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Max-Planck Institut für Astronomie AGN10 - September 11 th, 2012.

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Presentation on theme: "Max-Planck Institut für Astronomie AGN10 - September 11 th, 2012."— Presentation transcript:

1 Max-Planck Institut für Astronomie AGN10 - September 11 th, 2012

2 How do galaxies and BHs coevolve? M BH L Host ** R inf Black holes BLR Host galaxies

3 How do galaxies and BHs coevolve? What are the properties of a galaxy which hosts a QSO? (feedback, AGN triggering,...)

4 L R BLR M BH = G -1 R BLR v BLR 2 R BLR ~  L  v BLR = f FWHM CIV – MgII – H 

5 0.30.8 Redshift Gain depth through stacking! 340 SDSS images ≈ 1/2 hr 8m class telescope “Population” properties vs. individual objects

6 0.3 0.8 Redshift M BH 5 10 7 2 10 9 15,018 QSOs 446

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11 0.3 0.8 Redshift M BH 5 10 7 2 10 9

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13 r-z z 0.3<z<0.4

14 r-z z 0.4<z<0.5

15 r-z z 0.5<z<0.6

16 r-z z 0.6<z<0.7

17 r-z z 0.7<z<0.8

18 n sersic R eff [kpc]

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25 QSO PSF

26 QSO PSF

27 SFH

28  ≡ M BH /M host increases of a factor ~7 from z=0 to z=3 CIV – MgII – H 


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