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Z. Wang

3 papers hereh-index 218 citations6 works total

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

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
  • Z. Wang — 121 papers, h 9
  • Z. Wang — 73 papers, h 3
  • Z. Wang — 50 papers, h 17
  • Z. Wang — 43 papers
  • Z. Wang — 41 papers, h 3
  • Z. Wang — 39 papers, h 5

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 citedoMEGACat. IX. Chemical Tagging of Omega Centauri Populations with Machine-Learning-Inferred Abundances from the MUSE Spectrograph

2 citations · 2 across the 1 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2026★ 2 cited

oMEGACat. IX. Chemical Tagging of Omega Centauri Populations with Machine-Learning-Inferred Abundances from the MUSE Spectrograph

Z. Wang, A. C. Seth, C. Clontz +14

We present chemical abundance measurements for 7,302 red giant branch stars within the half-light radius (~5') of I¨‰ Centauri (I¨‰ Cen), derived from MUSE spectra using the neur…

astro-ph.GA2024

oMEGACat V: Helium Enrichment in I¨‰ Centauri as a Function of Metallicity

C. Clontz, A. C. Seth, Z. Wang +12

Constraining the helium enhancement in stars is critical for understanding the formation mechanisms of multiple populations in star clusters. However, measuring helium variations f…

astro-ph.GA2024

oMEGACat IV: Constraining Ages of Omega Centauri sub-giant branch stars with HST and MUSE

C. Clontz, A. C. Seth, A. Dotter +13

We present age estimates for over 8100 sub-giant branch (SGB) stars in Omega Centauri (I¨‰ Cen) to study its star formation history. Our large data set, which combines multi-wavel…

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