Radio Identification of Submillimeter Sources in the Hubble Deep Field
作者： E. A. Richards
DOI: 10.1086/311905
关键词: Population 、 Astronomy 、 Galaxy 、 James Clerk Maxwell Telescope 、 Galaxy formation and evolution 、 Observational cosmology 、 Astrophysics 、 Hubble Deep Field 、 Hubble Ultra-Deep Field 、 Redshift 、 Physics 、 Space and Planetary Science 、 Astronomy and Astrophysics
摘要: Determination of the epoch dependent star-formation rate field galaxies is one principal goals modern observational cosmology. Recently, Hughes et al. (1998) using SCUBA instrument on James Clerk Maxwell Telescope, report detection a new population heavily dust enshrouded, star-forming at high redshifts (z > 2), dramatically altering picture galaxy evolution. However, we show that this interpretation must be treated with caution because ambiguities in identification host galaxies. Based our deep, resolution 1.4 GHz obervations Hubble Deep Field, suggest alternate identifications to sub-mm detections. These argue for substantially lower redshift consequential lowering z 2 sub-mm/far infrared luminosity density and global rate.
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