He Sun (0000-0003-1526-6787)

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He Sun is an assistant professor in the National Biomedical Imaging Center (NBIC) at Peking University. His research primarily focuses on computational imaging and adaptive optics, which tightly integrates optics, control, signal processing and machine learning to design more capable scientific imaging instruments. Prior to starting at Peking University, He was a postdoctoral researcher and Amazon AI4Science Fellow at California Institute of Technology. He obtained his Ph.D. from Princeton University in 2019 and his bachelor’s degree from Peking University in 2014. His past work has contributed to interdisciplinary science missions, including the Event Horizon Telescope for black hole interferometric imaging and space telescope missions for exoplanet direct imaging.

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Peking University: Beijing, CN

2022-05 to present | Assistant Professor (National Biomedical Imaging Center)

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He Sun

https://orcid.org/0000-0003-1526-6787

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Employment (2)

Peking University: Beijing, CN

California Institute of Technology: Pasadena, CA, US

Education and qualifications (3)

Princeton University: Princeton, NJ, US

Peking University: Beijing, Beijing, CN

University of Maryland at College Park: College Park, MD, US

Works (46)

Deep learning-assisted analysis of single molecule dynamics from liquid-phase electron microscopy

Discovering Structure From Corruption for Unsupervised Image Reconstruction

Image Reconstruction without Explicit Priors

Polarimetric Geometric Modeling for mm-VLBI Observations of Black Holes

Recovering a Molecule's 3D Dynamics from Liquid-phase Electron Microscopy Movies

Filamentary structures as the origin of blazar jet radio variability

A universal power-law prescription for variability from synthetic images of black hole accretion flows

Characterizing and mitigating intraday variability: reconstructing source structure in accreting black holes with mm-VLBI

First Sagittarius A* Event Horizon Telescope results. I. The shadow of the supermassive black hole in the center of the Milky Way

First Sagittarius A* Event Horizon Telescope Results. II. EHT and Multi-wavelength Observations, Data Processing, and Calibration

First Sagittarius A* event horizon telescope results. III. Imaging of the galactic center supermassive black hole

First Sagittarius A* Event Horizon Telescope results. IV. Variability, morphology, and black hole mass

First Sagittarius A* event horizon telescope results. V. Testing astrophysical models of the galactic center black hole

First Sagittarius A* event horizon telescope results. VI. Testing the black hole metric

Millimeter Light Curves of Sagittarius A* Observed during the 2017 Event Horizon Telescope Campaign

Selective dynamical imaging of interferometric data

The filamentary internal structure of the 3C279 blazar jet

The variability of the black hole image in M87 at the dynamical timescale

α-deep Probabilistic Inference (α-DPI): Efficient Uncertainty Quantification from Exoplanet Astrometry to Black Hole Feature Extraction

Bernoulli generalized likelihood ratio test for signal detection from photon counting images

Broadband Multi-wavelength Properties of M87 during the 2017 Event Horizon Telescope Campaign

Constraining the Orbit and Mass of epsilon Eridani b with Radial Velocities, Hipparcos IAD-Gaia DR2 Astrometry, and Multiepoch Vortex Coronagraphy Upper Limits

Constraints on black-hole charges with the 2017 EHT observations of M87

Data-driven subspace predictive control of adaptive optics for high-contrast imaging

Data-driven subspace predictive control: lab demonstration and future outlook

Deep probabilistic imaging: Uncertainty quantification and multi-modal solution characterization for computational imaging

End-to-end sequential sampling and reconstruction for mr imaging

Exoplanet detection in starshade images

First M87 event horizon telescope results. VII. Polarization of the ring

First M87 event horizon telescope results. VIII. Magnetic field structure near the event horizon

Polarimetric properties of Event Horizon Telescope targets from ALMA

The polarized image of a synchrotron-emitting ring of gas orbiting a black hole

A sequential generalized likelihood ratio test for signal detection from photon counting images

Efficient wavefront sensing for space-based adaptive optics

Learning a probabilistic strategy for computational imaging sensor selection

High-contrast integral field spectrograph (HCIFS): multi-spectral wavefront control and reduced-dimensional system identification

Learning heuristic functions for mobile robot path planning using deep neural networks

Modern wavefront control for space-based exoplanet coronagraph imaging

Sequential generalized likelihood ratio test for planet detection with photon-counting mode

The high-contrast spectroscopy testbed for segmented telescopes (HCST): new wavefront control demonstrations

First light of the high contrast integral field spectrograph (hcifs)

Identification and adaptive control of a high-contrast focal plane wavefront correction system

Neural network control of the high-contrast imaging system

Identification of the focal plane wavefront control system using EM algorithm

Improved high-contrast wavefront controllers for exoplanet coronagraphic imaging systems

Modified deformable mirror stroke minimization control for direct imaging of exoplanets