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Bo-Yuan Liu

4 papers hereh-index 00 citations0 works total

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

author position
  • middle author2
  • last author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
same name
  • Bo-Yuan Liu — 2 papers, h 0
  • Bo-Yuan Liu — 2 papers, h 0
  • Bo-Yuan Liu — 1 paper, h 0

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

collaborators

4 papers

astro-ph.GA2026

LATED: JWST integral field spectroscopy of a galaxy caught in chemical infancy at z=4.8 behind Abell 2744

Mingyu Li, Roberto Maiolino, Zheng Cai +26

When Population III (Pop III) star formation ended remains an open question. LATED-1 is an intrinsically faint (MUV​=−16.15) Lyα emitter at z=4.80 revealed by VLT/MU…

astro-ph.GA2026

LATED: Lyα-anchored photometric selection of candidate metal-free and extremely metal-poor star formation from the end of reionisation to cosmic noon

Mingyu Li, Zheng Cai, Roberto Maiolino +24

Cosmological simulations allow a low-level tail of Population III (Pop III) star formation to persist to z=2−6. Spectroscopic confirmation is expensive, so an efficient photometr…

astro-ph.GA2026

Pebbles to Gems: Intermediate-mass black holes in the first star clusters

Benedetta Mestichelli, Manuel Arca Sedda, Marta Volonteri +9

The rapid assembly of supermassive black holes (SMBHs) observed at z≳7 requires efficient seeding mechanisms in the early Universe. Population III (Pop. III) star clusters…

astro-ph.GA2025

Mass distribution of Pop III star clusters: A-SLOTH predictions for JWST observability

Veronika Lipatova, Simon C. O. Glover, Ralf S. Klessen +1

This study aims to model the expected luminosities of the first four Balmer-series transitions from Pop.\,III star-forming halos and assess their detectability with JWST/NIRSpec ac…

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