High-redshift quasar host galaxies with adaptive optics

Free access article

Issue		A&A Volume 439, Number 2, August IV 2005


Page(s)		497 - 512
Section		Extragalactic astronomy
DOI		http://dx.doi.org/10.1051/0004-6361:20041305

A&A 439, 497-512 (2005)
DOI: 10.1051/0004-6361:20041305

High-redshift quasar host galaxies with adaptive optics

B. Kuhlbrodt^{1, 2}, E. Örndahl^{3, 4}, L. Wisotzki^{1, 5} and K. Jahnke^{1, 2}

¹ Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
² Hamburger Sternwarte, Gojenbergsweg 112, 21029 Hamburg, Germany
³ Tuorla Observatory, University of Turku, Väisäläntie 20, 21500 Piikkiö, Finland
e-mail: evaorn@utu.fi
⁴ Department of Astronomy and Space Physics, Uppsala University, Box 515, 751 20 Uppsala, Sweden
⁵ Institut für Physik, Potsdam University, Am Neuen Palais 10, 14469 Potsdam, Germany

(Received 17 May 2004 / Accepted 21 April 2005 )

Abstract
We present K band adaptive optics observations of three high-redshift ( $z \sim 2.2$ ) high-luminosity quasars, all of which were studied for the first time. We also observed several point spread function (PSF) calibrators, non-simultaneously because of the small field of view. The significant temporal PSF variations on timescales of minutes inhibited a straightforward scaled PSF removal from the quasar images. Characterising the degree of PSF concentration by the radii encircling 20% and 80% of the total flux, respectively, we found that even under very different observing conditions the r₂₀ vs. r₈₀ relation varied coherently between individual short exposure images, delineating a well-defined relation for point sources. Placing the quasar images on this relation, we see indications that all three objects were resolved. We designed a procedure to estimate the significance of this result, and to estimate host galaxy parameters, by reproducing the statistical distribution of the individual short exposure images. We find in all three cases evidence for a luminous host galaxy, with a mean absolute magnitude of M_R = -27.0 and scale lengths around ~4-12 kpc. Together with a rough estimate of the central black hole masses obtained from C $\:$ IV line widths, the location of the objects on the bulge luminosity vs. black hole mass relation is not significantly different from the low-redshift regime, assuming only passive evolution of the host galaxy. Corresponding Eddington luminosities are $L_{\rm nuc}/L_{\rm Edd} \sim 0.1$ -0.6.

Key words: instrumentation: adaptive optics -- quasars: general -- galaxies: fundamental parameters -- galaxies: high-redshift

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