An upper limit to [C II] emission in a z = 5 galaxy
نویسندگان
چکیده
منابع مشابه
An upper limit to [ C II ] emission in a z 5 galaxy
Low-ionization-state far-infrared (FIR) emission lines may be useful diagnostics of star formation activity in young galaxies, and at high redshift may be detectable from the ground. In practice, however, very little is known concerning how strong such line emission might be in the early Universe. We attempted to detect the 158-μm [C II] line from a lensed galaxy at z = 4.926 using the Caltech ...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2005
ISSN: 0035-8711,1365-2966
DOI: 10.1111/j.1365-2966.2005.08837.x