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Max-Planck Institut für Astronomie
Seeing the invisibleQuasar host galaxies from SDSS stacked imagesRoberto Decarli, Stefano Zibetti
AGN10 - September 11th, 2012
Black holes and host galaxies
• How do galaxies and BHs coevolve?
Gultekin et al. (2009)M
BH
MB
HLHost
s*Rinf
Blackholes
BLR
Host galaxies
• How do galaxies and BHs coevolve?
• What are the properties of a galaxy which hosts a QSO?(feedback, AGN triggering, ...)
Fabian et al. (2003)
Black holes and host galaxies
QSO host galaxies
0.3 0.8Redshift
Gain depth through stacking!
340 SDSS images ≈ 1/2 hr 8m class telescope
“Population” properties vs. individual objects
Decarli & Zibetti (in prep)
Stack of the quasars
Stack of the ref.stars
DifferenceMax PSF subtraction
Max PSF + fit galfit
galfit (residuals) galfit (residuals,different scale)
Residuals: ~ 1% signal
ConclusionsOur stacking analysis on SDSS images allowed us to:
• directly measure the SED of QSO host galaxies with unprecedented accuracy in 4 bands
• locate QSO hosts in the color-mag plane up to z=0.8=> QSO host galaxies are the bluest
galaxies at given luminosity & redshift
• derive structural parameters (nsersic, Reff) for QSO host galaxies in multiple bands
• infer reliable stellar masses => first MBH – Mhost relation at z>0
Decarli & Zibetti (in prep)
Objects rejected in the jackknife analysis
Stack of the quasars
Stack of the ref.stars
Difference