Portrait of Te Han
Astrophysicist & Planet Hunter

Te Han

Ph.D. candidate at UC Irvine building surveys and data tools that reveal how planets grow around stars of every kind. I chase newborn worlds, improve the sensitivity of space missions, and deliver pipelines that the community can rely on.

Irvine, California teh2@uci.edu (805) 280-6544
About

Mapping the next generation of worlds

I’m an astronomer who loves turning huge, messy datasets into clear stories about planets and the stars they orbit. I build tools and methods that help uncover what standard surveys might overlook — from better TESS photometry to new ways of combining transits, radial velocities, and imaging.

I care about making data not just accurate, but useful — for myself and for the broader community. I like solving tricky problems, sharing what I learn, and building things that help others explore how planets form, evolve, and survive around some of the most extreme stars of the galaxy.

Current focus

  • Measuring planet demographics with the GEMS survey and NEIDSpecMatch.
  • Launching SURFSUP to catch the youngest, fastest-spinning stellar hosts.

On deck

  • TWIRL — the TESS White dwarf Investigation of Remnant pLanets, a search for surviving worlds around WDs.
Research

Selected work

Building shared infrastructure for exoplanet discovery while chasing the most revealing planetary systems.

TESS–Gaia Light Curve performance visualization

TESS–Gaia Light Curve: A PSF-based TESS FFI Light-curve Product

Turning raw TESS full-frame images into precision light curves—released as a MAST HLSP that now underpins community time-domain science.

  • Community pipelines
  • Time-domain astronomy
  • Open science
Visualization of TESS radius bias for hundreds of exoplanets

Hundreds of TESS Exoplanets Might Be Larger than We Thought

Revealing a systematic radius bias in the TESS catalog by reanalyzing planets with TGLC light curves, revised stellar parameters, and updated inference.

  • Planet demographics
  • Precision photometry
  • Bias correction
GEMS survey visualization of TOI-5344 b discovery

TOI-5344 b: A Saturn-like Planet Orbiting a Super-solar Metallicity M0 Dwarf

Mapping giant planets around M dwarfs through the GEMS survey, highlighted by the TOI-5344 b discovery that probes formation across the lowest-mass stars.

  • Radial velocities
  • M-dwarf planets
  • Survey design
Spotlight

Recent highlights

Talks, papers, and signals I am excited about right now.

Hundreds of TESS planets might be bigger than we thought

ApJL 2025: uncovering a systematic bias in measured radii using TGLC-informed modeling.

SURFSUP takes the stage

Early SURFSUP findings shared at CoolStars22 and Know Thy Star II, showcasing the youngest rotating systems.

TWIRL takes shape

Preparing the TESS White dwarf Investigation of Remnant pLanets to mine 200-s FFIs for post-main-sequence worlds with machine-learning vetting and TGLC photometry.

CV

Snapshot resume

Prefer the full document? Grab the PDF directly, or open the sections below for quick context.

B.S. in Physics

UC Santa Barbara
Advisor: Timothy Brandt

Ph.D. in Physics

UC Irvine
Advisor: Paul Robertson

Physics Study Room Fellow & Learning Assistant

UC Santa Barbara

2018–2020

Lab Assistant

UC Santa Barbara

2020–2021

Teaching Assistant

UC Irvine

2021–2022

Graduate Student Researcher

UC Irvine

2023–present

Visiting Graduate Student

MIT

2025
Awards & honors
  • Chancellor’s Fellowship, UC Irvine — 2021–2023
  • Highest Honors (Honors at Graduation), UC Santa Barbara — 2017–2020
  • Dean’s Honors (Letters & Science), UC Santa Barbara — 2018–2020
First-author publications
  • TESS–Gaia Light Curve: A PSF-based TESS FFI Light-curve Product, Han & Brandt, AJ 165, 71 (2023). ADS
  • TOI-5344 b: A Saturn-like Planet Orbiting a Super-solar Metallicity M0 Dwarf, Han et al., AJ 167, 4 (2024). ADS
  • NEIDSpecMatch: Stellar Parameter Estimation with NEID Spectra Using an Empirical Library, Han et al., RNAAS 9, 63 (2025). ADS
  • Hundreds of TESS Exoplanets Might Be Larger than We Thought, Han et al., ApJL 988, L4 (2025). ADS
  • SURFSUP: Surveying Ultrafast Rotators For Superyoung Planets, Han et al., In preparation (2025).
  • TESS–Gaia Light Curve: Photometric precision analysis and new functionalities, Han et al., In preparation (2025).
Talks & posters
  • Invited: Caltech/IPAC Lunch Seminar — The radius bias of TESS exoplanets · Apr 2025
  • Invited: TESS Science Talk, MIT (Remote) — TGLC Technical Details · Apr 2024
  • Invited: ExoSoCal 2023, Caltech — TOI-5344 b as a GEMS planet · Dec 2023
  • Invited: TESS Science Talk, MIT — TGLC Methods · Aug 2023
  • Contributed: TESS Science Conference III, MIT — TGLC Performance · Jul 2024
  • Contributed: TESS Mission Update, MIT — GEMS progress · Jun 2023
  • Poster: Know Thy Star, Caltech — SURFSUP highlights · Feb 2025
  • Poster: Cool Stars 22, UC San Diego — SURFSUP early results · Jun 2024
Skills
  • Programming: Python
  • Research & data: Ground-based telescope planning & observing (Shane 3-m, HET, WIYN), Exoplanet modeling, Radial velocity analysis, Light curve analysis, Spectra analysis, 3D modeling
  • Technical tools: Deep space astrophotography, DSLR/drone photography, 3D printing
  • Communication: Public speaking, Teaching, Science writing, TEDx organizer (TEDxHarbinNo3HighSchool)
  • Languages: Chinese (Native), English (Fluent)
Contact

Let's collaborate

Have an idea, a dataset, or a mission concept? I would love to hear about it.

Email: teh2@uci.edu

Phone: (805) 280-6544

Office: FRH 2156, Department of Physics & Astronomy, UC Irvine