Dependence of the BALQSO fraction on Radio Luminosity

Francesco Shankar, Xinyu Dai, Gregory R. Sivakoff

We find that the fraction of classical Broad Absorption Line quasars (BALQSOs) among the FIRST radio sources in the Sloan Data Release 3, is 20.5^{+7.3}_{-5.9}% at the faintest rad…