Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Supernova, Astronomy, Galaxy, and Light curve.
Kilonova Constraints for the LIGO/Virgo/KAGRA Neutron Star Merger Candidate S250206dm: GW-MMADS Observations
JWST Observations of SN 2024ggi. I. Interpretation and Model Comparison of the Type II Supernova 2024ggi at 55 Days past Explosion
An axisymmetric shock breakout indicated by prompt polarized emission from the type II supernova 2024ggi
Carnegie Supernova Project I and II: Measurements of H <sub>0</sub> Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae*
ASASSN-15LH: A SUPERLUMINOUS ULTRAVIOLET REBRIGHTENING OBSERVED by SWIFT and HUBBLE
Ground-based and JWST Observations of SN 2022pul. II. Evidence from Nebular Spectroscopy for a Violent Merger in a Peculiar Type Ia Supernova
JWST MIRI/Medium Resolution Spectrograph (MRS) Observations and Spectral Models of the Underluminous Type Ia Supernova 2022xkq
A JWST Medium-resolution MIRI Spectrum and Models of the Type Ia Supernova 2021aefx at +415 days
The nature of an ultra-faint galaxy in the cosmic dark ages seen with JWST
A shock flash breaking out of a dusty red supergiant
Early Time Spectropolarimetry of the Aspherical Type II Supernova SN 2023ixf
JWST's PEARLS: Transients in the MACS J0416.1−2403 Field
A JWST Near- and Mid-infrared Nebular Spectrum of the Type Ia Supernova 2021aefx
JWST Low-resolution MIRI Spectral Observations of SN 2021aefx: High-density Burning in a Type Ia Supernova
Ground-based and JWST Observations of SN 2022pul. I. Unusual Signatures of Carbon, Oxygen, and Circumstellar Interaction in a Peculiar Type Ia Supernova
JWST’s PEARLS: Dust Attenuation and Gravitational Lensing in the Backlit-galaxy System VV 191
The core normal Type Ia supernova 2019np – an overall spherical explosion with an aspherical surface layer and an aspherical 56Ni core
JWST NIRCam Observations of SN 1987A: Spitzer Comparison and Spectral Decomposition
SN 2021fxy: mid-ultraviolet flux suppression is a common feature of Type Ia supernovae
Bump Morphology of the CMAGIC Diagram
Spectropolarimetry of the Type IIP supernova 2021yja: an unusually high continuum polarization during the photospheric phase
An Independent Determination of the Distance to Supernova SN 1987A by Means of the Light Echo AT 2019xis
JWST PEARLS. Prime Extragalactic Areas for Reionization and Lensing Science: Project Overview and First Results
JWST's PEARLS: Bright 1.5–2.0 μm Dropouts in the Spitzer/IRAC Dark Field
Using 1991T/1999aa-like Type Ia Supernovae as Standardizable Candles
Spectropolarimetry of the Type Ia SN 2019ein rules out significant global asphericity of the ejecta
The interaction of supernova 2018evt with a substantial amount of circumstellar matter – An SN 1997cy-like event
Spectropolarimetry of the Thermonuclear Supernova SN 2021rhu: High Calcium Polarization 79 Days after Peak Luminosity
An imaging polarimetry survey of Type Ia supernovae: are peculiar extinction and polarization properties produced by circumstellar or interstellar matter?
The Interaction of Supernova 2018evt with a Substantial Amount of Circumstellar Matter -- An SN1997cy-like Event