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A DIRECT MEASUREMENT OF THE LINEAR BIAS OF MID-INFRARED-SELECTED QUASARS AT <i>z</i> โ 1 USING COSMIC MICROWAVE BACKGROUND LENSING
We measure the cross-power spectrum of the projected mass density as traced by the convergence of the cosmic microwave background lensing field from the South Pole Telescope (SPT) and a sample of Type 1 and 2 (unobscured and obscured) quasars at ใzใ โผ 1 selected with the Wide-field Infrared Survey โฆ