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C. Shu

5 papers hereh-index 7173 citations7 works total

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

author position
  • first author1

Across the 1 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph5
same name
  • C. Shu — 4 papers, h 12
  • C. Shu — 2 papers, h 4
  • C. Shu — 2 papers, h 3
  • C. Shu — 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

activity
20052008
most citedAEGIS: Infrared Spectroscopy of An Infrared Luminous Lyman Break Galaxy at z=3.01

27 citations · 70 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph2008★ 16 cited

Comparisons between isothermal and NFW mass profiles for strong-lensing galaxy clusters

Chenggang Shu, Binglu Zhou, Matthias Bartelmann +3

While both isothermal and NFW-based mass models for galaxy clusters are widely adopted in strong-lensing studies, they cannot easily be distinguished based solely on observed posit…

astro-ph2006★ 27 cited

AEGIS: Infrared Spectroscopy of An Infrared Luminous Lyman Break Galaxy at z=3.01

J. -S. Huang, D. Rigopoulou, C. Papovich +16

We report the detection of rest--frame 6.2 and 7.7 \micron emission features arising from Polycyclic Aromatic Hydrocarbons (PAH) in the Spitzer/IRS spectrum of an infrared-luminous…

astro-ph2005

Infrared Luminous Lyman Break Galaxies: A Population that Bridges LBGs and SCUBA Galaxies

J. -S. Huang, D. Rigopoulou, S. P. Willner +12

A deep mid- and far-infrared survey in the Extended Groth Strip (EGS) area gives 3.6 to 8\micron flux densities or upper limits for 253 Lyman Break Galaxies (LBGs). The LBGs are a…

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