Dr. Cheng Li

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===== What can you find from this site? =====

Look at [[wiki:about|this page]] if you're interested about myself, and refer to the  [[wiki:research|Research Page]] for a brief introduction to my research and lists of my students/postdocs. My publications are listed on [[wiki:publications|this page]]. My courses are listed on the [[wiki:teaching|Teaching Page]]. You're welcome to [[wiki:contact|Contact]] me, if you're interested to visit and talk with me on my research or courses, but before that you may want to consult my [[wiki:schedule|Weekly Schedule and Travel plan]].

==== Recent research works ====

  * [[https://ui.adsabs.harvard.edu/abs/2024ApJ...964..161M|Measuring Galaxy Abundance and Clustering at High Redshift from Incomplete Spectroscopic Data: Tests on Mock Catalogs]] 
  * [[https://ui.adsabs.harvard.edu/abs/2024ApJ...963...86L|On the Existence, Rareness, and Uniqueness of Quenched H I-rich Galaxies in the Local Universe]] 
  * [[https://ui.adsabs.harvard.edu/abs/2024ApJ...962...51J|Criss-cross Nebula: A Case Study of Shock Regions with Resolved Microstructures at Scales of ∼1000 au]] 
  * [[https://ui.adsabs.harvard.edu/abs/2024ApJ...961..216C|Post-starburst Galaxies in SDSS-IV MaNGA: Two Broad Categories of Evolutionary Pathways]] 
  * [[https://ui.adsabs.harvard.edu/abs/2023ApJ...957...75Z|Mapping Dust Attenuation and the 2175 Å Bump at Kiloparsec Scales in Nearby Galaxies]] 
  * [[https://ui.adsabs.harvard.edu/abs/2023MNRAS.525.1254C|A conditional abundance matching method of extending simulated halo merger trees to resolve low-mass progenitors and subhalos]] 
  * [[https://ui.adsabs.harvard.edu/abs/2023MNRAS.520.1774W|Relating galaxies across different redshift to study galaxy evolution]] 
  * [[https://ui.adsabs.harvard.edu/abs/2023ChPhB..32c9801L|Measuring stellar populations, dust attenuation and ionized gas at kpc scales in 10010 nearby galaxies using the integral field spectroscopy from MaNGA]] 
  * [[https://ui.adsabs.harvard.edu/abs/2023ApJ...944...75M|Galaxy Populations in Groups and Clusters: Evidence for a Characteristic Stellar Mass Scale at M <SUB>∗</SUB> 10<SUP>9.5</SUP> M <SUB>⊙</SUB>]] 
  * [[https://ui.adsabs.harvard.edu/abs/2022ApJ...941...48L|Conditional H I Mass Functions and the H I-to-halo Mass Relation in the Local Universe]]
Dr. Cheng Li

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