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Jing Lu (陆晶)

Hi, my name is Jing, pronounced exactly like "Jingle Bell" without the "-gle bell".

Jing Lu

Who I Am

I am an astrophysicist studying the physics of supernovae using data-driven and machine learning approaches. By coincidence, my journey as a scientist has been closely tied to capital cities. I earned my bachelor's degree in Physics from Nanjing Normal University in China, located in Nanjing, the capital of Jiangsu Province and a historic capital of several dynasties. I then moved to the United States to pursue my PhD at Florida State University in Tallahassee, the capital of Florida. Afterward, I became a postdoctoral researcher at Michigan State University in Lansing, the capital of Michigan.

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What I Do

Supernovae are some of the most powerful explosions in the universe. I work on understanding the physical origin of these events by bridging between observations and physical simulations. Over the past decade, I have worked on large-scale data analysis, generative modeling, deep learning, Monte Carlo methods, and Bayesian inference, primarily in Python. My work has led to 40+ publications and 1,000+ citations, and I have contributed to several open-source scientific software projects, including BYOST (developer), SNooPy (contributor), and TARDIS (maintainer).

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My Work

A selection of the publication that I have led spanning peculiar Type Ia supernovae, near-infrared spectral templates, stripped-envelope supernova simulations, and helium detection in Type Ic supernovae. A full publication list can be found in my Google Scholar page.

ASASSN-15hy supernova image

ASASSN-15hy: An Underluminous, Red 03fg-like Type Ia Supernova

Lu et al. (2021) · ApJ 920, 107

ASASSN-15hy belongs to the peculiar "super-Chandrasekhar" 03fg-like subclass of Type Ia supernovae, yet is unusually underluminous and red compared to its groupmates. Optical and near-infrared observations reveal broad light curves, persistent carbon features, and a low silicon velocity. These properties are best explained by a "deflagration core-degenerate" scenario, the secular merger of a white dwarf with the degenerate core of an asymptotic giant branch star, requiring a low-metallicity progenitor.

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Carnegie Supernova Project NIR spectra

Carnegie Supernova Project II: Near-infrared Spectral Diversity and Template of Type Ia Supernovae

Lu et al. (2023) · ApJ 948, 27

We present 339 near-infrared spectra of 98 Type Ia supernovae from the Carnegie Supernova Project II, the largest and most homogeneous NIR spectral dataset of its kind at the time. Using principal component analysis and Gaussian process regression, we construct a spectral template as a function of phase and light-curve shape. The new template reduces systematic K-correction uncertainties by ~90% over previous templates, with the potential of improving cosmological distance measurements that uses type Ia supernovae.

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Stripped-envelope supernova simulations

Physics-driven Explosions of Stripped High-mass Stars: Synthetic Light Curves and Spectra with Broad Light Curves

Lu et al. (2025) · ApJ 979, 148

We compute synthetic light curves and spectra of the explosions of massive (45–120 M☉) Wolf–Rayet stars exploded with physics-driven neutrino-driven models. The resulting broad, faint light curves are marginally consistent with the ~15% of observed stripped-envelope supernovae with broad light curves. We find that even as little as 0.02 M☉ of helium produces persistent He I lines, and that standard ejecta mass estimators can overestimate the true value by up to a factor of 2.6.

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Helium in Type Ic Supernova 2014L

Traces of Helium Detected in Type Ic Supernova 2014L

Lu et al. (2026) · ApJL 1002, L11

Type Ic supernovae are classified by the absence of helium in optical spectra, but whether helium is truly absent or merely spectroscopically hidden remains debated. We trained a deep learning model that emulates the radiative transfer code TARDIS, then apply Bayesian inference to infer the physical properties of SN Ic 2014L's ejecta providing both optical and NIR spectra. We constrain 0.018–0.020 M☉ of helium in its outer ejecta. A Bayesian statistical test confirms the spectra are inconsistent with a helium-free composition, providing direct observational evidence for hidden helium in a Type Ic supernova.

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Jing Lu's CV

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