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Chenghao Zhu

4 papers hereh-index 318 citations9 works total

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

author position
  • first author1
  • middle author1
  • last author2

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

fields
  • astro-ph.GA4
same name
  • Chenghao Zhu — 6 papers, h 3
  • Chenghao Zhu — 3 papers, h 1
  • Chenghao Zhu — 2 papers, h 3

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

SDSS+JWST Census of Stellar and Nebular Dust Attenuation at z∼0-7: Mass Dependence and Redshift Evolution

Jie Song, Masami Ouchi, Tomokazu Kiyota +3

We present the demography of dust attenuation, including its mass dependence and redshift evolution, using spectroscopic samples of 34,182 SDSS galaxies at z∼0.1 and 863 JWST/…

astro-ph.GA2025

A High Incidence of Mid-infrared Variability in Local Ultraluminous Infrared Galaxies

Shun Hatano, Masatoshi Imanishi, Takanobu Kirihara +3

We explore mid-infrared (MIR) variability in local ultraluminous infrared galaxies (ULIRGs; infrared luminsoity LIR​>1012 L⊙​) utilizing the ∼11 years of photo…

astro-ph.GA2025

Cosmic Himalayas: The Highest Quasar Density Peak Identified in a 10,000 deg2 Sky with Spatial Discrepancies between Galaxies, Quasars, and IGM HI

Yongming Liang, Masami Ouchi, Dongsheng Sun +27

We report the identification of a quasar overdensity in the BOSSJ0210 field, dubbed Cosmic Himalayas, consisting of 11 quasars at z=2.16−2.20, the densest overdensity of quasars…

astro-ph.GA2025

The Physical Origin of Extreme Emission Line Galaxies at High redshifts: Strong {\sc [Oiii]} Emission Lines Produced by Obscured AGNs

Chenghao Zhu, Yuichi Harikane, Masami Ouchi +21

We present deep Subaru/FOCAS spectra for two extreme emission line galaxies (EELGs) at z∼1 with strong {\sc[Oiii]}I^»5007 emission lines, exhibiting equivalent widths (EWs)…

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