Di Li
Tsinghua University, National Astronomical Observatories Chinese Academy of Sciences, Cornell University
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Astrophysics and Star Formation Studies · Pulsars and Gravitational Waves Research · Galaxies: Formation, Evolution, Phenomena
About
Dr. Li, a radio astronomer, currently a Chair professor of Tsinghua University and the Chief Scientist of the FAST telescope (former) operated by the NAOC. He won the Marcel Grossman Award “For his groundbreaking contributions to the scientific definition of the most sensitive radio telescope and his numerous innovations in characterizing the dynamic universe”. He pioneered several observing and data analysis techniques, including HI narrow self-absorption (HINSA),which facilitates precise measurements of interstellar magnetic field that was firstly published on the cover of Nature. Dr. Li has (co-)led multiple discoveries, including the first detection of interstellar molecular oxygen, the largest set of fast radio burst (FRB) events, the slowest pulsar in globular clusters, etc. He proposed and implemented a novel high-cadence-CAL technique that multiplied the survey efficiency of FAST. He has published more than 300 peer-reviewed journal articles, including 6 on Nature and 2 on Science. He took on many leading and/or advisory roles in national and international organizations, including the Steering Committee of Australia Telescope National Facility (ATNF), the Science and Engineering Advisory Committee of the Square Kilometer Array (SKA), and the advisory panel of the Breakthrough Listen initiative.
Employment
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Tsinghua University Chair Professor2024 - Present
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National Astronomical Observatories Chinese Academy of Sciences Chief Scientist2012 - Present
Education
Projects & Funding
Projects & funding information is unavailable.
Publications (886)
- Fast Radio Bursts Associated with Persistent Radio Sources Prefer Hydrogen-poor Superluminous Supernova Host Environments Save
- FAST Observations of Filamentary and Compact H i Structure in the Magellanic Stream IV Field Save
- A High-Galactic-altitude Scattering Screen: Scintillation from Globular Cluster Pulsar M53A Save
- Trace the Self-gravitating Gas Using CO Isotopologues Save
- ALOHA IRDCs molecular line follow-up Save
- Constraining the Anisotropy of the Galactic Halo with Fast Radio Burst Dispersion Measures: A Two-point Correlation Analysis Save
- Identifying the principal mechanism of star formation feedback Save
- Local constraints on alcohol–thioalcohol analogs in G35.2N Save
- Molecule-dependent abundance behavior of oxygen-bearing complex organics in high-mass star-forming regions: A uniform 50-source survey Save
- Indication for Decreasing Dispersion Measure in the Population of Repeating Fast Radio Bursts and Connection to Young Supernova Remnant Expansion Save
- Divergent Evolution of Radial Metallicity Gradients in the Thin and Thick Disks of the Milky Way Save
- Interstellar Dust-catalyzed Hydrogen Formation Enabled by Nuclear Quantum Effects Save
- Scintillation of the First-known Pulsar Planetary System Save
- A HINSA view of cosmic-ray ionization in IC 348 and NGC 1333: Evidence for a strong low-energy cosmic-ray disparity Save
- Anomalously high deuterium fractionation in a galactic translucent cloud: A challenge to chemical models Save
- Gravitational wave radiation from rapidly deformed post-merger neutron star: perspective for the Milky way detection by LIGO-Virgo-KAGRA Save
- Star Formation Drives Production of Low-energy Cosmic Rays Save
- Pulsed radio emission from a central compact object Save
- The Real and Pseudo Dispersion Measures of FRB 20220912A Save
- Flux Variations of Fast Radio Bursts and Their Persistent Radio Sources: Evidence for a Shared Progenitor Save