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Bright [CII] 158m emission in a quasar host galaxy at
E. Bañados, R. Decarli, F. Walter +3
The [CII] 158m fine-structure line is known to trace regions of active star formation and is the main coolant of the cold, neutral atomic medium. In this \textit{Letter}, we rep…
Constraining the radio-loud fraction of quasars at z>5.5
E. Bañados, B. P. Venemans, E. Morganson +18
Radio-loud Active Galactic Nuclei at z~2-4 are typically located in dense environments and their host galaxies are among the most massive systems at those redshifts, providing key…
The identification of z-dropouts in Pan-STARRS1: three quasars at 6.5<z<6.7
B. P. Venemans, E. Bañados, R. Decarli +30
Luminous distant quasars are unique probes of the high redshift intergalactic medium (IGM) and of the growth of massive galaxies and black holes in the early universe. Absorption d…