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Tiancheng Yang

11 papers hereh-index 331 citations12 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author8
  • last author1

Across the 10 of 11 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA10
  • astro-ph.CO1
same name
  • Tiancheng Yang — 2 papers, h 2
  • Tiancheng Yang — 2 papers, h 2
  • Tiancheng Yang — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20232026
most citedJWST/MIRI reveals the true number density of massive galaxies in the early Universe

20 citations · 62 across the 11 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.CO2026

A cosmic filament catalog for COSMOS-Web Data Release 1 across 0.5 < z < 3.5

Qiaoyang Hao, Tao Wang, Weishan Zhu +4

Cosmic filaments represent the environments in which most galaxies form and evolve. However, the spatial distribution of filaments and the link between galaxy properties and their…

astro-ph.GA2026★ 2 cited

A Bending in the Size-mass Relation of Star-forming Galaxies across 0.5<z<6.0 at a Critical Stellar Mass of 1010M⊙​ Revealed by JWST

Longyue Chen, Tao Wang, Hanwen Sun +12

We investigate the rest-frame optical size-stellar mass relation of galaxies at 0.5<z<6.0 using deep JWST/NIRCam and MIRI imaging from the PRIMER survey. We find that star-formin…

astro-ph.GA2026★ 2 cited

ULTIMATE-deblending I. A 50-band Ultraviolet to Mid-infrared Photometric Catalog Combining Space- and Ground-based Data in the JWST/PRIMER survey

Hanwen Sun, Tao Wang, Ke Xu +16

Our understanding of the early Universe has long been limited by biased galaxy samples selected through various color criteria. With deep JWST infrared imaging, mass-complete galax…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.