The emission-line properties of the QSO population at Z approximately 2
We compare the ultraviolet emission-line properties of the three subclasses of the QSO population (radio quiet, flat radio spectrum radio loud, steep radio spectrum radio loud) during the 'QSO epoch' at z approximately 2. Our total sample consists of 79 objects that are well matched in luminosity and redshift, which should allow unbiased comparison of their spectral properties. We confirm recent results that radio-loud objects have, on average, narrower and stronger C IV lambda 1549 and C III)...[Show more]
|Collections||ANU Research Publications|
|Source:||The Astronomical Journal|
|Access Rights:||Open Access|
|1994AJ____108_2016C.pdf||940.64 kB||Adobe PDF|
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