activity
20182026
most citedImage Subtraction in Fourier Space

58 citations · 126 across the 14 of their papers we have counts for

collaborators

15 papers

astro-ph.HE2026

High-Redshift Type Ia Supernovae Exhibit Enhanced Calcium Abundances

Xingzhuo Chen, Ulisses Braga-Neto, Lifan Wang

Type Ia supernovae (SNe Ia) are major contributors to cosmic chemical enrichment, and their elemental abundances provide a probe of progenitor properties and explosion physics acro…

astro-ph.IM2026

A GPU-Accelerated Transient Detection Pipeline for DECam Time-Domain Surveys

Lei Hu, Tomás Cabrera, Antonella Palmese +8

We present a GPU-accelerated transient detection pipeline developed for time-domain surveys with the Dark Energy Camera (DECam). It enables real-time-capable image processing, inco…

cs.LG2026

Convolution Operator Network for Forward and Inverse Problems (FI-Conv): Application to Plasma Turbulence Simulations

Xingzhuo Chen, Anthony Poole, Ionut-Gabriel Farcas +2

We propose the Convolutional Operator Network for Forward and Inverse Problems (FI-Conv), a framework capable of predicting system evolution and estimating parameters in complex sp…

astro-ph.HE2025

SEDONA-GesaRaT: an AI-Accelerated Radiative Transfer Program for 3-D Supernova Simulations

Xingzhuo Chen, Ulisses Braga-Neto, Lifan Wang +5

We present SEDONA-GesaRaT, a rapid code for supernova radiative transfer simulation developed based on the Monte-Carlo radiative transfer code SEDONA. We use a set of atomic physic…

astro-ph.HE2025★ 10 cited

Kilonova constraints for the LIGO/Virgo/KAGRA neutron star merger candidate S250206dm: GW-MMADS observations

Lei Hu, Tomás Cabrera, Antonella Palmese +35

Gravitational wave (GW) neutron star mergers with an associated electromagnetic counterpart constitute powerful probes of binary evolution, the production sites of heavy elements,…

astro-ph.IM2025

Measuring Type Ia Supernova Angular-Diameter Distances with Intensity Interferometry

A. G. Kim, P. E. Nugent, Xingzhuo Chen +2

This paper investigates the potential of intensity interferometry, based on the Hanbury Brown-Twiss effect, for measuring supernova sizes and distances. Through optimized telescope…

astro-ph.HE2024

An Integral-Based Technique (IBT) to Accelerate the Monte-Carlo Radiative Transfer Computation for Supernovae

Xingzhuo Chen, Lifan Wang, Daniel Kasen

We present an integral-based technique (IBT) algorithm to accelerate supernova (SN) radiative transfer calculations. The algorithm utilizes ``integral packets'', which are calculat…

astro-ph.HE2022

Artificial Intelligence Assisted Inversion (AIAI): Quantifying the Spectral Features of Ni of Type Ia Supernovae

Xingzhuo Chen, Lifan Wang, Lei Hu +1

Following our previous study of Artificial Intelligence Assisted Inversion (AIAI) of supernova analyses (Chen et al. 2020), we train a set of deep neural networks based on the one-…

astro-ph.HE2022★ 2 cited

Using Physics Informed Neural Networks for Supernova Radiative Transfer Simulation

Xingzhuo Chen, David J. Jeffery, Ming Zhong +3

We use physics informed neural networks (PINNs) to solve the radiative transfer equation and calculate a synthetic spectrum for a Type Ia supernova (SN~Ia) SN 2011fe. The calculati…

astro-ph.CO2022★ 20 cited

Constraints on Cosmological Parameters with a Sample of Type Ia Supernovae from JWST

Jia Lu, Lifan Wang, Xingzhuo Chen +7

We investigate the potential of using a sample of very high-redshift () (VHZ) Type Ia supernovae (SNe~Ia) attainable by the James Webb Space Telescope (JWST)…

astro-ph.HE2022★ 24 cited

Spectroscopic Studies of Type Ia Supernovae Using LSTM Neural Networks

Lei Hu, Xingzhuo Chen, Lifan Wang

We present a data-driven method based on long short-term memory (LSTM) neural networks to analyze spectral time series of Type Ia supernovae (SNe Ia). The dataset includes 3091 spe…

astro-ph.IM2021★ 58 cited

Image Subtraction in Fourier Space

Lei Hu, Lifan Wang, Xingzhuo Chen +1

Image subtraction is essential for transient detection in time-domain astronomy. The point spread function (PSF), photometric scaling, and sky background generally vary with time a…

astro-ph.GA2021

Constraining Type Ia Supernova Delay Time with Spatially Resolved Star Formation Histories

Xingzhuo Chen, Lei Hu, Lifan Wang

We present the delay time distribution (DTD) estimates of Type Ia supernovae (SNe~Ia) using spatially resolved SN~Ia host galaxy spectra from MUSE and MaNGA. By employing a groupin…

astro-ph.HE2019★ 12 cited

Artificial Intelligence Assisted Inversion (AIAI) of Synthetic Type Ia Supernova Spectra

Xingzhuo Chen, Lei Hu, Lifan Wang

We generate 100,000 model spectra of Type Ia Supernovae (SNIa) to form a spectral library for the purpose of building an Artificial Intelligence Assisted Inversion (AIAI) al…

astro-ph.HE2018

A New Method to Classify Type IIP/IIL Supernovae Based on their Spectra

Xingzhuo Chen, Shihao Kou, Xuewen Liu

Type IIP and type IIL supernovae (SNe) are defined on their light curves, but the spectrum criteria in distinguishing these two type SNe remains unclear. We propose a new classific…