Simple stellar population modelling of low S/N galaxy spectra and quasar host galaxy applications

To study the effect of supermassive black holes (SMBHs) on their host galaxies it is important to study the hosts when the SMBH is near its peak activity. A method to investigate the host galaxies of high luminosity quasars is to obtain optical spectra at positions offset from the nucleus where the...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2015-02, Vol.447 (2), p.1638-1660
Hauptverfasser:	Mosby, G., Tremonti, C. A., Hooper, E. J., Wolf, M. J., Sheinis, A. I., Richards, J. W.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Black holes Diffusion Luminosity Modelling Quasars Recovering Spectra Star & galaxy formation Stellar populations Symbols
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