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    • A Direct Measurement of the Linear Bias of Mid-infrared-selected Quasars at z ap 1 Using Cosmic Microwave Background Lensing 

      Geach, J.~E.; Hickox, R.~C.; Bleem, L.~E.; Brodwin, M.; Holder, G.~P.; Aird, K.~A.; Benson, B.~A.; Bhattacharya, S.; Carlstrom, J.~E.; Chang, C.~L.; Cho, H.-M.; Crawford, T.~M.; Crites, A.~T.; de Haan, T.; Dobbs, M.~A.; Dudley, J.; George, E.~M.; Hainline, K.~N.; Halverson, N.~W.; Holzapfel, W.~L.; Hoover, S.; Hou, Z.; Hrubes, J.~D.; Keisler, R.; Knox, L.; Lee, A.~T.; Leitch, E.~M.; Lueker, M.; Luong-Van, D.; Marrone, D.~P.; McMahon, J.~J.; Mehl, J.; Meyer, S.~S.; Millea, M.; Mohr, J.~J.; Montroy, T.~E.; Myers, A.~D.; Padin, S.; Plagge, T.; Pryke, C.; Reichardt, C.~L.; Ruhl, J.~E.; Sayre, J.~T.; Schaffer, K.~K.; Shaw, L.; Shirokoff, E.; Spieler, H.~G.; Staniszewski, Z.; Stark, A.~A.; Story, K.~T.; van Engelen, A.; Vanderlinde, K.; Vieira, J.~D.; Williamson, R.; Zahn, O. (2013-10-20)
      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 ...