlensing Telescope Network's high-cadence observation…

astro-ph.EP2019★ 34 cited

OGLE-2018-BLG-1011L\lowercase{b,c}: Microlensing Planetary System with Two Giant Planets Orbiting a Low-mass Star

Cheongho Han, David P. Bennett, Andrzej Udalski +70

We report a multiplanetary system found from the analysis of microlensing event OGLE-2018-BLG-1011, for which the light curve exhibits a double-bump anomaly around the peak. We fin…

astro-ph.EP2019★ 17 cited

OGLE-2018-BLG-0532Lb: Cold Neptune With Possible Jovian Sibling

Yoon-Hyun Ryu, Andrzej Udalski, Jennifer C. Yee +34

We report the discovery of the planet OGLE-2018-BLG-0532Lb, with very obvious signatures in the light curve that lead to an estimate of the planet-host mass ratio $q=M_{\rm planet}…

astro-ph.EP2019★ 17 cited

Parallax of OGLE-2018-BLG-0596: A Low-mass-ratio Planet around an M-dwarf

Youn Kil Jung, Andrew Gould, Andrzej Udalski +63

We report the discovery of a microlensing planet OGLE-2018-BLG-0596Lb, with preferred planet-host mass ratio . The planetary signal, which is chara…

astro-ph.SR2019★ 15 cited

Spitzer Microlensing parallax reveals two isolated stars in the Galactic bulge

Weicheng Zang, Yossi Shvartzvald, Tianshu Wang +90

We report the mass and distance measurements of two single-lens events from the 2017 Spitzer microlensing campaign. The ground-based observations yield the detection of finite-sour…

astro-ph.SR2019★ 17 cited

OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing

Shun-Sheng Li, Weicheng Zang, Andrzej Udalski +102

We present the analysis of the event OGLE-2017-BLG-1186 from the 2017 Spitzer microlensing campaign. This is a remarkable microlensing event because its source is photometrically b…

astro-ph.EP2018★ 12 cited

Kmt-2016-blg-1397b: Kmtnet-only discovery of a microlens giant planet

Weicheng Zang, Kyu-Ha Hwang, Hyoun-Woo Kim +20

We report the discovery of a giant planet in the KMT-2016-BLG-1397 microlensing event, which was found by The Korea Microlensing Telescope Network (KMTNet) alone. The time scale of…

astro-ph.EP2018★ 38 cited

KMT-2017-BLG-0165Lb: A Super-Neptune mass planet Orbiting a Sun-like Host Star

Youn Kil Jung, Andrew Gould, Weicheng Zang +22

We report the discovery of a low mass-ratio planet , i.e., 2.5 times higher than the Neptune/Sun ratio. The planetary system was discovered from the analysi…

astro-ph.EP2018★ 10 cited

OGLE-2017-BLG-1130: The First Binary Gravitational Microlens Detected From Spitzer Only

Tianshu Wang, S. Calchi Novati, A. Udalski +36

We analyze the binary gravitational microlensing event OGLE-2017-BLG-1130 (mass ratio q~0.45), the first published case in which the binary anomaly was only detected by the Spitzer…

astro-ph.SR2017★ 9 cited

Ground-based parallax confirmed by Spitzer: binary microlensing event MOA-2015-BLG-020

Tianshu Wang, Wei Zhu, Shude Mao +83

We present the analysis of the binary gravitational microlensing event MOA-2015-BLG-020. The event has a fairly long timescale (about 63 days) and thus the light curve deviates sig…