Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-25T15:52:55.345Z Has data issue: false hasContentIssue false
  • English
  • Français

Adaptive optics imaging of QSO UM402 field

Published online by Cambridge University Press:  21 March 2013

Y. P. Wang ,
T. Yamada ,
I. Tanaka ,
M. Iye  and
T. Ji
Y. P. Wang
Affiliation:
Key Laboratory of Optical Astronomy, National Astronomical Observatories, CAS
T. Yamada
Affiliation:
Tohoku University, Japan
I. Tanaka
Affiliation:
Subaru telescope, National Astronomical Obs. of Japan
M. Iye
Affiliation:
National Astronomical Obs. of Japan
T. Ji
Affiliation:
Polar Research Institute of China
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present initial results from adaptive optics deep imaging in the Ks-band of QSO UM402 (zem=2.856), with the IRCS camera on Subaru telescope.

Keywords

quasars: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 195
Copyright
Copyright © International Astronomical Union 2013

References

Dunlop, J. S., McLure, R. J.et al., 2003, MNRAS, 340, 1095CrossRefGoogle Scholar
Falomo, R., Treves, A., Kotilainen, J. K.et al., 2008, ApJ, 673, 694CrossRefGoogle Scholar
Guillenmin, P. & Bergeron, J., 1997, A&A 328, 499Google Scholar
Vestergaard, M. & Peterson, B. M. 2006, ApJ, 641, 689CrossRefGoogle Scholar