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Weichen Wang

3 papers hereh-index 13786 citations23 works total

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author position
  • first author1
  • middle author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
same name
  • Weichen Wang — 2 papers
  • Weichen Wang — 1 paper, h 13

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

most citedUVI colour gradients of 0.4<z<1.4 star-forming main sequence galaxies in CANDELS: dust extinction and star formation profiles

55 citations · 82 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2017★ 27 cited

The Origins of UV-optical Color Gradients in Star-forming Galaxies at z ~ 2: Predominant Dust Gradients But Negligible sSFR Gradients

F. S. Liu, Dongfei Jiang, S. M. Faber +13

The rest-frame UV-optical (i.e., NUV−B) color is sensitive to both low-level recent star formation (specific star formation rate - sSFR) and dust. In this Letter, we extend our p…

astro-ph.GA2017★ 55 cited

UVI colour gradients of 0.4<z<1.4 star-forming main sequence galaxies in CANDELS: dust extinction and star formation profiles

Weichen Wang, S. M. Faber, F. S. Liu +10

This paper uses radial colour profiles to infer the distributions of dust, gas and star formation in z=0.4-1.4 star-forming main sequence galaxies. We start with the standard UVJ-b…

astro-ph.GA2016

The UV-optical Color Gradients in Star-Forming Galaxies at 0.5<z<1.5: Origins and Link to Galaxy Assembly

F. S. Liu, Dongfei Jiang, Yicheng Guo +10

The rest-frame UV-optical (i.e., NUV-B) color index is sensitive to the low-level recent star formation and dust extinction, but it is insensitive to the metallicity. In this Lette…

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