ALMA detection of [C ii] 158μm emission from a strongly lensedz= 2.013 star-forming galaxy

2015/02/12 by D. Schaerer, F. Boone, T. Jones +9 · 25 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Cosmic dust #Emission spectrum #Galactic nuclei #Galaxies: Formation, Evolution, Phenomena #Galaxy #Interstellar medium #Radio galaxy #Star formation #Ultraviolet astronomy #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201425542

published in Astronomy and Astrophysics 576, L2 (EDP Sciences) · 5 pages, 4 figures. Accepted for publication in Astronomy & Astrophysics, Letters

arxiv created 2015/02/12 · openalex publication_date 2015/02/20 · arxiv updated 2015/03/18 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. Our objectives are to determine the properties of the interstellar medium (ISM) and of star formation in typical star-forming galaxies at high redshift.

Citations

• TheHerschelLensing Survey (HLS): Overview
• The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types
• Enhanced [CII] emission in az = 4.76 submillimetre galaxy

Cited by

• Planck’s Dusty GEMS
• Observations of [OI]63 μm line emission in main-sequence galaxies at z ∼ 1.5