activity
20192022
most citedThe Peculiar Transient AT2018cow: A Possible Origin of A Type Ibn/IIn Supernova

40 citations · 77 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2022

SN 2019va: A Type IIP Supernova with Large Influence of Nickel-56 Decay on the Plateau-phase Light Curve

Xinghan Zhang, Xiaofeng Wang, Hanna Sai +12

We present multi-band photometric and spectroscopic observations of the type II supernova, (SN) 2019va, which shows an unusually flat plateau-phase evolution in its V-band light cu…

astro-ph.HE202140 cited

The Peculiar Transient AT2018cow: A Possible Origin of A Type Ibn/IIn Supernova

Danfeng Xiang, Xiaofeng Wang, Weili Lin +47

We present our photometric and spectroscopic observations on the peculiar transient AT2018cow. The multi-band photometry covers from peak to 70 days and the spectroscopy rang…

astro-ph.IM202036 cited

The Tsinghua University-Ma Huateng Telescopes for Survey: Overview and Performance of the System

Ji-Cheng Zhang, Xiao-Feng Wang, Jun Mo +16

Over the past decade, time-domain astronomy in optical bands has developed rapidly with the operations of some wide-field survey facilities. However, most of these surveys are cond…

astro-ph.HE2020

Optical and spectral observations and hydrodynamic modelling of Type IIb Supernova 2017gpn

Elena A. Balakina, Maria V. Pruzhinskaya, Alexander S. Moskvitin +6

In this work we present the photometric and spectroscopic observations of Type IIb Supernova 2017gpn. This supernova was discovered in the error-box of LIGO/Virgo G299232 gravitati…

cs.LG20201 cited

Demystifying Orthogonal Monte Carlo and Beyond

Han Lin, Haoxian Chen, Tianyi Zhang +2

Orthogonal Monte Carlo (OMC) is a very effective sampling algorithm imposing structural geometric conditions (orthogonality) on samples for variance reduction. Due to its simplicit…

astro-ph.HE2019

SN 2017gmr: An energetic Type II-P supernova with asymmetries

Jennifer E. Andrews, D. J. Sand, S. Valenti +77

We present high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days…