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Investigating the AGN-Merger Connection at z~2 with CANDELS Background Evolution of AGN Fueling Modes -2 z = 0.1 z = 0.2 z = 0.5 -4 -6 log 10 [ (M B )] [Mpc -3 mag -1 ] -8 -2 z = 0.8 z = 1.0 z = 2.0 -4 -6 -8 -16 -20 -24 -28


  1. Investigating the AGN-Merger Connection at z~2 with CANDELS

  2. Background

  3. Evolution of AGN Fueling Modes -2 z = 0.1 z = 0.2 z = 0.5 -4 -6 log 10 [ φ (M B )] [Mpc -3 mag -1 ] -8 -2 z = 0.8 z = 1.0 z = 2.0 -4 -6 -8 -16 -20 -24 -28 -16 -20 -24 -28 -16 -20 -24 -28 M B Hopkins ¡& ¡Hernquist ¡(2006) ¡

  4. Wide Field Camera 3 Rest-Frame UV Rest-Frame Optical V z Y J H z=1.55

  5. X-ray AGN in GOODS-S ERS II CANDELS Deep CANDELS Wide Soft Source Hard Source

  6. X-ray Luminosity Distribution

  7. Host Morphologies Spheroids Disks Mergers / Interactions F160W (H) F775W (i) Rest-Frame UV Rest-Frame Optical V z Y J H z=1.55

  8. Visual Classifications

  9. Mass-Matched Control Sample

  10. Classification Results

  11. AGN Still Favor Spheroids All Disks All Spheroids Control AGN Pure Disks Disk + Spheroid Pure Spheroids (Disk with Bulge)

  12. Standard Caveats Spheroids Disks Mergers / Interactions F160W (H) F775W (i)

  13. Morphologies of Compton Thick AGN

  14. Constraints on Time Delay Caveat Spheroids Disks Mergers / Interactions F160W (H) F775W (i)

  15. Implications for AGN Fueling Models 10 -3 -2 log 10 [ φ (M B )] [Mpc -3 mag -1 ] z = 2.0 1.5 < z < 2.0 10 -4 d Φ /d(log L X ) -4 10 -5 -6 10 -6 10 -7 50% 50% -8 Disks Disks 10 -8 41 42 43 44 45 46 -16 -20 -24 -28 log(L X / erg s -1 ) M B

  16. Alternatives to Mergers BLACK HOLE GROWTH AND AGN OBSCURATION BY INSTABILITY-DRIVEN INFLOWS IN HIGH-REDSHIFT DISK GALAXIES FED BY COLD STREAMS Fr´ ed´ eric Bournaud CEA, IRFU, SAp, 91191 Gif-sur-Yvette, France; frederic.bournaud@cea.fr Avishai Dekel Racah Institute of Physics, The Hebrew University, Jerusalem 91904, Israel; dekel@phys.huji.ac.il

  17. Clumpy Disks Among AGN Hosts 4000A (rest) 4000A (rest) 4000A (rest) 4000A (rest) z = 0.5 - 0.8 F775W z = 0.5 - 0.8 F775W z = 0.5 - 0.8 F775W z = 0.5 - 0.8 F775W z = 0.8 - 1.2 F850LP z = 0.8 - 1.2 F850LP z = 0.8 - 1.2 F850LP z = 1.2 - 1.9 F125W z = 1.2 - 1.9 F125W z = 1.9 - 2.5 F160W

  18. Clumpy Disks Among AGN Hosts

  19. Clumpy Disks Among AGN Hosts

  20. Clumpy Disks Among AGN Hosts

  21. Clumpy Disks Among AGN Hosts

  22. Alternatives to Mergers Spheroids Disks Mergers / Interactions F160W (H) F775W (i)

  23. Conclusions Spheroids Disks Mergers / Interactions F160W (H) F775W (i)

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